This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj
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 09 07.1843 2461290.6843 10.99 03:33:09.83 +43:31:03.9
151.47786 -10.21104 galactic Per Second-epoch detections are separated by 1.4" and 7.3 pix
The object was found in VSX 1" Vend272
Type: SR
# Max. Min./Amp. JD0 Period
10.500 R1 10.800 R1 2451549.00000 67.600000000000 M3
The object was not found in astcheck.
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:09.83 +43:31:03.9: 11.88 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:09.83 +43:31:03.9: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 33 09.83 +43 31 03.9 11.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Vend272,2461290.6843,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
Vend272 20260907.1843 10.99CV 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 09 07.1843 2461290.6843 11.34 03:34:29.36 +43:36:01.8
151.62566 -10.00285 galactic Per Second-epoch detections are separated by 0.6" and 7.3 pix
The object was found in VSX14" Gaia DR3 238555750779170304
Type: ROT
# Max. Min./Amp. JD0 Period
14.990 G 15.020 G 3.594920000000 G
ATTENTION: measured mag 11.34 is 3.7 mag brighter than the VSX record maximum brightness 14.99 - 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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:29.36 +43:36:01.8: 12.24 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:29.36 +43:36:01.8: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 34 29.36 +43 36 01.8 11.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238555750779170304,2461290.6843,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238555750779170304 20260907.1843 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.62 03:37:10.34 +44:06:13.9
151.71757 -9.31067 galactic Per Second-epoch detections are separated by 0.5" and 7.1 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 | Gaia DR3 238592545759641088 | 03:37:10.32 +44:06:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.742+/-0.026 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:37:10.34 +44:06:13.9: 12.49 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:37:10.34 +44:06:13.9: 12.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 37 10.34 +44 06 13.9 11.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238592545759641088,2461290.6843,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238592545759641088 20260907.1843 11.62CV 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 09 07.1843 2461290.6843 11.63 03:34:36.64 +43:15:08.9
151.85249 -10.27072 galactic Per Second-epoch detections are separated by 0.8" and 7.3 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 | Gaia DR3 238266716660188800 | 03:34:36.64 +43:15:09.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.470+/-0.033 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:36.64 +43:15:08.9: 12.55 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:36.64 +43:15:08.9: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 34 36.64 +43 15 08.9 11.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238266716660188800,2461290.6843,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238266716660188800 20260907.1843 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.75 03:33:59.53 +43:26:09.2
151.65028 -10.18895 galactic Per Second-epoch detections are separated by 0.8" and 7.2 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 | 03:33:59.53 +43:26:09.2 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.384+/-0.028 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:59.53 +43:26:09.2: 12.64 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:59.53 +43:26:09.2: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 33 59.53 +43 26 09.2 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 11.75CV 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 09 07.1843 2461290.6843 11.76 03:35:38.55 +43:16:00.6
151.99764 -10.14787 galactic Per Second-epoch detections are separated by 2.1" and 7.0 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 | Gaia DR3 238357082771673600 | 03:35:38.57 +43:16:01.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.463+/-0.028 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:35:38.55 +43:16:00.6: 12.68 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:35:38.55 +43:16:00.6: 12.69 +/- 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!
TCP 2026 09 07.1843* 03 35 38.55 +43 16 00.6 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238357082771673600,2461290.6843,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238357082771673600 20260907.1843 11.76CV 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 09 07.1843 2461290.6843 11.91 03:27:39.05 +42:10:18.4
151.43400 -11.89353 galactic Per Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 238006746580983424 | 03:27:39.13 +42:10:19.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.679+/-0.030 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:27:39.05 +42:10:18.4: 12.83 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:27:39.05 +42:10:18.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 27 39.05 +42 10 18.4 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238006746580983424,2461290.6843,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238006746580983424 20260907.1843 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.82 03:29:33.66 +42:34:46.1
151.48906 -11.35710 galactic Per Second-epoch detections are separated by 1.3" and 7.3 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 | 03:29:33.66 +42:34:46.1 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.487+/-0.034 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:29:33.66 +42:34:46.1: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:29:33.66 +42:34:46.1: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 29 33.66 +42 34 46.1 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.89 03:28:53.69 +42:31:36.0
151.41791 -11.47100 galactic Per Second-epoch detections are separated by 1.3" and 7.3 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 | ATO J052.2086+42.5278 | 03:28:53.69 +42:31:36.0 (user input) | CBF (ATLAS) | (ATLAS) | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.633+/-0.031 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:28:53.69 +42:31:36.0: 12.87 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:28:53.69 +42:31:36.0: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 28 53.69 +42 31 36.0 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J052.2086+42.5278,2461290.6843,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 J052.2086+42.5278 20260907.1843 11.89CV 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 09 07.1843 2461290.6843 11.90 03:40:44.47 +45:01:36.1
151.67026 -8.19109 galactic Per Second-epoch detections are separated by 1.4" and 7.0 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 J055.1855+45.0269 | 03:40:44.47 +45:01:36.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.295+/-0.030 (F)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:40:44.47 +45:01:36.1: 12.91 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:40:44.47 +45:01:36.1: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 40 44.47 +45 01 36.1 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J055.1855+45.0269,2461290.6843,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 J055.1855+45.0269 20260907.1843 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.92 03:39:37.87 +45:04:49.7
151.47957 -8.26661 galactic Per Second-epoch detections are separated by 0.5" and 7.1 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 | 03:39:37.87 +45:04:49.7 (user input) | T | P | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.151+/-0.031 (F)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:39:37.87 +45:04:49.7: 12.92 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:39:37.87 +45:04:49.7: 12.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 39 37.87 +45 04 49.7 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.95 03:37:07.16 +44:30:43.0
151.46331 -8.98878 galactic Per Second-epoch detections are separated by 2.1" and 7.2 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 J054.2690+44.5219 | 03:37:08.32 +44:31:19.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.867+/-0.030 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:37:07.16 +44:30:43.0: 12.94 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:37:07.16 +44:30:43.0: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 37 07.16 +44 30 43.0 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J054.2690+44.5219,2461290.6843,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 J054.2690+44.5219 20260907.1843 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.99 03:43:26.70 +45:44:00.1
151.61630 -7.34142 galactic Per Second-epoch detections are separated by 0.9" and 7.0 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 | Gaia DR3 244797128533706496 | 03:43:26.67 +45:44:00.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.078+/-0.033 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:43:26.70 +45:44:00.1: 12.96 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:43:26.70 +45:44:00.1: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 43 26.70 +45 44 00.1 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244797128533706496,2461290.6843,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244797128533706496 20260907.1843 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.95 03:37:40.96 +44:13:55.2
151.71436 -9.15324 galactic Per Second-epoch detections are separated by 0.6" and 7.3 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 | Large-amplitude variable Gaia DR2 238600658953962240 | 03:37:40.94 +44:13:56.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=1.093+/-0.027 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:37:40.96 +44:13:55.2: 12.97 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:37:40.96 +44:13:55.2: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 37 40.96 +44 13 55.2 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 238600658953962240,2461290.6843,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
Large-amplitude variable Gaia DR2 238600658953962240 20260907.1843 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 12.08 03:38:32.99 +44:00:24.8
151.97725 -9.24014 galactic Per Second-epoch detections are separated by 1.0" and 7.0 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 | 03:38:32.99 +44:00:24.8 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.219+/-0.028 (F)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:38:32.99 +44:00:24.8: 13.11 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:38:32.99 +44:00:24.8: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 38 32.99 +44 00 24.8 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 12.04 03:34:52.61 +43:18:56.9
151.85414 -10.19100 galactic Per Second-epoch detections are separated by 3.0" and 7.4 pix
The object was found in VSX 8" Gaia DR3 238267300775724032
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.810 G 15.880 G 0.059371100000 A
ATTENTION: measured mag 12.04 is 3.8 mag brighter than the VSX record maximum brightness 15.81 - 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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:52.61 +43:18:56.9: 13.12 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:52.61 +43:18:56.9: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 34 52.61 +43 18 56.9 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238267300775724032,2461290.6843,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238267300775724032 20260907.1843 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 12.05 03:43:04.60 +45:47:30.8
151.52896 -7.33439 galactic Per Second-epoch detections are separated by 2.3" and 6.9 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 | 03:43:04.60 +45:47:30.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.794+/-0.032 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:43:04.60 +45:47:30.8: 13.15 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:43:04.60 +45:47:30.8: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 43 04.60 +45 47 30.8 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 12.05CV 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 09 07.1843 2461290.6843 12.21 03:35:23.14 +43:30:45.8
151.81134 -9.97760 galactic Per Second-epoch detections are separated by 0.5" and 7.3 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 | 03:35:23.14 +43:30:45.8 (user input) | T | P | (position from user input) J-Ks=0.750+/-0.033 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:35:23.14 +43:30:45.8: 13.34 +/- 0.03 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:35:23.14 +43:30:45.8: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 35 23.14 +43 30 45.8 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 12.09 03:35:16.23 +43:44:58.5
151.65187 -9.79911 galactic Per Second-epoch detections are separated by 1.6" and 7.2 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 | 03:35:16.23 +43:44:58.5 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.035 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:35:16.23 +43:44:58.5: 13.21 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:35:16.23 +43:44:58.5: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 35 16.23 +43 44 58.5 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 12.04 03:42:38.54 +45:13:07.7
151.82122 -7.83468 galactic Per Second-epoch detections are separated by 0.5" and 7.0 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 | 03:42:38.54 +45:13:07.7 (user input) | T | P | (position from user input) J-Ks=0.931+/-0.030 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:38.54 +45:13:07.7: 13.18 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:38.54 +45:13:07.7: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 42 38.54 +45 13 07.7 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 12.04 03:33:30.82 +44:30:11.2
150.94335 -9.37590 galactic Per Second-epoch detections are separated by 2.9" and 7.6 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 | 03:33:30.82 +44:30:11.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.542+/-0.028 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:30.82 +44:30:11.2: 13.14 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:30.82 +44:30:11.2: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 33 30.82 +44 30 11.2 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.90 03:41:28.22 +45:13:25.8
151.65284 -7.95634 galactic Per Second-epoch detections are separated by 0.6" and 6.9 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 | 03:41:28.22 +45:13:25.8 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.034 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:28.22 +45:13:25.8: 13.14 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:28.22 +45:13:25.8: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 41 28.22 +45 13 25.8 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 12.03 03:34:32.01 +43:28:57.9
151.70281 -10.09318 galactic Per Second-epoch detections are separated by 0.6" and 7.4 pix
The object was found in VSX22" Gaia DR3 238457653726777984
Type: S
# Max. Min./Amp. JD0 Period
17.010 G 17.250 G O
ATTENTION: measured mag 12.03 is 5.0 mag brighter than the VSX record maximum brightness 17.01 - 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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:32.01 +43:28:57.9: 13.12 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:32.01 +43:28:57.9: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 34 32.01 +43 28 57.9 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238457653726777984,2461290.6843,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238457653726777984 20260907.1843 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.96 03:42:09.48 +45:31:10.8
151.56808 -7.64803 galactic Per Second-epoch detections are separated by 0.7" and 6.9 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 | Gaia DR3 244773312935300608 | 03:42:09.52 +45:31:11.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.988+/-0.031 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:09.48 +45:31:10.8: 13.11 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:09.48 +45:31:10.8: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 42 09.48 +45 31 10.8 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244773312935300608,2461290.6843,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244773312935300608 20260907.1843 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 31 11.93 +43 54 15.2 11.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GK Per,2461290.6843,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
GK Per 20260907.1843 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.94 03:38:14.55 +45:14:36.4
151.18287 -8.28323 galactic Per Second-epoch detections are separated by 1.1" and 7.2 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 J054.5607+45.2436 | 03:38:14.57 +45:14:37.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.291+/-0.024 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:38:14.55 +45:14:36.4: 13.04 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:38:14.55 +45:14:36.4: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 38 14.55 +45 14 36.4 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J054.5607+45.2436,2461290.6843,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 J054.5607+45.2436 20260907.1843 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.99 03:34:57.24 +43:18:47.8
151.86716 -10.18473 galactic Per Second-epoch detections are separated by 0.6" 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 | 03:34:57.24 +43:18:47.8 (user input) | T | P | (position from user input) J-Ks=0.693+/-0.033 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:57.24 +43:18:47.8: 13.01 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:57.24 +43:18:47.8: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 34 57.24 +43 18 47.8 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 12.03 03:39:32.02 +44:44:36.6
151.67084 -8.54598 galactic Per Second-epoch detections are separated by 1.4" and 6.9 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 | 03:39:32.02 +44:44:36.6 (user input) | T | P | (position from user input) J-Ks=0.757+/-0.027 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:39:32.02 +44:44:36.6: 12.98 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:39:32.02 +44:44:36.6: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 39 32.02 +44 44 36.6 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.73 03:34:11.53 +43:02:16.9
151.91860 -10.48886 galactic Per Second-epoch detections are separated by 0.5" and 7.5 pix
The object was found in VSX 0" NSVS 4169150
Type: EW
# Max. Min./Amp. JD0 Period
12.924 g Y 0.533 g 2458434.91400 0.431408000000
The object was not found in astcheck.
