This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ
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 06.2462 2461289.7462 11.56 03:57:02.78 +34:12:08.7
161.16089 -14.55282 galactic Per Second-epoch detections are separated by 1.1" and 1.3 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 | 03:57:02.78 +34:12:08.7 (user input) | T | P | (position from user input) SpType: A2: 1985CBVMS.C......0V NGC 1499 +34 28 J-Ks=0.127+/-0.028 (A)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:57:02.78 +34:12:08.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:57:02.78 +34:12:08.7: 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 06.2462* 03 57 02.78 +34 12 08.7 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
target,2461289.7462,11.56,0.05,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 20260906.2462 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 11.62 03:57:11.49 +34:09:21.9
161.21592 -14.56738 galactic Per Second-epoch detections are separated by 5.1" and 0.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J059.2878+34.1609 | 03:57:11.49 +34:09:21.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.642+/-0.027 (K)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:57:11.49 +34:09:21.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:57:11.49 +34:09:21.9: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 06.2462* 03 57 11.49 +34 09 21.9 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
ATO J059.2878+34.1609,2461289.7462,11.62,0.05,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
ATO J059.2878+34.1609 20260906.2462 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 06.2462 2461289.7462 11.40 03:46:47.71 +40:01:46.3
155.69068 -11.43508 galactic Per Second-epoch detections are separated by 2.7" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J056.7137+40.0296 | 03:46:47.71 +40:01:46.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.473+/-0.036 (K)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:47.71 +40:01:46.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:47.71 +40:01:46.3: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 06.2462* 03 46 47.71 +40 01 46.3 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 J056.7137+40.0296,2461289.7462,11.40,0.05,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 J056.7137+40.0296 20260906.2462 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 11.29 03:47:23.71 +40:48:46.4
155.27899 -10.75428 galactic Per Second-epoch detections are separated by 0.8" and 1.3 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 J056.8644+40.8153 | 03:47:23.99 +40:48:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:23.71 +40:48:46.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:23.71 +40:48:46.4: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 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 06.2462* 03 47 23.71 +40 48 46.4 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
ATO J056.8644+40.8153,2461289.7462,11.29,0.05,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
ATO J056.8644+40.8153 20260906.2462 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
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 11.28 03:46:55.94 +41:11:10.5
154.97119 -10.51867 galactic Per Second-epoch detections are separated by 0.7" and 1.2 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 225103569610001280 | 03:46:55.85 +41:11:10.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.654+/-0.028 (K)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:55.94 +41:11:10.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:55.94 +41:11:10.5: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2462* 03 46 55.94 +41 11 10.5 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 225103569610001280,2461289.7462,11.28,0.05,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 225103569610001280 20260906.2462 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 11.44 04:03:08.57 +35:54:48.7
160.93091 -12.44709 galactic Per Second-epoch detections are separated by 0.8" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.8067 Helfenstein 512 -193 547 17.0 -0 0
ATTENTION: measured mag 11.44 is 5.6 mag brighter than the predicted asteroid brightness 17.0 - the transient may be an unrelated new object!
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:03:08.57 +35:54:48.7: 12.39 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:03:08.57 +35:54:48.7: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2462* 04 03 08.57 +35 54 48.7 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
VARIABLE_NAME,2461289.7462,11.44,0.05,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
VARIABLE_NAME 20260906.2462 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 06.2462 2461289.7462 11.11 04:33:48.29 +41:05:11.2
161.52690 -4.55345 galactic Per Second-epoch detections are separated by 1.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J068.4517+41.0864 | 04:33:48.41 +41:05:11.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.486+/-0.030 (K)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:33:48.29 +41:05:11.2: 12.36 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:33:48.29 +41:05:11.2: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 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 06.2462* 04 33 48.29 +41 05 11.2 11.1 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
ATO J068.4517+41.0864,2461289.7462,11.11,0.05,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 J068.4517+41.0864 20260906.2462 11.11CV 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 06.2462 2461289.7462 11.27 04:19:27.16 +39:14:05.6
160.96475 -7.81415 galactic Per Second-epoch detections are separated by 0.7" and 1.2 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 227449343307954432 | 04:19:27.23 +39:14:06.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.915+/-0.028 (M)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:19:27.16 +39:14:05.6: 12.33 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:19:27.16 +39:14:05.6: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2462* 04 19 27.16 +39 14 05.6 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 227449343307954432,2461289.7462,11.27,0.05,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 227449343307954432 20260906.2462 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 11.35 04:01:19.83 +34:21:27.8
161.73054 -13.84405 galactic Per Second-epoch detections are separated by 1.9" and 1.7 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 218616962103288960 | 04:01:19.83 +34:21:28.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.397+/-0.032 (G)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:01:19.83 +34:21:27.8: 12.34 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:01:19.83 +34:21:27.8: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2462* 04 01 19.83 +34 21 27.8 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 218616962103288960,2461289.7462,11.35,0.05,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
Gaia DR3 218616962103288960 20260906.2462 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 06.2462 2461289.7462 11.25 03:59:49.97 +33:56:26.8
161.78445 -14.36088 galactic Per Second-epoch detections are separated by 1.6" and 1.4 pix
The object was found in VSX 1" Gaia DR3 218581163554066304
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.110 G 12.140 G F
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:59:49.97 +33:56:26.8: 12.30 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:59:49.97 +33:56:26.8: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2462* 03 59 49.97 +33 56 26.8 11.2 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
Gaia DR3 218581163554066304,2461289.7462,11.25,0.05,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 218581163554066304 20260906.2462 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 11.28 04:00:31.63 +34:05:38.5
161.78766 -14.15070 galactic Per Second-epoch detections are separated by 2.1" and 1.3 pix
The object was found in VSX 0" Gaia DR3 218607307017069184
Type: ROT
# Max. Min./Amp. JD0 Period
12.020 G 12.050 G G
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:00:31.63 +34:05:38.5: 12.22 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:00:31.63 +34:05:38.5: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 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 06.2462* 04 00 31.63 +34 05 38.5 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 218607307017069184,2461289.7462,11.28,0.05,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 218607307017069184 20260906.2462 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.95 04:35:28.14 +40:59:21.3
161.81117 -4.38731 galactic Per Second-epoch detections are separated by 0.2" and 1.3 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 J068.8826+40.9850 | 04:35:28.04 +40:59:20.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:28.14 +40:59:21.3: 12.18 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:28.14 +40:59:21.3: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 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 06.2462* 04 35 28.14 +40 59 21.3 10.9 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 J068.8826+40.9850,2461289.7462,10.95,0.05,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 J068.8826+40.9850 20260906.2462 10.95CV 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 06.2462 2461289.7462 11.14 04:19:33.88 +39:00:32.0
161.14181 -7.95833 galactic Per Second-epoch detections are separated by 0.4" and 1.2 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 J064.8912+39.0091 | 04:19:33.89 +39:00:32.