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:11.53 +43:02:16.9: 12.98 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:11.53 +43:02:16.9: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 34 11.53 +43 02 16.9 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 4169150,2461290.6843,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 4169150 20260907.1843 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.89 03:39:55.72 +45:11:18.6
151.45609 -8.14879 galactic Per Second-epoch detections are separated by 0.6" and 7.0 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 | Gaia DR3 244669172867900544 | 03:39:55.76 +45:11:19.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=0.956+/-0.028 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:39:55.72 +45:11:18.6: 12.96 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:39:55.72 +45:11:18.6: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 39 55.72 +45 11 18.6 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244669172867900544,2461290.6843,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244669172867900544 20260907.1843 11.89CV 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 09 07.1843 2461290.6843 12.01 03:42:07.95 +45:05:07.4
151.83143 -7.99524 galactic Per Second-epoch detections are separated by 0.9" 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 | Gaia DR3 244743385605981440 | 03:42:07.87 +45:05:06.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.864+/-0.030 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:07.95 +45:05:07.4: 12.96 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:07.95 +45:05:07.4: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 42 07.95 +45 05 07.4 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244743385605981440,2461290.6843,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244743385605981440 20260907.1843 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.94 03:32:27.72 +42:51:24.1
151.76642 -10.82167 galactic Per Second-epoch detections are separated by 0.9" and 7.5 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 | target | 03:32:27.72 +42:51:24.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.775+/-0.028 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:32:27.72 +42:51:24.1: 12.95 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:32:27.72 +42:51:24.1: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 32 27.72 +42 51 24.1 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.90 03:35:22.83 +43:45:28.0
151.66319 -9.78075 galactic Per Second-epoch detections are separated by 2.3" and 7.0 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 | 03:35:22.83 +43:45:28.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.710+/-0.031 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:35:22.83 +43:45:28.0: 12.93 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:35:22.83 +43:45:28.0: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 35 22.83 +43 45 28.0 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.88 03:40:23.15 +44:48:01.9
151.75795 -8.40922 galactic Per Second-epoch detections are separated by 0.9" and 6.9 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 | 03:40:23.15 +44:48:01.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.723+/-0.028 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:40:23.15 +44:48:01.9: 12.92 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:40:23.15 +44:48:01.9: 12.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 40 23.15 +44 48 01.9 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.96 03:33:18.16 +43:29:34.1
151.51345 -10.21647 galactic Per Second-epoch detections are separated by 0.5" and 7.2 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 | Gaia DR3 238472084816940928 | 03:33:18.10 +43:29:33.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.905+/-0.029 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:18.16 +43:29:34.1: 12.92 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:18.16 +43:29:34.1: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 33 18.16 +43 29 34.1 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238472084816940928,2461290.6843,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238472084816940928 20260907.1843 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.96 03:38:28.37 +44:25:35.7
151.71091 -8.91278 galactic Per Second-epoch detections are separated by 1.0" and 7.1 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 | Gaia DR3 244608424850811904 | 03:38:28.40 +44:25:36.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.790+/-0.030 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:38:28.37 +44:25:35.7: 12.88 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:38:28.37 +44:25:35.7: 12.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 38 28.37 +44 25 35.7 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244608424850811904,2461290.6843,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244608424850811904 20260907.1843 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.93 03:41:55.90 +45:53:12.1
151.31128 -7.38074 galactic Per Second-epoch detections are separated by 1.3" 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 | Gaia DR3 244829804644876544 | 03:41:54.37 +45:53:50.8 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.407+/-0.032 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:55.90 +45:53:12.1: 12.88 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:55.90 +45:53:12.1: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 41 55.90 +45 53 12.1 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244829804644876544,2461290.6843,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244829804644876544 20260907.1843 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.84 03:42:29.93 +45:09:05.7
151.84241 -7.90337 galactic Per Second-epoch detections are separated by 1.5" and 7.2 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 | 03:42:29.93 +45:09:05.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.366+/-0.035 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:29.93 +45:09:05.7: 12.86 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:29.93 +45:09:05.7: 12.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 42 29.93 +45 09 05.7 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 11.84CV 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 09 07.1843 2461290.6843 11.88 03:33:38.99 +43:45:01.4
151.41147 -9.97108 galactic Per Second-epoch detections are separated by 1.9" and 7.6 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 | 03:33:38.99 +43:45:01.4 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.325+/-0.028 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:38.99 +43:45:01.4: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:38.99 +43:45:01.4: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 33 38.99 +43 45 01.4 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.90 03:41:33.14 +45:13:33.9
151.66304 -7.94578 galactic Per Second-epoch detections are separated by 2.6" and 7.1 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 J055.3922+45.2260 | 03:41:33.14 +45:13:33.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.436+/-0.033 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:33.14 +45:13:33.9: 12.83 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:33.14 +45:13:33.9: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 41 33.14 +45 13 33.9 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J055.3922+45.2260,2461290.6843,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 J055.3922+45.2260 20260907.1843 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.87 03:36:12.70 +44:13:03.3
151.50868 -9.32189 galactic Per Second-epoch detections are separated by 2.4" 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 | 03:36:12.70 +44:13:03.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.391+/-0.030 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:36:12.70 +44:13:03.3: 12.80 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:36:12.70 +44:13:03.3: 12.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 36 12.70 +44 13 03.3 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.70 03:42:24.52 +45:07:02.0
151.85085 -7.94030 galactic Per Second-epoch detections are separated by 1.4" and 7.1 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 J055.6075+45.1151 | 03:42:24.49 +45:07:02.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.184+/-0.031 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:24.52 +45:07:02.0: 12.80 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:24.52 +45:07:02.0: 12.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 42 24.52 +45 07 02.0 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J055.6075+45.1151,2461290.6843,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 J055.6075+45.1151 20260907.1843 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.83 03:43:20.39 +45:59:44.9
151.43986 -7.14501 galactic Per Second-epoch detections are separated by 0.8" and 6.8 pix
The object was found in VSX 2" Gaia DR3 244851928016656640
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.370 G 13.400 G A
The object was not found in astcheck.
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:43:20.39 +45:59:44.9: 12.77 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:43:20.39 +45:59:44.9: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 43 20.39 +45 59 44.9 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244851928016656640,2461290.6843,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244851928016656640 20260907.1843 11.83CV 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 09 07.1843 2461290.6843 11.87 03:44:11.71 +45:55:50.9
151.59839 -7.10532 galactic Per Second-epoch detections are separated by 0.8" and 7.0 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 | Gaia DR3 244806062065531136 | 03:44:11.69 +45:55:51.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5) J-Ks=0.724+/-0.028 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:44:11.71 +45:55:50.9: 12.77 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:44:11.71 +45:55:50.9: 12.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 44 11.71 +45 55 50.9 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244806062065531136,2461290.6843,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244806062065531136 20260907.1843 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.75 03:36:52.38 +43:49:19.2
151.84421 -9.56901 galactic Per Second-epoch detections are separated by 0.6" and 7.3 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 | Gaia DR3 238397455463970944 | 03:36:52.42 +43:49:18.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5) J-Ks=0.950+/-0.029 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:36:52.38 +43:49:19.2: 12.71 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:36:52.38 +43:49:19.2: 12.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 36 52.38 +43 49 19.2 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238397455463970944,2461290.6843,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238397455463970944 20260907.1843 11.75CV 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 09 07.1843 2461290.6843 11.76 03:37:58.26 +44:00:22.9
151.89319 -9.30301 galactic Per Second-epoch detections are separated by 2.2" and 6.9 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 J054.5024+44.0090 | 03:37:58.26 +44:00:22.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.395+/-0.028 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:37:58.26 +44:00:22.9: 12.67 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:37:58.26 +44:00:22.9: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 37 58.26 +44 00 22.9 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J054.5024+44.0090,2461290.6843,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 J054.5024+44.0090 20260907.1843 11.76CV 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 09 07.1843 2461290.6843 11.65 03:40:29.28 +45:07:47.4
151.57127 -8.13601 galactic Per Second-epoch detections are separated by 0.8" and 7.1 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 J055.1248+45.1342 | 03:40:29.24 +45:07:47.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.428+/-0.031 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:40:29.28 +45:07:47.4: 12.67 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:40:29.28 +45:07:47.4: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 40 29.28 +45 07 47.4 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J055.1248+45.1342,2461290.6843,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 J055.1248+45.1342 20260907.1843 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.76 03:41:38.91 +45:50:54.0
151.29528 -7.44115 galactic Per Second-epoch detections are separated by 2.8" and 6.6 pix
The object was found in VSX13" Gaia DR3 244828121017742592
Type: ROT
# Max. Min./Amp. JD0 Period
13.790 G 13.810 G G
The object was not found in astcheck.
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:38.91 +45:50:54.0: 12.70 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:38.91 +45:50:54.0: 12.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 41 38.91 +45 50 54.0 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244828121017742592,2461290.6843,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244828121017742592 20260907.1843 11.76CV 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 09 07.1843 2461290.6843 11.69 03:41:13.01 +44:57:17.8
151.78178 -8.19718 galactic Per Second-epoch detections are separated by 2.1" and 7.0 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 | 03:41:13.01 +44:57:17.8 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.174+/-0.028 (F)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:13.01 +44:57:17.8: 12.66 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:13.01 +44:57:17.8: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 41 13.01 +44 57 17.8 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6843,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260907.1843 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.63 03:34:07.77 +43:36:16.0
151.56987 -10.03807 galactic Per Second-epoch detections are separated by 1.7" 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 | Gaia DR3 238473837163513600 | 03:34:07.78 +43:36:15.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.287+/-0.028 (F)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:07.77 +43:36:16.0: 12.65 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:07.77 +43:36:16.0: 12.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 34 07.77 +43 36 16.0 11.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238473837163513600,2461290.6843,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238473837163513600 20260907.1843 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.68 03:34:42.13 +43:28:20.4
151.73413 -10.08352 galactic Per Second-epoch detections are separated by 1.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 238551142276661504 | 03:34:42.10 +43:28:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.840+/-0.033 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:42.13 +43:28:20.4: 12.63 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:42.13 +43:28:20.4: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 34 42.13 +43 28 20.4 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238551142276661504,2461290.6843,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238551142276661504 20260907.1843 11.68CV 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 09 07.1843 2461290.6843 11.72 03:33:58.26 +43:50:23.9
151.40560 -9.86454 galactic Per Second-epoch detections are separated by 0.3" and 7.3 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 | Gaia DR3 238573961440453760 | 03:33:58.23 +43:50:23.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.723+/-0.025 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:58.26 +43:50:23.9: 12.64 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:58.26 +43:50:23.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 33 58.26 +43 50 23.9 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238573961440453760,2461290.6843,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238573961440453760 20260907.1843 11.72CV 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 09 07.1843 2461290.6843 11.67 03:40:37.20 +45:04:22.3
151.62482 -8.16729 galactic Per Second-epoch detections are separated by 1.3" and 6.9 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 | Gaia DR3 244663774091258112 | 03:40:37.16 +45:04:23.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.892+/-0.028 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:40:37.20 +45:04:22.3: 12.63 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:40:37.20 +45:04:22.3: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 40 37.20 +45 04 22.3 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244663774091258112,2461290.6843,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244663774091258112 20260907.1843 11.67CV 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 09 07.1843 2461290.6843 11.72 03:31:13.68 +43:07:20.7
151.42203 -10.73758 galactic Per Second-epoch detections are separated by 0.9" 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 | Gaia DR3 238434460903680768 | 03:31:13.68 +43:07:21.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.327+/-0.031 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:31:13.68 +43:07:20.7: 12.63 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:31:13.68 +43:07:20.7: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 31 13.68 +43 07 20.7 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 238434460903680768,2461290.6843,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 238434460903680768 20260907.1843 11.72CV 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 09 07.1843 2461290.6843 11.72 03:42:18.74 +45:06:56.5
151.83819 -7.95187 galactic Per Second-epoch detections are separated by 0.7" and 6.9 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 | Gaia DR3 244743488685256064 | 03:42:18.72 +45:06:56.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.364+/-0.031 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:18.74 +45:06:56.5: 12.61 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:18.74 +45:06:56.5: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 42 18.74 +45 06 56.5 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244743488685256064,2461290.6843,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244743488685256064 20260907.1843 11.72CV 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 09 07.1843 2461290.6843 11.69 03:41:41.31 +45:25:02.5
151.56493 -7.77931 galactic Per Second-epoch detections are separated by 1.0" and 7.0 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 | Gaia DR3 244766720165510272 | 03:41:41.30 +45:25:02.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.333+/-0.028 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:41.31 +45:25:02.5: 12.59 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:41.31 +45:25:02.5: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 41 41.31 +45 25 02.5 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244766720165510272,2461290.6843,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244766720165510272 20260907.1843 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.62 03:42:53.09 +45:43:21.0
151.54498 -7.40978 galactic Per Second-epoch detections are separated by 0.6" 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 | Gaia DR3 244776542750697856 | 03:42:53.06 +45:43:20.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.361+/-0.032 (G)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:53.09 +45:43:21.0: 12.56 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:53.09 +45:43:21.0: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 42 53.09 +45 43 21.0 11.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244776542750697856,2461290.6843,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244776542750697856 20260907.1843 11.62CV 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 09 07.1843 2461290.6843 11.53 03:33:52.92 +43:44:15.4
151.45354 -9.95676 galactic Per Second-epoch detections are separated by 1.2" 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 | ATO J053.4646+43.7467 | 03:33:52.94 +43:44:15.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.788+/-0.026 (K)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:52.92 +43:44:15.4: 12.48 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:52.92 +43:44:15.4: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 33 52.92 +43 44 15.4 11.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J053.4646+43.7467,2461290.6843,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 J053.4646+43.7467 20260907.1843 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.44 03:36:19.51 +44:08:00.2
151.57597 -9.37751 galactic Per Second-epoch detections are separated by 0.8" and 7.0 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 J054.0764+44.1325 | 03:36:19.50 +44:08:00.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.875+/-0.028 (M)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:36:19.51 +44:08:00.2: 12.36 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:36:19.51 +44:08:00.2: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 36 19.51 +44 08 00.2 11.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J054.0764+44.1325,2461290.6843,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 J054.0764+44.1325 20260907.1843 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1843 2461290.6843 11.35 03:44:20.93 +45:45:18.3
151.72844 -7.22757 galactic Per Second-epoch detections are separated by 0.3" and 6.9 pix
The object was found in VSX 1" ASASSN-V J034421.00+454518.4
Type: L
# Max. Min./Amp. JD0 Period
12.370 V 12.700 V
The object was not found in astcheck.
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:44:20.93 +45:45:18.3: 12.29 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:44:20.93 +45:45:18.3: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 44 20.93 +45 45 18.3 11.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J034421.00+454518.4,2461290.6843,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 J034421.00+454518.4 20260907.1843 11.35CV 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 09 07.1843 2461290.6843 11.29 03:43:24.02 +45:46:46.7
151.58153 -7.30959 galactic Per Second-epoch detections are separated by 0.9" 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 | Gaia DR3 244800388409120640 | 03:43:24.01 +45:46:47.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=0.256+/-0.033 (F)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:43:24.02 +45:46:46.7: 12.19 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:43:24.02 +45:46:46.7: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.1843* 03 43 24.02 +45 46 46.7 11.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 244800388409120640,2461290.6843,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 244800388409120640 20260907.1843 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.58214624 09.01.2026 01:58:07.435 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
First image: 2461049.58214624 09.01.2026 01:58:07.435 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Last image: 2461290.68474950 07.09.2026 04:25:52.357 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 13 seconds
Number of parallel threads: 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): 17956
Objects passed selection criteria: 17818
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 9967.5
Average stars matched: 9618.5 (96.4986 %)
Memory usage VmPeak: 244836 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 7 00:32:30 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: 2461049.58214624 09.01.2026 01:58:07.435 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
First image: 2461049.58214624 09.01.2026 01:58:07.435 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Last image: 2461290.68474950 07.09.2026 04:25:52.357 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 201
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 30 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): 140864
Objects passed selection criteria: 140229
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 81486
Average stars matched: 77471.2 (95.0731 %)
Memory usage VmPeak: 616588 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 7 00:34:40 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/TTUQ2b1x1/TTUQ2_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/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
SExtractor catalog cache: saved Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.cat to cache
SExtractor catalog cache: saved Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.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/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.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: 2461290.68393600
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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits exists and is non-empty
wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits exists and is non-empty
wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits exists and is non-empty
wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (1st reference image)
verification OK: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:36:01.913 +46:00:00.61 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_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits (1st new image)
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Image size: 940.9'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 03:36:01.665 +45:59:51.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:36:01.913 +46:00:00.61
Second-epoch image center 03:36:01.665 +45:59:51.95
Angular distance between the image centers 0.0025 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits (2nd new image)
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
Image size: 940.8'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 03:35:59.952 +46:00:30.11 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:36:01.913 +46:00:00.61
Second-epoch image center 03:35:59.952 +46:00:30.11
Angular distance between the image centers 0.0100 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 03:36:01.665 +45:59:51.95
Second-epoch second image center 03:35:59.952 +46:00:30.11
Angular distance between the image centers 0.01170 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/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits &> /tmp/tmp.EHfqovjT3s
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits &> /tmp/tmp.U1P5utW0tG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits &> /tmp/tmp.otoyEY6mCB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits &> /tmp/tmp.tAkcGfiulP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
Found non-empty wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
The reference image (wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits) and catalog (wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat) found
'wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat' -> 'wcsmag.cat'
Read 24919 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2386 to 65.8886 deg, Dec +39.8263 to +51.4097 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 41.2386 to 65.8886 deg, Dec 39.8263 to 51.4097 deg
Loaded 12587 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): 8299 out of 9376 total matches.
Matched with Tycho-2 9376 out of 24919 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.954600
a=0.000000 b=1.000000 c=22.954600
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 24919 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2386 to 65.8886 deg, Dec +39.8263 to +51.4097 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 41.2386 to 65.8886 deg, Dec 39.8263 to 51.4097 deg
Loaded 12587 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): 8299 out of 9376 total matches.
Matched with Tycho-2 9376 out of 24919 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Forced-photometry filter: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits -> calib.txt_param_ref_wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (aperture=5.7)
Read 25014 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2390 to 65.8888 deg, Dec +39.8264 to +51.4150 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 41.2390 to 65.8888 deg, Dec 39.8264 to 51.4150 deg
Loaded 12591 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): 8306 out of 9365 total matches.
Matched with Tycho-2 9365 out of 25014 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Forced-photometry filter: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits -> calib.txt_param_ref_wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits (aperture=5.8)
____ 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:
2.0 pix Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
2.0 pix Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
2.2 pix fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
2.2 pix fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
Limiting magnitude estimates:
15.4 mag. Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
15.4 mag. Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
10.9 mag. fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
10.9 mag. fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
All-image limiting magnitude estimate: 10.9 (SNR ) 9.4 (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.EHfqovjT3s (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits' -> 'wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Checking if the catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS catalog name: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=2608, bad_region=5544, passed=24919
Got 24919 stars (including 17235 good ones) from the SExtractor catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
util/solve_plate_with_UCAC5 got 24919 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 4918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 20428 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 20428 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 20428 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4919 stars left (next iteration limit 5409)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits N_match=4919 sigma_overall_arcsec=0.425 sigma_q1_arcsec=0.552 sigma_q2_arcsec=0.379 sigma_q3_arcsec=0.375 sigma_q4_arcsec=0.379 n_q1=1615 n_q2=801 n_q3=1627 n_q4=876 worst_quadrant_to_overall_ratio=1.300
The image catalog is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits -region wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.U1P5utW0tG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits' -> 'wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.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/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Checking if the catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS catalog name: wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=17, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2561, bad_region=5578, passed=24997
Got 24997 stars (including 17348 good ones) from the SExtractor catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat
util/solve_plate_with_UCAC5 got 24997 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 4919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 20490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 20490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 20490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4920 stars left (next iteration limit 5410)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits N_match=4920 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.466 sigma_q2_arcsec=0.360 sigma_q3_arcsec=0.350 sigma_q4_arcsec=0.356 n_q1=1613 n_q2=791 n_q3=1642 n_q4=874 worst_quadrant_to_overall_ratio=1.221
The image catalog is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits -region wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.otoyEY6mCB (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_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.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_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
WCS-calibrated image found: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=42, bad_region=449, passed=1072
Got 1072 stars (including 598 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat
util/solve_plate_with_UCAC5 got 1072 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 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 652 to 708 (Dec 40.5 to 51.2)
Done reading UCAC5 zone files...
Matched 574 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 571 matched stars entering correct_measured_positions(), 528 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 571 matched stars entering correct_measured_positions(), 584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
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 652 to 708 (Dec 40.5 to 51.2)
Done reading UCAC5 zone files...
Matched 574 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 571 matched stars entering correct_measured_positions(), 585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Accuracy estimation diagnostic: 571 matched stars entering correct_measured_positions(), 585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 571 stars left (next iteration limit 628)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=571 robust_rms=4.922 arcsec worst_quadrant_rms=9.217 arcsec
SIP_REFIT: SIP order 3 trial: matched=571 robust_rms=0.766 arcsec worst_quadrant_rms=0.886 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=571 robust_rms_before=1.634 arcsec robust_rms_before_corrected=0.833 arcsec robust_rms_after=0.766 arcsec worst_quadrant_rms_before=1.310 worst_quadrant_rms_after=0.886
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Image size: 940.5'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 03:36:01.741 +45:59:50.79 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1072 stars ###
'wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/correct_sextractor_wcs_catalog_usingxy2sky3375543.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 1.634 -> 0.766 arcsec)
WCS_QUALITY_DIAG: file=fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits N_match=571 sigma_overall_arcsec=0.810 sigma_q1_arcsec=0.722 sigma_q2_arcsec=0.840 sigma_q3_arcsec=1.077 sigma_q4_arcsec=0.586 n_q1=205 n_q2=104 n_q3=176 n_q4=86 worst_quadrant_to_overall_ratio=1.329
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits -region wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.tAkcGfiulP (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_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.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_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
WCS-calibrated image found: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=39, bad_region=453, passed=1119
Got 1119 stars (including 646 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat
util/solve_plate_with_UCAC5 got 1119 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 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 652 to 708 (Dec 40.6 to 51.2)
Done reading UCAC5 zone files...
Matched 616 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 613 matched stars entering correct_measured_positions(), 573 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 613 matched stars entering correct_measured_positions(), 628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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 652 to 708 (Dec 40.6 to 51.2)
Done reading UCAC5 zone files...
Matched 616 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 613 matched stars entering correct_measured_positions(), 628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 613 matched stars entering correct_measured_positions(), 628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 613 stars left (next iteration limit 674)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=613 robust_rms=4.781 arcsec worst_quadrant_rms=9.642 arcsec
SIP_REFIT: SIP order 3 trial: matched=613 robust_rms=0.731 arcsec worst_quadrant_rms=0.946 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=613 robust_rms_before=1.644 arcsec robust_rms_before_corrected=0.823 arcsec robust_rms_after=0.731 arcsec worst_quadrant_rms_before=1.291 worst_quadrant_rms_after=0.946
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
Image size: 940.4'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 03:36:00.032 +46:00:28.97 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1119 stars ###
'wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/correct_sextractor_wcs_catalog_usingxy2sky3364245.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 1.644 -> 0.731 arcsec)
WCS_QUALITY_DIAG: file=fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits N_match=613 sigma_overall_arcsec=0.707 sigma_q1_arcsec=0.568 sigma_q2_arcsec=0.674 sigma_q3_arcsec=0.968 sigma_q4_arcsec=0.584 n_q1=223 n_q2=110 n_q3=191 n_q4=89 worst_quadrant_to_overall_ratio=1.370
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits -region wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits to local_wcs_cache/
'wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits' -> 'local_wcs_cache/wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits'
Saving the final (post-refit) wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits to local_wcs_cache/
'wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits' -> 'local_wcs_cache/wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits'
Saving the final (post-refit) wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits to local_wcs_cache/
'wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits' -> 'local_wcs_cache/wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits'
Saving the final (post-refit) wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits to local_wcs_cache/
'wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits' -> 'local_wcs_cache/wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits sigma_overall=0.425 worst_q_ratio=1.300
ref2=Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits sigma_overall=0.382 worst_q_ratio=1.221
new1=fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits sigma_overall=0.810 worst_q_ratio=1.329
new2=fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits sigma_overall=0.707 worst_q_ratio=1.370
reference average sigma_overall=0.4035 worst_q_ratio=1.2605
warn-on-ratio threshold: 2.0x reference
###################################
WCS_QUALITY_RETRY: 1st new image (fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits) flagged: sigma=0.810 (ref avg 0.4035), ratio=1.329 (ref avg 1.2605), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
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_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.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_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/lib/make_outxyls_for_astrometric_calibration found 1026 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out3424874.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3424874.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 36.3161 (5.9141e+15), 7 match, 0 conflict, 27 distractors, 29 index.
RA,Dec = (54.0083,45.9934), pixel scale 5.97063 arcsec/pix.
Hit/miss: Hit/miss: --+-+---+--------+---+-+---------+(best)--------------------+---------------+--------------+--------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out3424874.solved to indicate this.
Field: out3424874.xyls
Field center: (RA,Dec) = (54.010225, 45.998796) deg.
Field center: (RA H:M:S, Dec D:M:S) = (03:36:02.454, +45:59:55.667).
Field size: 15.7756 x 10.5511 degrees
Field rotation angle: up is -1.65985 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits' -> 'fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Sep 7 00:33 fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
-rw-r--r-- 1 apache apache 12K Sep 7 00:33 out3424874.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits for reading... done!
Creating new image file (wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits (fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out3424874.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3424874.axy"...
Only searching for solutions within 15.7183 degrees of RA,Dec (54.0114,45.9996)
log-odds ratio 36.3161 (5.9141e+15), 7 match, 0 conflict, 27 distractors, 29 index.
RA,Dec = (54.0083,45.9934), pixel scale 5.97063 arcsec/pix.
Hit/miss: Hit/miss: --+-+---+--------+---+-+---------+(best)--------------------+---------------+--------------+--------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out3424874.solved to indicate this.
Field: out3424874.xyls
Field center: (RA,Dec) = (54.010225, 45.998796) deg.
Field center: (RA H:M:S, Dec D:M:S) = (03:36:02.454, +45:59:55.667).
Field size: 15.7756 x 10.5511 degrees
Field rotation angle: up is -1.65985 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Sep 7 00:33 fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
-rw-r--r-- 1 apache apache 12K Sep 7 00:33 out3424874.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits for reading... done!
Creating new image file (wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Generating wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat from image00003.cat
Catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits created.
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Image size: 943.1'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:36:02.732 +45:59:58.73 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1072 stars ###
'wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/correct_sextractor_wcs_catalog_usingxy2sky3447005.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=42, bad_region=449, passed=1072
Got 1072 stars (including 598 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat
util/solve_plate_with_UCAC5 got 1072 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.1'
Seting catalog search parameters based on the expected field of view 943.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013099 (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 0.010479 (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 652 to 708 (Dec 40.5 to 51.2)
Done reading UCAC5 zone files...
Matched 514 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 463 matched stars entering correct_measured_positions(), 425 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 460 matched stars entering correct_measured_positions(), 509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.55"
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 652 to 708 (Dec 40.5 to 51.2)
Done reading UCAC5 zone files...
Matched 521 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 489 matched stars entering correct_measured_positions(), 532 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.33"
Accuracy estimation diagnostic: 487 matched stars entering correct_measured_positions(), 543 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.14"
Excluding outliers - 487 stars left (next iteration limit 506)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=487 robust_rms=2.812 arcsec worst_quadrant_rms=35.721 arcsec
SIP_REFIT: SIP order 3 trial: matched=487 robust_rms=0.639 arcsec worst_quadrant_rms=0.854 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=487 robust_rms_before=13.397 arcsec robust_rms_before_corrected=2.948 arcsec robust_rms_after=0.639 arcsec worst_quadrant_rms_before=11.671 worst_quadrant_rms_after=0.854
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Image size: 940.3'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 03:36:01.737 +45:59:50.81 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1072 stars ###
'wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/correct_sextractor_wcs_catalog_usingxy2sky3459205.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 13.397 -> 0.639 arcsec)
WCS_QUALITY_DIAG: file=fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits N_match=487 sigma_overall_arcsec=0.747 sigma_q1_arcsec=0.613 sigma_q2_arcsec=0.801 sigma_q3_arcsec=1.468 sigma_q4_arcsec=0.563 n_q1=182 n_q2=104 n_q3=114 n_q4=87 worst_quadrant_to_overall_ratio=1.965
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits -region wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 1st new image (fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits): sigma 0.810->0.747, ratio 1.329->1.965; reverting to order 3
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020_astrometric_residuals.png (4919 matched stars from wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021_astrometric_residuals.png (4920 matched stars from wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149_astrometric_residuals.png (571 matched stars from wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.66 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150_astrometric_residuals.png (613 matched stars from wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.60 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits'
Saving fully-calibrated image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits'
Preparing the HTML report for the field Per-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Per-02-Q2b1x1 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/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
SExtractor catalog cache: saved Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.cat to cache
SExtractor catalog cache: saved Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Creating symlink local_wcs_cache/wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Creating symlink local_wcs_cache/wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Creating symlink local_wcs_cache/wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits exists and is non-empty
wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits exists and is non-empty
wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits exists and is non-empty
wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (1st reference image)
verification OK: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:36:01.913 +46:00:00.61 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_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits (1st new image)
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Image size: 940.5'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 03:36:01.741 +45:59:50.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:36:01.913 +46:00:00.61
Second-epoch image center 03:36:01.741 +45:59:50.79
Angular distance between the image centers 0.0028 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits (2nd new image)
verification OK: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
Image size: 940.4'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 03:36:00.032 +46:00:28.97 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:36:01.913 +46:00:00.61
Second-epoch image center 03:36:00.032 +46:00:28.97
Angular distance between the image centers 0.0096 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 03:36:01.741 +45:59:50.79
Second-epoch second image center 03:36:00.032 +46:00:28.97
Angular distance between the image centers 0.01170 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/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits &> /tmp/tmp.pvpF7DbTit
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits &> /tmp/tmp.nzG8Sy0TBm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits &> /tmp/tmp.gF1Gy1XY1Z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits &> /tmp/tmp.aoIxSU3Nqr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
Found non-empty wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
The reference image (wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits) and catalog (wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat) found
'wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat' -> 'wcsmag.cat'
Read 189134 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2226 to 65.9097 deg, Dec +39.7810 to +51.4146 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 41.2226 to 65.9097 deg, Dec 39.7810 to 51.4146 deg
Loaded 12673 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): 6489 out of 9455 total matches.
Matched with Tycho-2 9455 out of 189134 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.821000
a=0.000000 b=1.000000 c=22.821000
From vast_summary.log: estimated ref. image limiting mag.: -7.19
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.63
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.63
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 189134 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2226 to 65.9097 deg, Dec +39.7810 to +51.4146 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 41.2226 to 65.9097 deg, Dec 39.7810 to 51.4146 deg
Loaded 12673 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): 6489 out of 9455 total matches.
Matched with Tycho-2 9455 out of 189134 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Forced-photometry filter: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits -> calib.txt_param_ref_wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (aperture=4.3)
Read 187812 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2223 to 65.9102 deg, Dec +39.7810 to +51.4199 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 41.2223 to 65.9102 deg, Dec 39.7810 to 51.4199 deg
Loaded 12677 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): 6500 out of 9428 total matches.
Matched with Tycho-2 9428 out of 187812 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Forced-photometry filter: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits -> calib.txt_param_ref_wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 183 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.8 pix Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
1.9 pix Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
1.9 pix fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
2.0 pix fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
Limiting magnitude estimates:
15.6 mag. Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
15.6 mag. Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
12.1 mag. fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
12.3 mag. fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
All-image limiting magnitude estimate: 12.1 (SNR ) 12.1 (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.pvpF7DbTit (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits' -> 'wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Checking if the catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS catalog name: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=43, blended=23506, bad_region=33336, passed=189091
Got 189091 stars (including 135790 good ones) from the SExtractor catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
util/solve_plate_with_UCAC5 got 189091 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 4923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 162706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 162706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 162706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4923 stars left (next iteration limit 5415)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits N_match=4923 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.527 sigma_q2_arcsec=0.369 sigma_q3_arcsec=0.359 sigma_q4_arcsec=0.356 n_q1=1620 n_q2=815 n_q3=1614 n_q4=874 worst_quadrant_to_overall_ratio=1.300
The image catalog is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits -region wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.nzG8Sy0TBm (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits' -> 'wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.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/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Checking if the catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS catalog name: wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=6, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=23390, bad_region=33357, passed=187770
Got 187770 stars (including 134514 good ones) from the SExtractor catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat
util/solve_plate_with_UCAC5 got 187770 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 4919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 161324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 161324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 161324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4919 stars left (next iteration limit 5410)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.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_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits N_match=4919 sigma_overall_arcsec=0.370 sigma_q1_arcsec=0.437 sigma_q2_arcsec=0.354 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.344 n_q1=1627 n_q2=807 n_q3=1602 n_q4=883 worst_quadrant_to_overall_ratio=1.180
The image catalog is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits -region wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.gF1Gy1XY1Z (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_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.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_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
WCS-calibrated image found: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=218, bad_region=4005, passed=12468
Got 12468 stars (including 8328 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat
util/solve_plate_with_UCAC5 got 12468 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.5'
Seting catalog search parameters based on the expected field of view 940.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013063 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010450 (37.6 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 651 to 708 (Dec 40.3 to 51.2)
Done reading UCAC5 zone files...
Matched 4901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 4866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 9064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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 651 to 708 (Dec 40.3 to 51.2)
Done reading UCAC5 zone files...
Matched 4902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 9064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 9064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 4865 stars left (next iteration limit 5352)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.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=4865 robust_rms=5.124 arcsec worst_quadrant_rms=7.272 arcsec
SIP_REFIT: SIP order 3 trial: matched=4865 robust_rms=0.919 arcsec worst_quadrant_rms=1.357 arcsec
SIP_REFIT: SIP order 5 trial: matched=4865 robust_rms=0.839 arcsec worst_quadrant_rms=1.256 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4865 robust_rms_before=0.938 arcsec robust_rms_before_corrected=0.846 arcsec robust_rms_after=0.839 arcsec worst_quadrant_rms_before=1.274 worst_quadrant_rms_after=1.256
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.274 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits N_match=4865 sigma_overall_arcsec=0.839 sigma_q1_arcsec=0.737 sigma_q2_arcsec=0.824 sigma_q3_arcsec=1.238 sigma_q4_arcsec=0.744 n_q1=1727 n_q2=1108 n_q3=1172 n_q4=858 worst_quadrant_to_overall_ratio=1.477
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits -region wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.aoIxSU3Nqr (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_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.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_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
WCS-calibrated image found: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=2, blended=221, bad_region=4034, passed=12745
Got 12745 stars (including 8563 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat
util/solve_plate_with_UCAC5 got 12745 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.4'
Seting catalog search parameters based on the expected field of view 940.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013061 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010449 (37.6 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 651 to 708 (Dec 40.3 to 51.2)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 4865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 9301 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
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 651 to 708 (Dec 40.3 to 51.2)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 9301 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 9301 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 4867 stars left (next iteration limit 5352)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.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=4867 robust_rms=5.155 arcsec worst_quadrant_rms=7.732 arcsec
SIP_REFIT: SIP order 3 trial: matched=4867 robust_rms=0.904 arcsec worst_quadrant_rms=1.393 arcsec
SIP_REFIT: SIP order 5 trial: matched=4867 robust_rms=0.807 arcsec worst_quadrant_rms=1.278 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4867 robust_rms_before=0.912 arcsec robust_rms_before_corrected=0.796 arcsec robust_rms_after=0.807 arcsec worst_quadrant_rms_before=1.280 worst_quadrant_rms_after=1.278
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.280 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits N_match=4867 sigma_overall_arcsec=0.788 sigma_q1_arcsec=0.695 sigma_q2_arcsec=0.710 sigma_q3_arcsec=1.197 sigma_q4_arcsec=0.752 n_q1=1765 n_q2=1118 n_q3=1152 n_q4=832 worst_quadrant_to_overall_ratio=1.520
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits -region wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.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_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Saving fully-calibrated image wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.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_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
Preparing the HTML report for the field Per-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:50.13 +47:36:36.7: 9.36 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:56:36.37 +46:25:48.7: 9.07 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:56:20.21 +46:34:19.1: 9.16 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:28.18 +47:13:43.2: 9.25 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:36.86 +47:37:45.8: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:50.70 +46:40:50.2: 9.34 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:17.76 +47:11:25.9: 9.80 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:45.64 +47:43:04.8: 9.95 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:44.17 +47:00:20.8: 9.96 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:50.70 +46:40:50.2: 9.31 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.32 +/- 0.00
Forced photometry filter REJECTED candidate at 03:57:50.70 +46:40:50.2: ref_mag=9.32 +/- 0.00 new_mean_mag=10.0076 delta=-0.68 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:50.13 +47:36:36.7: 9.35 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:56:36.37 +46:25:48.7: 9.11 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:28.18 +47:13:43.2: 9.25 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:56:20.21 +46:34:19.1: 9.17 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:36.86 +47:37:45.8: 99.00 +/- 99.00 saturated
Forced photometry reference-image weighted average: 9.36 +/- 0.00
Forced photometry filter REJECTED candidate at 04:00:36.86 +47:37:45.8: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry reference-image weighted average: 9.09 +/- 0.00
Forced photometry reference-image weighted average: 9.25 +/- 0.00
Forced photometry reference-image weighted average: 9.17 +/- 0.00
Forced photometry filter REJECTED candidate at 04:00:50.13 +47:36:36.7: ref_mag=9.36 +/- 0.00 new_mean_mag=9.7380 delta=-0.38 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:00:28.18 +47:13:43.2: ref_mag=9.25 +/- 0.00 new_mean_mag=9.6044 delta=-0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:56:20.21 +46:34:19.1: ref_mag=9.17 +/- 0.00 new_mean_mag=10.0259 delta=-0.86 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:56:36.37 +46:25:48.7: ref_mag=9.09 +/- 0.00 new_mean_mag=9.8288 delta=-0.74 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:17.76 +47:11:25.9: 9.79 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.79 +/- 0.00
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:30.01 +47:40:50.5: 9.33 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:45.64 +47:43:04.8: 9.96 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 03:59:17.76 +47:11:25.9: ref_mag=9.79 +/- 0.00 new_mean_mag=10.4116 delta=-0.62 (need > 0.90)
Forced photometry reference-image weighted average: 9.95 +/- 0.00
Forced photometry filter REJECTED candidate at 04:00:45.64 +47:43:04.8: ref_mag=9.95 +/- 0.00 new_mean_mag=10.4319 delta=-0.48 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:44.17 +47:00:20.8: 9.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.96 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:44.17 +47:00:20.8: ref_mag=9.96 +/- 0.00 new_mean_mag=10.4863 delta=-0.53 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:30.01 +47:40:50.5: 9.32 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.32 +/- 0.00
Forced photometry filter REJECTED candidate at 03:59:30.01 +47:40:50.5: ref_mag=9.32 +/- 0.00 new_mean_mag=10.5349 delta=-1.21 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:55:43.80 +46:21:34.0: 9.94 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:01:27.57 +48:45:43.1: 9.70 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:08.38 +48:18:42.9: 9.45 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:46.39 +47:37:20.4: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:18.17 +46:29:26.3: 10.58 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:50.64 +46:55:51.7: 10.14 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:55.02 +47:13:13.0: 10.37 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:01:52.27 +47:27:24.2: 11.15 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:51.36 +47:03:53.5: 10.43 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:55:43.80 +46:21:34.0: 9.92 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:01:27.57 +48:45:43.1: 9.68 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.93 +/- 0.00
Forced photometry filter REJECTED candidate at 03:55:43.80 +46:21:34.0: ref_mag=9.93 +/- 0.00 new_mean_mag=10.6798 delta=-0.75 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:08.38 +48:18:42.9: 9.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.69 +/- 0.00
Forced photometry filter REJECTED candidate at 04:01:27.57 +48:45:43.1: ref_mag=9.69 +/- 0.00 new_mean_mag=10.8288 delta=-1.14 (need > 0.90)
Forced photometry reference-image weighted average: 9.44 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:08.38 +48:18:42.9: ref_mag=9.44 +/- 0.00 new_mean_mag=10.5825 delta=-1.14 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:46.39 +47:37:20.4: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 03:57:46.39 +47:37:20.4: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:18.17 +46:29:26.3: 10.55 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:50.64 +46:55:51.7: 10.15 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.57 +/- 0.00
Forced photometry filter REJECTED candidate at 03:57:18.17 +46:29:26.3: ref_mag=10.57 +/- 0.00 new_mean_mag=10.9950 delta=-0.43 (need > 0.90)
Forced photometry reference-image weighted average: 10.14 +/- 0.00
Forced photometry filter REJECTED candidate at 03:57:50.64 +46:55:51.7: ref_mag=10.14 +/- 0.00 new_mean_mag=10.9224 delta=-0.78 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:01:52.27 +47:27:24.2: 11.15 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:55.02 +47:13:13.0: 10.36 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Forced photometry reference-image weighted average: 10.37 +/- 0.00
Forced photometry filter REJECTED candidate at 04:01:52.27 +47:27:24.2: ref_mag=11.15 +/- 0.00 new_mean_mag=11.0631 delta=0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:58:55.02 +47:13:13.0: ref_mag=10.37 +/- 0.00 new_mean_mag=10.9396 delta=-0.57 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:56.26 +47:30:09.2: 10.34 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:51.36 +47:03:53.5: 10.44 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.43 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:51.36 +47:03:53.5: ref_mag=10.43 +/- 0.00 new_mean_mag=10.9573 delta=-0.52 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:54.26 +46:44:57.3: 10.53 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:42.27 +47:52:40.9: 9.98 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:08.47 +46:37:08.6: 10.86 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:41.08 +47:55:27.9: 10.53 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:56.26 +47:30:09.2: 10.30 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.32 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:56.26 +47:30:09.2: ref_mag=10.32 +/- 0.00 new_mean_mag=11.0485 delta=-0.73 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:38.60 +46:49:33.3: 10.65 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:49.74 +48:12:05.9: 9.99 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:56:48.16 +46:28:57.0: 10.77 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:30.44 +46:42:23.2: 11.20 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:54.26 +46:44:57.3: 10.53 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.53 +/- 0.00
Forced photometry filter REJECTED candidate at 03:57:54.26 +46:44:57.3: ref_mag=10.53 +/- 0.00 new_mean_mag=10.9775 delta=-0.44 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:38.85 +47:13:00.6: 11.00 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:42.27 +47:52:40.9: 9.97 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:08.47 +46:37:08.6: 10.84 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:41.08 +47:55:27.9: 10.52 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:38.60 +46:49:33.3: 10.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.85 +/- 0.00
Forced photometry reference-image weighted average: 9.98 +/- 0.00
Forced photometry reference-image weighted average: 10.52 +/- 0.00
Forced photometry reference-image weighted average: 10.64 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:08.47 +46:37:08.6: ref_mag=10.85 +/- 0.00 new_mean_mag=11.0765 delta=-0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:57:42.27 +47:52:40.9: ref_mag=9.98 +/- 0.00 new_mean_mag=11.0081 delta=-1.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:00:41.08 +47:55:27.9: ref_mag=10.52 +/- 0.00 new_mean_mag=11.0443 delta=-0.52 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:58:38.60 +46:49:33.3: ref_mag=10.64 +/- 0.00 new_mean_mag=11.1358 delta=-0.49 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:49.74 +48:12:05.9: 10.00 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.99 +/- 0.00
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:56:48.16 +46:28:57.0: 10.77 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 04:00:49.74 +48:12:05.9: ref_mag=9.99 +/- 0.00 new_mean_mag=11.2063 delta=-1.21 (need > 0.90)
Forced photometry reference-image weighted average: 10.77 +/- 0.00
Forced photometry filter REJECTED candidate at 03:56:48.16 +46:28:57.0: ref_mag=10.77 +/- 0.00 new_mean_mag=11.2894 delta=-0.52 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:28.97 +47:13:59.8: 11.03 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:30.44 +46:42:23.2: 11.21 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:30.44 +46:42:23.2: ref_mag=11.21 +/- 0.00 new_mean_mag=11.3842 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:38.85 +47:13:00.6: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.01 +/- 0.00
Forced photometry filter REJECTED candidate at 03:59:38.85 +47:13:00.6: ref_mag=11.01 +/- 0.00 new_mean_mag=11.2902 delta=-0.28 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:04.52 +48:25:19.6: 10.38 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:28.97 +47:13:59.8: 11.05 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:01:40.88 +47:41:47.2: 11.33 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.04 +/- 0.00
Forced photometry filter REJECTED candidate at 03:59:28.97 +47:13:59.8: ref_mag=11.04 +/- 0.00 new_mean_mag=11.3703 delta=-0.33 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:23.14 +47:23:50.8: 11.05 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:56:18.26 +46:52:55.3: 9.66 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:01:07.07 +47:33:02.1: 11.56 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:46.14 +48:16:34.0: 10.56 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:53.81 +46:45:09.9: 11.46 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:56:00.35 +46:24:24.9: 11.19 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:04.52 +48:25:19.6: 10.38 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.38 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:04.52 +48:25:19.6: ref_mag=10.38 +/- 0.00 new_mean_mag=11.2907 delta=-0.91 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:01:40.88 +47:41:47.2: 11.33 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.00
Forced photometry filter REJECTED candidate at 04:01:40.88 +47:41:47.2: ref_mag=11.33 +/- 0.00 new_mean_mag=11.3265 delta=0.00 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:46.25 +48:16:00.0: 10.80 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:56:18.26 +46:52:55.3: 9.67 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:23.14 +47:23:50.8: 11.08 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.67 +/- 0.00
Forced photometry filter REJECTED candidate at 03:56:18.26 +46:52:55.3: ref_mag=9.67 +/- 0.00 new_mean_mag=11.3366 delta=-1.67 (need > 0.90)
Forced photometry reference-image weighted average: 11.06 +/- 0.00
Forced photometry filter REJECTED candidate at 03:59:23.14 +47:23:50.8: ref_mag=11.06 +/- 0.00 new_mean_mag=11.4633 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:01:07.07 +47:33:02.1: 11.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.00
Forced photometry filter REJECTED candidate at 04:01:07.07 +47:33:02.1: ref_mag=11.57 +/- 0.00 new_mean_mag=11.3963 delta=0.17 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:46.14 +48:16:34.0: 10.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.55 +/- 0.00
Forced photometry filter REJECTED candidate at 03:57:46.14 +48:16:34.0: ref_mag=10.55 +/- 0.00 new_mean_mag=11.4825 delta=-0.93 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:53.81 +46:45:09.9: 11.46 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:56:00.35 +46:24:24.9: 11.17 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.00
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:12.66 +47:54:16.6: 10.23 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 03:58:53.81 +46:45:09.9: ref_mag=11.46 +/- 0.00 new_mean_mag=11.6582 delta=-0.20 (need > 0.90)
Forced photometry reference-image weighted average: 11.18 +/- 0.00
Forced photometry filter REJECTED candidate at 03:56:00.35 +46:24:24.9: ref_mag=11.18 +/- 0.00 new_mean_mag=11.6972 delta=-0.52 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:46.25 +48:16:00.0: 10.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.79 +/- 0.00
Forced photometry filter REJECTED candidate at 03:59:46.25 +48:16:00.0: ref_mag=10.79 +/- 0.00 new_mean_mag=11.5473 delta=-0.76 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:56:59.50 +46:28:10.6: 11.35 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:08.74 +46:26:39.8: 11.71 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:12.66 +47:54:16.6: 10.25 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:01:58.54 +48:14:10.3: 11.25 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:51.69 +48:18:05.7: 10.82 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.24 +/- 0.00
Forced photometry filter REJECTED candidate at 03:59:12.66 +47:54:16.6: ref_mag=10.24 +/- 0.00 new_mean_mag=11.6137 delta=-1.37 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:48.00 +48:12:21.5: 11.05 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:56:11.62 +46:28:26.6: 11.32 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:01:38.21 +48:41:10.7: 10.91 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:56:59.50 +46:28:10.6: 11.36 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.00
Forced photometry filter REJECTED candidate at 03:56:59.50 +46:28:10.6: ref_mag=11.36 +/- 0.00 new_mean_mag=11.7221 delta=-0.37 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:56:03.70 +46:22:57.7: 11.34 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:01:58.54 +48:14:10.3: 11.23 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:51.69 +48:18:05.7: 10.84 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.00
Forced photometry filter REJECTED candidate at 04:01:58.54 +48:14:10.3: ref_mag=11.24 +/- 0.00 new_mean_mag=11.5265 delta=-0.29 (need > 0.90)
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:51.69 +48:18:05.7: ref_mag=10.83 +/- 0.00 new_mean_mag=11.6567 delta=-0.83 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:08.74 +46:26:39.8: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.00
Forced photometry filter REJECTED candidate at 03:57:08.74 +46:26:39.8: ref_mag=11.70 +/- 0.00 new_mean_mag=11.8160 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:48.00 +48:12:21.5: 11.03 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.04 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:48.00 +48:12:21.5: ref_mag=11.04 +/- 0.00 new_mean_mag=11.7533 delta=-0.71 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:56:11.62 +46:28:26.6: 11.34 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.00
Forced photometry filter REJECTED candidate at 03:56:11.62 +46:28:26.6: ref_mag=11.33 +/- 0.00 new_mean_mag=11.8671 delta=-0.54 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:01:38.21 +48:41:10.7: 10.93 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:47.56 +47:55:49.0: 11.35 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.92 +/- 0.00
Forced photometry filter REJECTED candidate at 04:01:38.21 +48:41:10.7: ref_mag=10.92 +/- 0.00 new_mean_mag=11.7089 delta=-0.79 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:56:03.70 +46:22:57.7: 11.36 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.35 +/- 0.00
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:12.57 +46:42:16.2: 11.38 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 03:56:03.70 +46:22:57.7: ref_mag=11.35 +/- 0.00 new_mean_mag=11.7964 delta=-0.45 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:47.56 +47:55:49.0: 11.37 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:57.18 +49:26:38.9: 9.88 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.00
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:40.51 +47:15:16.6: 12.08 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 03:57:47.56 +47:55:49.0: ref_mag=11.36 +/- 0.00 new_mean_mag=11.8972 delta=-0.54 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:46.06 +47:38:33.3: 10.58 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:04.81 +47:07:36.7: 10.96 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:56:43.03 +47:03:20.2: 11.14 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:12.57 +46:42:16.2: 11.39 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.39 +/- 0.00
Forced photometry filter REJECTED candidate at 03:57:12.57 +46:42:16.2: ref_mag=11.39 +/- 0.00 new_mean_mag=11.8324 delta=-0.44 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:54.29 +47:52:13.0: 11.25 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:58.23 +47:24:57.7: 12.09 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:57.18 +49:26:38.9: 9.90 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.89 +/- 0.00
Forced photometry filter REJECTED candidate at 03:59:57.18 +49:26:38.9: ref_mag=9.89 +/- 0.00 new_mean_mag=11.7499 delta=-1.86 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:46.06 +47:38:33.3: 10.57 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:40.51 +47:15:16.6: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.57 +/- 0.00
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry filter REJECTED candidate at 03:57:46.06 +47:38:33.3: ref_mag=10.57 +/- 0.00 new_mean_mag=11.9390 delta=-1.36 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:00:40.51 +47:15:16.6: ref_mag=12.06 +/- 0.01 new_mean_mag=11.9332 delta=0.13 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:30.35 +46:59:04.1: 12.21 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:04.81 +47:07:36.7: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.96 +/- 0.00
Forced photometry filter REJECTED candidate at 03:57:04.81 +47:07:36.7: ref_mag=10.96 +/- 0.00 new_mean_mag=11.8696 delta=-0.91 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:56:43.03 +47:03:20.2: 11.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.00
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:54.29 +47:52:13.0: 11.26 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 03:56:43.03 +47:03:20.2: ref_mag=11.13 +/- 0.00 new_mean_mag=12.0082 delta=-0.87 (need > 0.90)
Forced photometry reference-image weighted average: 11.25 +/- 0.00
Forced photometry filter REJECTED candidate at 03:59:54.29 +47:52:13.0: ref_mag=11.25 +/- 0.00 new_mean_mag=11.9420 delta=-0.69 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:04.51 +47:27:43.1: 12.17 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:58.23 +47:24:57.7: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry filter REJECTED candidate at 03:59:58.23 +47:24:57.7: ref_mag=12.08 +/- 0.01 new_mean_mag=12.0125 delta=0.07 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:06.79 +48:20:20.7: 11.17 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:30.35 +46:59:04.1: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry filter REJECTED candidate at 03:59:30.35 +46:59:04.1: ref_mag=12.22 +/- 0.01 new_mean_mag=12.0683 delta=0.15 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:04.51 +47:27:43.1: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter REJECTED candidate at 04:00:04.51 +47:27:43.1: ref_mag=12.17 +/- 0.01 new_mean_mag=12.0342 delta=0.14 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:56:14.90 +46:17:12.1: 11.94 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:39.10 +47:34:18.0: 11.81 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:27.76 +46:34:27.1: 11.86 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:06.79 +48:20:20.7: 11.17 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:06.79 +48:20:20.7: ref_mag=11.17 +/- 0.00 new_mean_mag=11.9301 delta=-0.76 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:30.71 +47:01:06.2: 12.39 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:48.14 +47:09:04.0: 11.76 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:33.84 +47:05:06.5: 11.13 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:05.52 +48:09:54.1: 11.30 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:56:14.90 +46:17:12.1: 11.90 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:39.10 +47:34:18.0: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter REJECTED candidate at 03:56:14.90 +46:17:12.1: ref_mag=11.92 +/- 0.01 new_mean_mag=12.1530 delta=-0.23 (need > 0.90)
Forced photometry reference-image weighted average: 11.81 +/- 0.00
Forced photometry filter REJECTED candidate at 03:59:39.10 +47:34:18.0: ref_mag=11.81 +/- 0.00 new_mean_mag=11.9179 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:18.31 +46:46:21.5: 11.86 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:27.76 +46:34:27.1: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Forced photometry filter REJECTED candidate at 03:57:27.76 +46:34:27.1: ref_mag=11.87 +/- 0.01 new_mean_mag=12.0659 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:30.71 +47:01:06.2: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter REJECTED candidate at 03:59:30.71 +47:01:06.2: ref_mag=12.39 +/- 0.01 new_mean_mag=12.2550 delta=0.13 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:48.14 +47:09:04.0: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:48.14 +47:09:04.0: ref_mag=11.76 +/- 0.00 new_mean_mag=12.0760 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:33.84 +47:05:06.5: 11.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.00
Forced photometry filter REJECTED candidate at 03:57:33.84 +47:05:06.5: ref_mag=11.13 +/- 0.00 new_mean_mag=12.0380 delta=-0.91 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:05.52 +48:09:54.1: 11.30 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:05.52 +48:09:54.1: ref_mag=11.30 +/- 0.00 new_mean_mag=12.0731 delta=-0.77 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:18.31 +46:46:21.5: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:18.31 +46:46:21.5: ref_mag=11.86 +/- 0.00 new_mean_mag=12.0849 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:56:10.37 +46:14:02.7: 11.81 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:09.83 +43:31:03.9: 11.88 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:29.36 +43:36:01.8: 12.24 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:37:10.34 +44:06:13.9: 12.49 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:36.64 +43:15:08.9: 12.55 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:59.53 +43:26:09.2: 12.64 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:35:38.55 +43:16:00.6: 12.68 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:56:10.37 +46:14:02.7: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.00
Forced photometry filter REJECTED candidate at 03:56:10.37 +46:14:02.7: ref_mag=11.81 +/- 0.00 new_mean_mag=11.9153 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:36:40.87 +45:03:26.0: 12.63 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:09.83 +43:31:03.9: 11.87 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:29.36 +43:36:01.8: 12.25 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:47.70 +45:55:21.0: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.00
Forced photometry filter KEPT candidate at 03:33:09.83 +43:31:03.9: ref_mag=11.87 +/- 0.00 new_mean_mag=10.9545 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry filter KEPT candidate at 03:34:29.36 +43:36:01.8: ref_mag=12.24 +/- 0.01 new_mean_mag=11.3277 delta=0.92 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:37:10.34 +44:06:13.9: 12.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter KEPT candidate at 03:37:10.34 +44:06:13.9: ref_mag=12.49 +/- 0.01 new_mean_mag=11.5753 delta=0.91 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:27:39.05 +42:10:18.4: 12.83 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:36.64 +43:15:08.9: 12.54 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:59.53 +43:26:09.2: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 03:34:36.64 +43:15:08.9: ref_mag=12.54 +/- 0.01 new_mean_mag=11.6311 delta=0.91 (need > 0.90)
Forced photometry filter KEPT candidate at 03:33:59.53 +43:26:09.2: ref_mag=12.64 +/- 0.01 new_mean_mag=11.7382 delta=0.90 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:35:38.55 +43:16:00.6: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 03:35:38.55 +43:16:00.6: ref_mag=12.68 +/- 0.01 new_mean_mag=11.7509 delta=0.93 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:36:40.87 +45:03:26.0: 12.60 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:47.70 +45:55:21.0: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter REJECTED candidate at 03:36:40.87 +45:03:26.0: ref_mag=12.61 +/- 0.01 new_mean_mag=11.7308 delta=0.88 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:57:47.70 +45:55:21.0: ref_mag=12.54 +/- 0.01 new_mean_mag=11.8144 delta=0.73 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:27:39.05 +42:10:18.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 03:27:39.05 +42:10:18.4: ref_mag=12.82 +/- 0.01 new_mean_mag=11.8797 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:29:33.66 +42:34:46.1: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:29:33.66 +42:34:46.1: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter KEPT candidate at 03:29:33.66 +42:34:46.1: ref_mag=12.83 +/- 0.01 new_mean_mag=11.8292 delta=1.00 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:28:53.69 +42:31:36.0: 12.87 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:55:37.34 +45:32:40.2: 11.81 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:55:37.34 +45:32:40.2: 11.77 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:28:53.69 +42:31:36.0: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.00
Forced photometry filter REJECTED candidate at 03:55:37.34 +45:32:40.2: ref_mag=11.79 +/- 0.00 new_mean_mag=11.4520 delta=0.34 (need > 0.90)
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 03:28:53.69 +42:31:36.0: ref_mag=12.86 +/- 0.01 new_mean_mag=11.8878 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:40:44.47 +45:01:36.1: 12.91 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:40:44.47 +45:01:36.1: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 03:40:44.47 +45:01:36.1: ref_mag=12.95 +/- 0.01 new_mean_mag=11.8996 delta=1.05 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:39:37.87 +45:04:49.7: 12.92 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:37:07.16 +44:30:43.0: 12.94 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:39:37.87 +45:04:49.7: 12.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 03:39:37.87 +45:04:49.7: ref_mag=12.90 +/- 0.01 new_mean_mag=11.9234 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:37:07.16 +44:30:43.0: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 03:37:07.16 +44:30:43.0: ref_mag=12.93 +/- 0.01 new_mean_mag=11.9576 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:37:40.96 +44:13:55.2: 12.97 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:43:26.70 +45:44:00.1: 12.96 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:37:40.96 +44:13:55.2: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 03:37:40.96 +44:13:55.2: ref_mag=12.96 +/- 0.01 new_mean_mag=11.9472 delta=1.01 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:43:26.70 +45:44:00.1: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 03:43:26.70 +45:44:00.1: ref_mag=12.96 +/- 0.01 new_mean_mag=11.9587 delta=1.00 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:01:53.25 +46:46:05.4: 12.19 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:01:53.25 +46:46:05.4: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter REJECTED candidate at 04:01:53.25 +46:46:05.4: ref_mag=12.17 +/- 0.01 new_mean_mag=11.5497 delta=0.62 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:38:32.99 +44:00:24.8: 13.11 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:43:04.60 +45:47:30.8: 13.15 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:38:32.99 +44:00:24.8: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Forced photometry filter KEPT candidate at 03:38:32.99 +44:00:24.8: ref_mag=13.10 +/- 0.01 new_mean_mag=12.0782 delta=1.02 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:52.61 +43:18:56.9: 13.12 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:43:04.60 +45:47:30.8: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.01
Forced photometry filter KEPT candidate at 03:43:04.60 +45:47:30.8: ref_mag=13.14 +/- 0.01 new_mean_mag=12.0589 delta=1.08 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:52.61 +43:18:56.9: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Forced photometry filter KEPT candidate at 03:34:52.61 +43:18:56.9: ref_mag=13.10 +/- 0.01 new_mean_mag=12.0205 delta=1.08 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:01:55.82 +47:07:13.0: 11.76 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:15.59 +46:33:51.3: 11.54 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:42.82 +46:52:43.3: 12.06 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:54.30 +46:44:02.1: 12.57 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:57:36.82 +46:14:25.7: 12.38 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:15.59 +46:33:51.3: 11.55 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.00
Forced photometry filter REJECTED candidate at 03:59:15.59 +46:33:51.3: ref_mag=11.55 +/- 0.00 new_mean_mag=11.5045 delta=0.04 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:54.30 +46:44:02.1: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter REJECTED candidate at 04:00:54.30 +46:44:02.1: ref_mag=12.56 +/- 0.01 new_mean_mag=11.8765 delta=0.68 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:01:55.82 +47:07:13.0: 11.78 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:42.82 +46:52:43.3: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.00
Forced photometry filter REJECTED candidate at 04:01:55.82 +47:07:13.0: ref_mag=11.77 +/- 0.00 new_mean_mag=11.7497 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry filter REJECTED candidate at 04:00:42.82 +46:52:43.3: ref_mag=12.07 +/- 0.01 new_mean_mag=11.7742 delta=0.29 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:57:36.82 +46:14:25.7: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter REJECTED candidate at 03:57:36.82 +46:14:25.7: ref_mag=12.39 +/- 0.01 new_mean_mag=12.1143 delta=0.28 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:01:30.30 +46:10:28.6: 12.54 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:07.39 +46:40:18.2: 11.24 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:52.55 +47:17:01.4: 11.02 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:35:16.23 +43:44:58.5: 13.21 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:35:23.14 +43:30:45.8: 13.34 +/- 0.03 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:01:30.30 +46:10:28.6: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter REJECTED candidate at 04:01:30.30 +46:10:28.6: ref_mag=12.54 +/- 0.01 new_mean_mag=11.9268 delta=0.61 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:07.39 +46:40:18.2: 11.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.00
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:52.55 +47:17:01.4: 11.01 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 03:58:07.39 +46:40:18.2: ref_mag=11.24 +/- 0.00 new_mean_mag=11.4133 delta=-0.17 (need > 0.90)
Forced photometry reference-image weighted average: 11.01 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:52.55 +47:17:01.4: ref_mag=11.01 +/- 0.00 new_mean_mag=11.4992 delta=-0.49 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:35:16.23 +43:44:58.5: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 03:35:16.23 +43:44:58.5: ref_mag=13.21 +/- 0.02 new_mean_mag=12.0684 delta=1.14 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:35:23.14 +43:30:45.8: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 03:35:23.14 +43:30:45.8: ref_mag=13.28 +/- 0.02 new_mean_mag=12.2162 delta=1.07 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:38.54 +45:13:07.7: 13.18 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:38.54 +45:13:07.7: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Forced photometry filter KEPT candidate at 03:42:38.54 +45:13:07.7: ref_mag=13.15 +/- 0.01 new_mean_mag=12.0481 delta=1.10 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:30.82 +44:30:11.2: 13.14 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:45.67 +45:22:56.4: 11.22 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:45.67 +45:22:56.4: 11.21 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.00
Forced photometry filter REJECTED candidate at 03:58:45.67 +45:22:56.4: ref_mag=11.22 +/- 0.00 new_mean_mag=11.1649 delta=0.05 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:30.82 +44:30:11.2: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.01
Forced photometry filter KEPT candidate at 03:33:30.82 +44:30:11.2: ref_mag=13.19 +/- 0.01 new_mean_mag=12.0310 delta=1.16 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:28.22 +45:13:25.8: 13.14 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:28.22 +45:13:25.8: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Forced photometry filter KEPT candidate at 03:41:28.22 +45:13:25.8: ref_mag=13.09 +/- 0.01 new_mean_mag=11.9161 delta=1.18 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:32.01 +43:28:57.9: 13.12 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:32.01 +43:28:57.9: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.01
Forced photometry filter KEPT candidate at 03:34:32.01 +43:28:57.9: ref_mag=13.13 +/- 0.01 new_mean_mag=12.0317 delta=1.10 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:09.48 +45:31:10.8: 13.11 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:09.48 +45:31:10.8: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Forced photometry filter KEPT candidate at 03:42:09.48 +45:31:10.8: ref_mag=13.09 +/- 0.01 new_mean_mag=11.9596 delta=1.13 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:38:14.55 +45:14:36.4: 13.04 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:38:14.55 +45:14:36.4: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter KEPT candidate at 03:38:14.55 +45:14:36.4: ref_mag=13.03 +/- 0.01 new_mean_mag=11.8930 delta=1.14 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:57.24 +43:18:47.8: 13.01 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:57.24 +43:18:47.8: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry filter KEPT candidate at 03:34:57.24 +43:18:47.8: ref_mag=12.99 +/- 0.01 new_mean_mag=11.9967 delta=0.99 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:39:32.02 +44:44:36.6: 12.98 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:39:32.02 +44:44:36.6: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 03:39:32.02 +44:44:36.6: ref_mag=12.97 +/- 0.01 new_mean_mag=12.0131 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:11.53 +43:02:16.9: 12.98 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:11.53 +43:02:16.9: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Forced photometry filter KEPT candidate at 03:34:11.53 +43:02:16.9: ref_mag=12.98 +/- 0.01 new_mean_mag=11.7429 delta=1.24 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:39:55.72 +45:11:18.6: 12.96 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:39:55.72 +45:11:18.6: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 03:39:55.72 +45:11:18.6: ref_mag=12.96 +/- 0.01 new_mean_mag=11.8966 delta=1.07 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:07.95 +45:05:07.4: 12.96 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:32:27.72 +42:51:24.1: 12.95 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:07.95 +45:05:07.4: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 03:42:07.95 +45:05:07.4: ref_mag=12.97 +/- 0.01 new_mean_mag=12.0167 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:32:27.72 +42:51:24.1: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 03:32:27.72 +42:51:24.1: ref_mag=12.95 +/- 0.01 new_mean_mag=11.9503 delta=1.00 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:35:22.83 +43:45:28.0: 12.93 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:35:22.83 +43:45:28.0: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter KEPT candidate at 03:35:22.83 +43:45:28.0: ref_mag=12.94 +/- 0.01 new_mean_mag=11.8745 delta=1.07 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:40:23.15 +44:48:01.9: 12.92 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:40:23.15 +44:48:01.9: 12.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 03:40:23.15 +44:48:01.9: ref_mag=12.89 +/- 0.01 new_mean_mag=11.8466 delta=1.05 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:18.16 +43:29:34.1: 12.92 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:18.16 +43:29:34.1: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry filter KEPT candidate at 03:33:18.16 +43:29:34.1: ref_mag=12.92 +/- 0.01 new_mean_mag=11.9191 delta=1.00 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:38:28.37 +44:25:35.7: 12.88 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:55.90 +45:53:12.1: 12.88 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:38:28.37 +44:25:35.7: 12.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Forced photometry filter KEPT candidate at 03:38:28.37 +44:25:35.7: ref_mag=12.87 +/- 0.01 new_mean_mag=11.9585 delta=0.91 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:55.90 +45:53:12.1: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 03:41:55.90 +45:53:12.1: ref_mag=12.90 +/- 0.01 new_mean_mag=11.9274 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:29.93 +45:09:05.7: 12.86 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:29.93 +45:09:05.7: 12.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter KEPT candidate at 03:42:29.93 +45:09:05.7: ref_mag=12.83 +/- 0.01 new_mean_mag=11.8153 delta=1.01 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:38.99 +43:45:01.4: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:38.99 +43:45:01.4: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter KEPT candidate at 03:33:38.99 +43:45:01.4: ref_mag=12.83 +/- 0.01 new_mean_mag=11.8558 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:33.14 +45:13:33.9: 12.83 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:33.14 +45:13:33.9: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 03:41:33.14 +45:13:33.9: ref_mag=12.85 +/- 0.01 new_mean_mag=11.8645 delta=0.99 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:36:12.70 +44:13:03.3: 12.80 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:24.52 +45:07:02.0: 12.80 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:36:12.70 +44:13:03.3: 12.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 03:36:12.70 +44:13:03.3: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8573 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:24.52 +45:07:02.0: 12.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 03:42:24.52 +45:07:02.0: ref_mag=12.78 +/- 0.01 new_mean_mag=11.7117 delta=1.07 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:43:20.39 +45:59:44.9: 12.77 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:44:11.71 +45:55:50.9: 12.77 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:43:20.39 +45:59:44.9: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter KEPT candidate at 03:43:20.39 +45:59:44.9: ref_mag=12.79 +/- 0.01 new_mean_mag=11.8274 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:44:11.71 +45:55:50.9: 12.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter KEPT candidate at 03:44:11.71 +45:55:50.9: ref_mag=12.79 +/- 0.01 new_mean_mag=11.8721 delta=0.92 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:59:53.50 +46:29:06.1: 13.30 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:59:53.50 +46:29:06.1: 13.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter REJECTED candidate at 03:59:53.50 +46:29:06.1: ref_mag=13.30 +/- 0.02 new_mean_mag=12.4570 delta=0.84 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:36:52.38 +43:49:19.2: 12.71 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:37:58.26 +44:00:22.9: 12.67 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:36:52.38 +43:49:19.2: 12.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:37:58.26 +44:00:22.9: 12.66 +/- 0.01 detection
Forced photometry filter KEPT candidate at 03:36:52.38 +43:49:19.2: ref_mag=12.71 +/- 0.01 new_mean_mag=11.7665 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter KEPT candidate at 03:37:58.26 +44:00:22.9: ref_mag=12.66 +/- 0.01 new_mean_mag=11.7411 delta=0.92 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:40:29.28 +45:07:47.4: 12.67 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:40:29.28 +45:07:47.4: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 03:40:29.28 +45:07:47.4: ref_mag=12.69 +/- 0.01 new_mean_mag=11.6262 delta=1.06 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:38.91 +45:50:54.0: 12.70 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:38.91 +45:50:54.0: 12.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 03:41:38.91 +45:50:54.0: ref_mag=12.71 +/- 0.01 new_mean_mag=11.7569 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:13.01 +44:57:17.8: 12.66 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:13.01 +44:57:17.8: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 03:41:13.01 +44:57:17.8: ref_mag=12.64 +/- 0.01 new_mean_mag=11.7023 delta=0.93 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:07.77 +43:36:16.0: 12.65 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:34:42.13 +43:28:20.4: 12.63 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:07.77 +43:36:16.0: 12.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 03:34:07.77 +43:36:16.0: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6416 delta=1.02 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:34:42.13 +43:28:20.4: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 03:34:42.13 +43:28:20.4: ref_mag=12.64 +/- 0.01 new_mean_mag=11.6762 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:58.26 +43:50:23.9: 12.64 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:58.26 +43:50:23.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 03:33:58.26 +43:50:23.9: ref_mag=12.63 +/- 0.01 new_mean_mag=11.7178 delta=0.91 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:40:37.20 +45:04:22.3: 12.63 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:40:37.20 +45:04:22.3: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 03:40:37.20 +45:04:22.3: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6584 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:31:13.68 +43:07:20.7: 12.63 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:31:13.68 +43:07:20.7: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter KEPT candidate at 03:31:13.68 +43:07:20.7: ref_mag=12.62 +/- 0.01 new_mean_mag=11.7143 delta=0.91 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:18.74 +45:06:56.5: 12.61 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:18.74 +45:06:56.5: 12.62 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:41.31 +45:25:02.5: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter KEPT candidate at 03:42:18.74 +45:06:56.5: ref_mag=12.62 +/- 0.01 new_mean_mag=11.7115 delta=0.91 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:41.31 +45:25:02.5: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter KEPT candidate at 03:41:41.31 +45:25:02.5: ref_mag=12.60 +/- 0.01 new_mean_mag=11.6629 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:53.09 +45:43:21.0: 12.56 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:53.09 +45:43:21.0: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 03:42:53.09 +45:43:21.0: ref_mag=12.57 +/- 0.01 new_mean_mag=11.6131 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:45.44 +46:03:15.5: 12.07 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:45.44 +46:03:15.5: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry filter REJECTED candidate at 04:00:45.44 +46:03:15.5: ref_mag=12.07 +/- 0.01 new_mean_mag=11.5415 delta=0.53 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:52.92 +43:44:15.4: 12.48 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:52.92 +43:44:15.4: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter KEPT candidate at 03:33:52.92 +43:44:15.4: ref_mag=12.49 +/- 0.01 new_mean_mag=11.5222 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:36:19.51 +44:08:00.2: 12.36 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:44:20.93 +45:45:18.3: 12.29 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:36:19.51 +44:08:00.2: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 03:36:19.51 +44:08:00.2: ref_mag=12.36 +/- 0.01 new_mean_mag=11.4413 delta=0.92 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:43:24.02 +45:46:46.7: 12.19 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:44:20.93 +45:45:18.3: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter KEPT candidate at 03:44:20.93 +45:45:18.3: ref_mag=12.29 +/- 0.01 new_mean_mag=11.3458 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:43:24.02 +45:46:46.7: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry filter KEPT candidate at 03:43:24.02 +45:46:46.7: ref_mag=12.19 +/- 0.01 new_mean_mag=11.2777 delta=0.91 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:21.19 +46:48:32.2: 9.30 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:21.19 +46:48:32.2: 9.29 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.29 +/- 0.00
Forced photometry filter REJECTED candidate at 04:00:21.19 +46:48:32.2: ref_mag=9.29 +/- 0.00 new_mean_mag=9.5449 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:00:46.60 +46:31:26.3: 12.85 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:00:46.60 +46:31:26.3: 12.87 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:58:39.19 +46:14:12.0: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter REJECTED candidate at 04:00:46.60 +46:31:26.3: ref_mag=12.86 +/- 0.01 new_mean_mag=12.1182 delta=0.74 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:01:10.28 +46:00:59.4: 12.99 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:58:39.19 +46:14:12.0: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry filter REJECTED candidate at 03:58:39.19 +46:14:12.0: ref_mag=12.04 +/- 0.01 new_mean_mag=11.5914 delta=0.45 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:01:10.28 +46:00:59.4: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry filter REJECTED candidate at 04:01:10.28 +46:00:59.4: ref_mag=12.99 +/- 0.01 new_mean_mag=12.2727 delta=0.72 (need > 0.90)
Adding exclusion_list_local.txt__out24616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93436.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 84s
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: 36s
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Considering the candidate 212359_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212359_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:32:59.48 +43:43:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212376_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212376_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 04:01:25.99 +47:27:01.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 212410_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212410_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 04:00:20.51 +47:34:17.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 212434_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212434_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 212435_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212435_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:59:44.73 +48:09:04.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 212448_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212448_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 212463_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212463_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 212479_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212479_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 212504_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212504_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 212506_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212506_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 212532_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212532_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:59:21.18 +48:45:43.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 212536_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212536_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 04:00:50.92 +48:14:37.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 212581_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212581_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 212598_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212598_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 212601_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212601_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 212603_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212603_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
Rejecting candidate due to large distance (56.6") between the two second-epoch detections
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Considering the candidate 212634_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212634_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 212665_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212665_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 212670_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212670_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 212672_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212672_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:56:49.05 +46:55:16.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 212690_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212690_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:56:12.59 +46:57:08.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 212737_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212737_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212756_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212756_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212758_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212758_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212765_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212765_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212771_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212771_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212802_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212802_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212809_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212809_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212824_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212824_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:57:02.77 +47:28:46.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212829_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212829_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212830_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212830_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212834_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212834_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212865_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212865_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212873_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212873_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212902_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212902_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212932_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212932_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
Rejecting candidate due to large distance (34.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212933_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212933_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212959_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 212959_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213026_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213026_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213027_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213027_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213034_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213034_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213053_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213053_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213063_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213063_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213098_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213098_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213232_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213232_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:44:45.13 +46:07:13.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 213236_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213236_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213243_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213243_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213280_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213280_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213295_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213295_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213312_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213312_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213320_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213320_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213327_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213327_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213399_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213399_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213411_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213411_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213420_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213420_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213432_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213432_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213437_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213437_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213462_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213462_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213465_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213465_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213502_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213502_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213530_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213530_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213542_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213542_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:32:14.51 +42:45:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213547_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213547_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213556_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213556_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
Rejecting candidate due to large distance (55.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213559_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213559_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213568_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213568_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213600_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213600_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213603_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213603_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213626_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213626_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
Rejecting candidate due to large distance (59.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213636_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213636_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213655_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213655_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
Rejecting candidate due to large distance (53.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213656_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213656_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213664_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213664_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213679_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213679_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213683_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213683_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213687_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213687_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213688_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213688_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213715_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213715_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:59:54.78 +48:32:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213727_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213727_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213729_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213729_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213739_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213739_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213780_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213780_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213824_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213824_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
Rejecting candidate due to large distance (78.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213827_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213827_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213830_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213830_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213849_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213849_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213861_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 213861_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166963_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 166963_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:09:07.73 +49:36:44.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139144_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 139144_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:24:19.72 +49:51:34.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133414_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 133414_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:42:55.35 +47:47:12.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 66312_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 66312_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:29:23.33 +44:24:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96878_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 96878_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 47663_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 47663_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 48307_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 48307_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 88256_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 88256_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
Rejecting candidate due to large distance (32.4") between the two second-epoch detections
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Considering the candidate 57299_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 57299_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 41898_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 41898_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 45264_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 45264_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 41826_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 41826_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 76502_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 76502_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 90776_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 90776_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 24616_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 24616_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 31079_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 31079_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 30342_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 30342_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 83082_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 83082_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 74375_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 74375_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 75882_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 75882_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 65274_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 65274_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 88296_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 88296_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 59407_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 59407_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 107689_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 107689_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 54805_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 54805_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 42745_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 42745_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 89245_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 89245_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 110020_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 110020_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 114648_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 114648_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 107007_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 107007_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 103339_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 103339_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 97102_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 97102_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 105728_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 105728_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 118059_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 118059_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 95886_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 95886_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 46424_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 46424_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 50788_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 50788_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 78004_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 78004_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 60082_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 60082_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
Rejecting candidate due to large distance (29.5") between the two second-epoch detections
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Considering the candidate 79784_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 79784_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 65545_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 65545_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 78463_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 78463_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 45913_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 45913_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 84086_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 84086_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 54778_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 54778_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 66788_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 66788_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
Rejecting candidate due to large distance (57.5") between the two second-epoch detections
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Considering the candidate 79768_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 79768_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 42626_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 42626_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 68884_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 68884_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 37728_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 37728_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 77932_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 77932_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 75301_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 75301_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 35051_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 35051_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 50898_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 50898_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 69894_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 69894_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 46486_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 46486_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 62887_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 62887_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 91475_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 91475_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 76628_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 76628_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 51293_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 51293_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 78339_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 78339_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 59477_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 59477_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 76361_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 76361_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 93436_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 93436_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 91961_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 91961_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 101714_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 101714_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
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Considering the candidate 59335_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 59335_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
Rejecting candidate due to large distance (28.4") between the two second-epoch detections
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Considering the candidate 52369_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 52369_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 54939_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 54939_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 76842_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 76842_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 90940_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 90940_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 72840_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 72840_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 48394_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 48394_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 45829_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 45829_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 53340_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 53340_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 75435_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 75435_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
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Considering the candidate 40109_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 40109_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76005_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 76005_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82122_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 82122_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88209_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 88209_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93262_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 93262_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50978_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 50978_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57821_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 57821_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88715_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 88715_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89477_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
Preparing report for the candidate 89477_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108551_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 108551_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102837_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 102837_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97065_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 97065_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92533_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 92533_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100381_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 100381_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:32:26.14 +46:03:22.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97528_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 97528_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:44:40.80 +46:05:58.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89159_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 89159_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:45:59.19 +45:40:54.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170155_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 170155_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:36:29.42 +48:11:32.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138730_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 138730_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:30:34.55 +47:59:41.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50351_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 50351_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 03:21:26.47 +43:19:48.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138522_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150
The candidate 138522_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150 did not pass the final checks
**** FOUND 02:59:50.02 +47:13:15.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 125s
Prepared the HTML report for the field Per-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
03:27:39.05 +42:10:18.4
03:28:53.69 +42:31:36.0
03:29:33.66 +42:34:46.1
03:32:27.72 +42:51:24.1
03:34:11.53 +43:02:16.9
03:31:13.68 +43:07:20.7
03:35:38.55 +43:16:00.6
03:34:36.64 +43:15:08.9
03:34:57.24 +43:18:47.8
03:34:52.61 +43:18:56.9
03:33:59.53 +43:26:09.2
03:34:42.13 +43:28:20.4
03:34:32.01 +43:28:57.9
03:35:23.14 +43:30:45.8
03:33:18.16 +43:29:34.1
03:33:09.83 +43:31:03.9
03:34:29.36 +43:36:01.8
03:34:07.77 +43:36:16.0
03:35:16.23 +43:44:58.5
03:35:22.83 +43:45:28.0
03:33:52.92 +43:44:15.4
03:33:38.99 +43:45:01.4
03:36:52.38 +43:49:19.2
03:33:58.26 +43:50:23.9
03:38:32.99 +44:00:24.8
03:37:58.26 +44:00:22.9
03:37:10.34 +44:06:13.9
03:36:19.51 +44:08:00.2
03:37:40.96 +44:13:55.2
03:36:12.70 +44:13:03.3
03:38:28.37 +44:25:35.7
03:37:07.16 +44:30:43.0
03:33:30.82 +44:30:11.2
03:39:32.02 +44:44:36.6
03:40:23.15 +44:48:01.9
03:41:13.01 +44:57:17.8
03:40:44.47 +45:01:36.1
03:42:07.95 +45:05:07.4
03:40:37.20 +45:04:22.3
03:39:37.87 +45:04:49.7
03:42:18.74 +45:06:56.5
03:42:24.52 +45:07:02.0
03:42:29.93 +45:09:05.7
03:40:29.28 +45:07:47.4
03:39:55.72 +45:11:18.6
03:42:38.54 +45:13:07.7
03:41:33.14 +45:13:33.9
03:41:28.22 +45:13:25.8
03:38:14.55 +45:14:36.4
03:41:41.31 +45:25:02.5
03:42:09.48 +45:31:10.8
03:42:53.09 +45:43:21.0
03:43:26.70 +45:44:00.1
03:44:20.93 +45:45:18.3
03:43:04.60 +45:47:30.8
03:43:24.02 +45:46:46.7
03:41:38.91 +45:50:54.0
03:41:55.90 +45:53:12.1
03:44:11.71 +45:55:50.9
03:43:20.39 +45:59:44.9
Source monitoring: measuring positions from /data_ssd/NMW-TexasTech/workdir/img_2026-09-06_CI_Per-02-Q2b1x1_232738_TTUQ2b1x1_2991255_uPH1YjTj/monitoring_positions.txt
Read 12468 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.5128 to 66.1654 deg, Dec +40.2533 to +51.2384 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 41.5128 to 66.1654 deg, Dec 40.2533 to 51.2384 deg
Loaded 11904 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): 5394 out of 5529 total matches.
Matched with Tycho-2 5529 out of 12468 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits via Tycho-2
util/pixel_flux_airmass_correction processing wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits
Observation time (mid-exposure, UTC): JD 2461290.68394 (FITS header)
Observing site: lat= +33.748292 deg lon= -101.958319 deg east-positive (SITELAT/SITELONG FITS header keywords)
Frame center (pixel 4788.5 3194.5): RA= 54.00610 deg Dec= +45.99659 deg
Frame center: alt= +15.365 deg az= 49.741 deg airmass= 3.7114
Header cross-check: CENTALT= 15.169 deg (difference +0.196 deg)
Header cross-check: AIRMASS= 3.7702 (we compute 3.7114)
Airmass zero-point fit: REJECT_K_RANGE k= -0.3253 +/- 0.0122 mag/airmass N= 3722 airmass span 2.3726-6.5954 scatter 0.6981 mag
Source monitoring: airmass zero-point for wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits: REJECT_K_RANGE -1.211429 +0.325307 3.7114 -0.3253 3722 4.2227 0.6981 2.3726 6.5954
Forced photometry (list mode): image=wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits list=monitoring_pixlist3175238.tmp aperture=4.2
Image size: 9576 x 6388
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
Saturation level: 57000.0
Calibration (from calib.txt_param_monitoring, fit_function=3): cal_mag = 0.000000 * x^2 + 1.000000 * x + 19.872200
Forced photometry: center=(4226.38, 1949.76) aperture=4.2
Annulus: inner=8.40 outer=21.00
Background annulus: 1166 pixels
Iterative clipping converged after 2 iterations, 1160/1166 pixels remain
SExtractor background: mode=1270.38 median=1269.00 mean=1268.08 sigma=51.69 -> bg=1270.38 (1160 pixels)
Aperture sum=20226.43 N_eff=13.8544
Net flux=2626.07 noise=192.40 SNR=13.65
Instrumental magnitude: -8.5483
Calibrated magnitude: 11.3239
Source monitoring: 1 position(s) measured on wcs_fd_Per-02-Q2b1x1_2026-09-06_23-24-42_20.00sec_-0.00C_LIGHT_0149.fits (aperture 4.2 pix)
Read 12747 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.5120 to 66.1651 deg, Dec +40.2538 to +51.2419 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 41.5120 to 66.1651 deg, Dec 40.2538 to 51.2419 deg
Loaded 11910 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): 5470 out of 5613 total matches.
Matched with Tycho-2 5613 out of 12747 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits via Tycho-2
util/pixel_flux_airmass_correction processing wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits
Observation time (mid-exposure, UTC): JD 2461290.68475 (FITS header)
Observing site: lat= +33.748292 deg lon= -101.958319 deg east-positive (SITELAT/SITELONG FITS header keywords)
Frame center (pixel 4788.5 3194.5): RA= 53.99898 deg Dec= +46.00720 deg
Frame center: alt= +15.546 deg az= 49.848 deg airmass= 3.6706
Header cross-check: CENTALT= 15.339 deg (difference +0.207 deg)
Header cross-check: AIRMASS= 3.7307 (we compute 3.6706)
Airmass zero-point fit: REJECT_K_RANGE k= -0.3400 +/- 0.0126 mag/airmass N= 3650 airmass span 2.3575-6.3876 scatter 0.7011 mag
Source monitoring: airmass zero-point for wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits: REJECT_K_RANGE -1.261462 +0.339961 3.6706 -0.3400 3650 4.0300 0.7011 2.3575 6.3876
Forced photometry (list mode): image=wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits list=monitoring_pixlist3175238.tmp aperture=4.3
Image size: 9576 x 6388
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
Saturation level: 57000.0
Calibration (from calib.txt_param_monitoring, fit_function=3): cal_mag = 0.000000 * x^2 + 1.000000 * x + 19.921550
Forced photometry: center=(4229.40, 1943.16) aperture=4.3
Annulus: inner=8.60 outer=21.50
Background annulus: 1217 pixels
Iterative clipping converged after 1 iterations, 1215/1217 pixels remain
SExtractor background: mode=1259.07 median=1261.00 mean=1262.29 sigma=51.98 -> bg=1259.07 (1215 pixels)
Aperture sum=21316.16 N_eff=14.5220
Net flux=3031.91 noise=198.07 SNR=15.31
Instrumental magnitude: -8.7043
Calibrated magnitude: 11.2173
Source monitoring: 1 position(s) measured on wcs_fd_Per-02-Q2b1x1_2026-09-06_23-25-52_20.00sec_0.00C_LIGHT_0150.fits (aperture 4.3 pix)
########### Completed Per-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
03:33:09.83 +43:31:03.9
03:34:29.36 +43:36:01.8
03:37:10.34 +44:06:13.9
03:34:36.64 +43:15:08.9
03:33:59.53 +43:26:09.2
03:35:38.55 +43:16:00.6
03:27:39.05 +42:10:18.4
03:29:33.66 +42:34:46.1
03:28:53.69 +42:31:36.0
03:40:44.47 +45:01:36.1
03:39:37.87 +45:04:49.7
03:37:07.16 +44:30:43.0
03:43:26.70 +45:44:00.1
03:37:40.96 +44:13:55.2
03:38:32.99 +44:00:24.8
03:34:52.61 +43:18:56.9
03:43:04.60 +45:47:30.8
03:35:23.14 +43:30:45.8
03:35:16.23 +43:44:58.5
03:42:38.54 +45:13:07.7
03:33:30.82 +44:30:11.2
03:41:28.22 +45:13:25.8
03:34:32.01 +43:28:57.9
03:42:09.48 +45:31:10.8
03:31:11.93 +43:54:15.2
03:38:14.55 +45:14:36.4
03:34:57.24 +43:18:47.8
03:39:32.02 +44:44:36.6
03:34:11.53 +43:02:16.9
03:39:55.72 +45:11:18.6
03:42:07.95 +45:05:07.4
03:32:27.72 +42:51:24.1
03:35:22.83 +43:45:28.0
03:40:23.15 +44:48:01.9
03:33:18.16 +43:29:34.1
03:38:28.37 +44:25:35.7
03:41:55.90 +45:53:12.1
03:42:29.93 +45:09:05.7
03:33:38.99 +43:45:01.4
03:41:33.14 +45:13:33.9
03:36:12.70 +44:13:03.3
03:42:24.52 +45:07:02.0
03:43:20.39 +45:59:44.9
03:44:11.71 +45:55:50.9
03:36:52.38 +43:49:19.2
03:37:58.26 +44:00:22.9
03:40:29.28 +45:07:47.4
03:41:38.91 +45:50:54.0
03:41:13.01 +44:57:17.8
03:34:07.77 +43:36:16.0
03:34:42.13 +43:28:20.4
03:33:58.26 +43:50:23.9
03:40:37.20 +45:04:22.3
03:31:13.68 +43:07:20.7
03:42:18.74 +45:06:56.5
03:41:41.31 +45:25:02.5
03:42:53.09 +45:43:21.0
03:33:52.92 +43:44:15.4
03:36:19.51 +44:08:00.2
03:44:20.93 +45:45:18.3
03:43:24.02 +45:46:46.7
###################################################################################
03:33:09.83 +43:31:03.9 -- not an asteroid (will add it to exclusion list)
03:34:29.36 +43:36:01.8 -- not an asteroid (will add it to exclusion list)
03:37:10.34 +44:06:13.9 -- not an asteroid (will add it to exclusion list)
03:34:36.64 +43:15:08.9 -- not an asteroid (will add it to exclusion list)
03:33:59.53 +43:26:09.2 -- not an asteroid (will add it to exclusion list)
03:35:38.55 +43:16:00.6 -- not an asteroid (will add it to exclusion list)
03:27:39.05 +42:10:18.4 -- not an asteroid (will add it to exclusion list)
03:29:33.66 +42:34:46.1 -- not an asteroid (will add it to exclusion list)
03:28:53.69 +42:31:36.0 -- not an asteroid (will add it to exclusion list)
03:40:44.47 +45:01:36.1 -- not an asteroid (will add it to exclusion list)
03:39:37.87 +45:04:49.7 -- not an asteroid (will add it to exclusion list)
03:37:07.16 +44:30:43.0 -- not an asteroid (will add it to exclusion list)
03:43:26.70 +45:44:00.1 -- not an asteroid (will add it to exclusion list)
03:37:40.96 +44:13:55.2 -- not an asteroid (will add it to exclusion list)
03:38:32.99 +44:00:24.8 -- not an asteroid (will add it to exclusion list)
03:34:52.61 +43:18:56.9 -- not an asteroid (will add it to exclusion list)
03:43:04.60 +45:47:30.8 -- not an asteroid (will add it to exclusion list)
03:35:23.14 +43:30:45.8 -- not an asteroid (will add it to exclusion list)
03:35:16.23 +43:44:58.5 -- not an asteroid (will add it to exclusion list)
03:42:38.54 +45:13:07.7 -- not an asteroid (will add it to exclusion list)
03:33:30.82 +44:30:11.2 -- not an asteroid (will add it to exclusion list)
03:41:28.22 +45:13:25.8 -- not an asteroid (will add it to exclusion list)
03:34:32.01 +43:28:57.9 -- not an asteroid (will add it to exclusion list)
03:42:09.48 +45:31:10.8 -- not an asteroid (will add it to exclusion list)
03:31:11.93 +43:54:15.2 -- listed in neverexclude_list.txt (will NOT add it to exclusion list)
03:38:14.55 +45:14:36.4 -- not an asteroid (will add it to exclusion list)
03:34:57.24 +43:18:47.8 -- not an asteroid (will add it to exclusion list)
03:39:32.02 +44:44:36.6 -- not an asteroid (will add it to exclusion list)
03:34:11.53 +43:02:16.9 -- not an asteroid (will add it to exclusion list)
03:39:55.72 +45:11:18.6 -- not an asteroid (will add it to exclusion list)
03:42:07.95 +45:05:07.4 -- not an asteroid (will add it to exclusion list)
03:32:27.72 +42:51:24.1 -- not an asteroid (will add it to exclusion list)
03:35:22.83 +43:45:28.0 -- not an asteroid (will add it to exclusion list)
03:40:23.15 +44:48:01.9 -- not an asteroid (will add it to exclusion list)
03:33:18.16 +43:29:34.1 -- not an asteroid (will add it to exclusion list)
03:38:28.37 +44:25:35.7 -- not an asteroid (will add it to exclusion list)
03:41:55.90 +45:53:12.1 -- not an asteroid (will add it to exclusion list)
03:42:29.93 +45:09:05.7 -- not an asteroid (will add it to exclusion list)
03:33:38.99 +43:45:01.4 -- not an asteroid (will add it to exclusion list)
03:41:33.14 +45:13:33.9 -- not an asteroid (will add it to exclusion list)
03:36:12.70 +44:13:03.3 -- not an asteroid (will add it to exclusion list)
03:42:24.52 +45:07:02.0 -- not an asteroid (will add it to exclusion list)
03:43:20.39 +45:59:44.9 -- not an asteroid (will add it to exclusion list)
03:44:11.71 +45:55:50.9 -- not an asteroid (will add it to exclusion list)
03:36:52.38 +43:49:19.2 -- not an asteroid (will add it to exclusion list)
03:37:58.26 +44:00:22.9 -- not an asteroid (will add it to exclusion list)
03:40:29.28 +45:07:47.4 -- not an asteroid (will add it to exclusion list)
03:41:38.91 +45:50:54.0 -- not an asteroid (will add it to exclusion list)
03:41:13.01 +44:57:17.8 -- not an asteroid (will add it to exclusion list)
03:34:07.77 +43:36:16.0 -- not an asteroid (will add it to exclusion list)
03:34:42.13 +43:28:20.4 -- not an asteroid (will add it to exclusion list)
03:33:58.26 +43:50:23.9 -- not an asteroid (will add it to exclusion list)
03:40:37.20 +45:04:22.3 -- not an asteroid (will add it to exclusion list)
03:31:13.68 +43:07:20.7 -- not an asteroid (will add it to exclusion list)
03:42:18.74 +45:06:56.5 -- not an asteroid (will add it to exclusion list)
03:41:41.31 +45:25:02.5 -- not an asteroid (will add it to exclusion list)
03:42:53.09 +45:43:21.0 -- not an asteroid (will add it to exclusion list)
03:33:52.92 +43:44:15.4 -- not an asteroid (will add it to exclusion list)
03:36:19.51 +44:08:00.2 -- not an asteroid (will add it to exclusion list)
03:44:20.93 +45:45:18.3 -- not an asteroid (will add it to exclusion list)
03:43:24.02 +45:46:46.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:27:39.05 +42:10:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:28:53.69 +42:31:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:29:33.66 +42:34:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:31:13.68 +43:07:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:32:27.72 +42:51:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:09.83 +43:31:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:18.16 +43:29:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:30.82 +44:30:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:38.99 +43:45:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:52.92 +43:44:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:58.26 +43:50:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:59.53 +43:26:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:07.77 +43:36:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:11.53 +43:02:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:29.36 +43:36:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:32.01 +43:28:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:36.64 +43:15:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:42.13 +43:28:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:52.61 +43:18:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:57.24 +43:18:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:16.23 +43:44:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:22.83 +43:45:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:23.14 +43:30:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:38.55 +43:16:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:12.70 +44:13:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:19.51 +44:08:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:52.38 +43:49:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:07.16 +44:30:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:10.34 +44:06:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:40.96 +44:13:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:58.26 +44:00:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:14.55 +45:14:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:28.37 +44:25:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:32.99 +44:00:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:32.02 +44:44:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:37.87 +45:04:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:55.72 +45:11:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:23.15 +44:48:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:29.28 +45:07:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:37.20 +45:04:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:44.47 +45:01:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:13.01 +44:57:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:28.22 +45:13:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:33.14 +45:13:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:38.91 +45:50:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:41.31 +45:25:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:55.90 +45:53:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:07.95 +45:05:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:09.48 +45:31:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:18.74 +45:06:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:24.52 +45:07:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:29.93 +45:09:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:38.54 +45:13:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:53.09 +45:43:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:04.60 +45:47:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:20.39 +45:59:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:24.02 +45:46:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:26.70 +45:44:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:11.71 +45:55:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:20.93 +45:45:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
03:27:39.05 +42:10:18.4 -- not a known variable star
03:28:53.69 +42:31:36.0 -- not a known variable star
03:29:33.66 +42:34:46.1 -- not a known variable star
03:31:13.68 +43:07:20.7 -- not a known variable star
03:32:27.72 +42:51:24.1 -- not a known variable star
03:33:09.83 +43:31:03.9 -- a known variable star
03:33:18.16 +43:29:34.1 -- not a known variable star
03:33:30.82 +44:30:11.2 -- not a known variable star
03:33:38.99 +43:45:01.4 -- not a known variable star
03:33:52.92 +43:44:15.4 -- not a known variable star
03:33:58.26 +43:50:23.9 -- not a known variable star
03:33:59.53 +43:26:09.2 -- not a known variable star
03:34:07.77 +43:36:16.0 -- not a known variable star
03:34:11.53 +43:02:16.9 -- a known variable star
03:34:29.36 +43:36:01.8 -- a known variable star
03:34:32.01 +43:28:57.9 -- a known variable star
03:34:36.64 +43:15:08.9 -- not a known variable star
03:34:42.13 +43:28:20.4 -- not a known variable star
03:34:52.61 +43:18:56.9 -- a known variable star
03:34:57.24 +43:18:47.8 -- not a known variable star
03:35:16.23 +43:44:58.5 -- not a known variable star
03:35:22.83 +43:45:28.0 -- not a known variable star
03:35:23.14 +43:30:45.8 -- not a known variable star
03:35:38.55 +43:16:00.6 -- not a known variable star
03:36:12.70 +44:13:03.3 -- not a known variable star
03:36:19.51 +44:08:00.2 -- not a known variable star
03:36:52.38 +43:49:19.2 -- not a known variable star
03:37:07.16 +44:30:43.0 -- not a known variable star
03:37:10.34 +44:06:13.9 -- not a known variable star
03:37:40.96 +44:13:55.2 -- not a known variable star
03:37:58.26 +44:00:22.9 -- not a known variable star
03:38:14.55 +45:14:36.4 -- not a known variable star
03:38:28.37 +44:25:35.7 -- not a known variable star
03:38:32.99 +44:00:24.8 -- not a known variable star
03:39:32.02 +44:44:36.6 -- not a known variable star
03:39:37.87 +45:04:49.7 -- not a known variable star
03:39:55.72 +45:11:18.6 -- not a known variable star
03:40:23.15 +44:48:01.9 -- not a known variable star
03:40:29.28 +45:07:47.4 -- not a known variable star
03:40:37.20 +45:04:22.3 -- not a known variable star
03:40:44.47 +45:01:36.1 -- not a known variable star
03:41:13.01 +44:57:17.8 -- not a known variable star
03:41:28.22 +45:13:25.8 -- not a known variable star
03:41:33.14 +45:13:33.9 -- not a known variable star
03:41:38.91 +45:50:54.0 -- a known variable star
03:41:41.31 +45:25:02.5 -- not a known variable star
03:41:55.90 +45:53:12.1 -- not a known variable star
03:42:07.95 +45:05:07.4 -- not a known variable star
03:42:09.48 +45:31:10.8 -- not a known variable star
03:42:18.74 +45:06:56.5 -- not a known variable star
03:42:24.52 +45:07:02.0 -- not a known variable star
03:42:29.93 +45:09:05.7 -- not a known variable star
03:42:38.54 +45:13:07.7 -- not a known variable star
03:42:53.09 +45:43:21.0 -- not a known variable star
03:43:04.60 +45:47:30.8 -- not a known variable star
03:43:20.39 +45:59:44.9 -- a known variable star
03:43:24.02 +45:46:46.7 -- not a known variable star
03:43:26.70 +45:44:00.1 -- not a known variable star
03:44:11.71 +45:55:50.9 -- not a known variable star
03:44:20.93 +45:45:18.3 -- a known variable star
Found 52 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
60 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 60 (excluding asteroids and hot pixels, 52 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)2461290.68393600 -observatory V36
11:38:11.48 +03:32:50.6 Mercury (-0.9mag)
13:35:46.90 -14:28:37.1 Venus (-4.7mag)
07:13:41.09 +22:59:18.4 Mars (1.2mag)
09:08:57.43 +16:57:56.3 Jupiter (-1.8mag)
00:51:45.57 +02:38:48.8 Saturn (0.4mag)
04:13:41.20 +21:01:59.2 Uranus (5.7mag)
00:13:45.45 -00:03:09.3 Neptune (7.7mag)
20:25:36.07 -23:39:35.5 Pluto (14.5mag)
07:39:08.35 +23:56:01.3 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 362 Sep 7 00:32 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461290.68393600:
09:09:03.01 +16:57:29.1 Io (6.2mag)
09:08:54.98 +16:58:09.6 Europa (6.3mag)
09:09:08.11 +16:57:02.5 Ganymede (5.7mag)
09:08:32.48 +16:59:59.2 Callisto (6.9mag)
09:06:43.45 +17:14:25.5 Himalia (15.7mag)
09:09:00.10 +16:57:44.1 Thebe (16.6mag)
09:06:20.76 +17:08:24.6 Elara (17.7mag)
09:12:51.23 +16:25:32.8 Pasiphae (17.9mag)
09:10:02.97 +17:15:41.1 Carme (19.0mag)
00:51:42.10 +02:39:12.2 Titan (8.3mag)
00:51:38.89 +02:38:44.1 Rhea (9.6mag)
00:52:01.08 +02:41:20.3 Iapetus (11.0mag)
00:51:59.53 +02:38:14.9 Hyperion (14.3mag)
00:50:32.46 +02:28:33.7 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 7 00:32 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461290.68393600:
22:04:07.81 +00:53:16.8 JWST
17:31:39.85 +37:21:36.3 Chandra
09:46:02.33 -54:43:18.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 7 00:32 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461290.68393600 -observatory V36
03:40:21.47 +19:20:05.8 17.4mag P/1996 R2 (Lagerkvist)
18:02:52.24 -34:12:48.9 14.3mag P/2010 H2 (Vales)
07:19:23.11 -70:17:42.9 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:15:40.79 +33:41:50.5 17.7mag C/2017 K2 (PANSTARRS)
04:51:15.59 +45:27:37.4 15.8mag P/2021 N1 (ZTF)
04:51:15.59 +45:27:37.4 15.8mag P/2021 N1 (ZTF)
04:51:15.59 +45:27:37.4 15.8mag P/2021 N1 (ZTF)
04:51:15.59 +45:27:37.4 15.8mag P/2021 N1 (ZTF)
04:51:15.59 +45:27:37.4 15.8mag P/2021 N1 (ZTF)
22:13:34.57 +28:41:03.2 17.4mag C/2022 E2 (ATLAS)
07:10:06.40 +25:58:51.2 16.9mag C/2022 N2 (PANSTARRS)
10:49:23.57 +27:13:48.5 17.1mag C/2022 QE78 (ATLAS)
09:48:35.88 +05:14:01.3 18.0mag C/2022 R6 (PANSTARRS)
15:29:33.84 -15:38:21.9 14.8mag C/2023 R1 (PANSTARRS)
08:38:17.58 +32:53:06.9 15.8mag C/2024 E1 (Wierzchos)
15:06:34.76 +15:19:27.7 17.9mag C/2024 G6 (ATLAS)
18:33:40.81 +43:10:46.0 13.7mag C/2024 J3 (ATLAS)
20:26:19.49 +49:18:28.0 17.4mag C/2024 R4 (PANSTARRS)
05:35:32.87 -13:01:29.8 15.1mag C/2024 T5 (ATLAS)
07:11:35.50 +18:33:57.5 17.8mag C/2025 J1 (Borisov)
11:17:47.89 +18:46:40.6 16.8mag C/2025 V2 (Rankin)
13:19:31.86 +00:07:31.5 16.8mag C/2025 Y1 (ATLAS)
16:41:05.23 +74:03:12.7 16.1mag C/2026 A2 (Bok)
03:05:51.13 +46:08:18.4 17.4mag C/2026 B2 (Sun-Gao)
12:13:09.97 +11:16:25.5 17.5mag A/2026 E1
22:25:55.33 -35:02:00.6 13.4mag 10P/Tempel
01:19:19.03 +37:00:30.2 17.9mag 11P/Tempel-Swift-LINEAR
11:48:05.70 -05:27:35.0 16.3mag 29P/Schwassmann-Wachmann
12:08:20.47 -05:03:32.6 17.6mag 63P/Wild
00:44:43.92 -07:03:44.4 15.4mag 65P/Gunn
06:39:06.78 +19:15:38.3 17.1mag 78P/Gehrels
03:17:16.55 +14:59:48.6 16.7mag 88P/Howell
05:37:50.77 +28:35:15.1 17.5mag 112P/Urata-Niijima
07:31:27.93 +24:50:42.9 17.9mag 114P/Wiseman-Skiff
10:27:38.38 +20:53:30.1 14.8mag 123P/West-Hartley
12:46:20.94 -21:17:57.8 17.4mag 124P/Mrkos
06:17:16.81 +20:38:33.3 15.9mag 128P/Shoemaker-Holt
02:32:39.43 -17:37:30.4 15.2mag 161P/Hartley-IRAS
09:37:47.74 +13:48:43.7 12.1mag 169P/NEAT
03:24:20.91 +08:29:03.2 14.5mag 220P/McNaught
04:47:46.09 +36:17:05.7 15.2mag 260P/McNaught
08:31:34.41 +35:42:46.9 17.3mag 295P/LINEAR
15:25:09.64 -00:14:11.0 17.9mag 391P/Kowalski
09:27:41.26 +16:51:22.0 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.2K Sep 7 00:32 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -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
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -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
-rw-r--r-- 1 apache apache 5.7K Sep 7 00:32 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
-rw-r--r-- 1 apache apache 190K Sep 7 00:32 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
00:34:06.502 +12:42:13.91 AT 2026ypz 2026-08-08.10 20
21:30:05.008 +02:38:33.95 AT 2026ypy 2026-08-06.53 20.21
21:00:04.179 -04:29:11.16 AT 2026ypx 2026-08-10.99 20.06
02:37:12.256 +15:20:39.63 AT 2026ypw 2026-08-12.19 20.13
20:30:21.422 +77:41:45.40 AT 2026ypv 2026-08-02.23 20.4969
13:32:08.201 +00:21:43.54 AT 2026ypu 2026-08-05.16 19.6868
14:07:14.862 +00:31:05.95 AT 2026ypt 2026-08-08.16 20.0684
17:39:38.555 +44:15:43.22 AT 2026yps 2026-07-22.33 20.9161
23:51:42.078 +03:04:27.33 AT 2026ypr 2026-08-12.07 20.05
02:34:15.880 +40:31:56.36 AT 2026ypq 2026-08-11.58 18.82
15:38:07.902 +06:01:37.84 AT 2026ypp 2026-08-11.26 20.34
15:24:17.953 +11:26:31.29 AT 2026ypo 2026-08-11.26 20.8
14:21:16.003 +25:15:33.98 AT 2026ypn 2026-08-11.26 18.72
16:23:56.085 +09:36:23.21 AT 2026ypm 2026-08-11.28 20.97
20:54:11.595 +10:54:51.15 SN 2026ypl 2026-08-09.34 20.4
00:40:25.122 +24:26:45.82 AT 2026ypk 2026-08-07.45 20.4501
17:05:06.872 +77:16:36.60 AT 2026ypj 2026-08-11.31 18.807
20:49:46.878 -06:36:38.40 AT 2026ypi 2026-08-09.29 20.4359
00:12:21.150 -17:28:55.44 AT 2026yph 2026-08-08.42 20.4034
00:48:58.972 +17:28:17.78 AT 2026ypg 2026-08-05.48 20.2336
-rw-r--r-- 1 apache apache 88K Sep 7 00:32 tns_transients_list.txt
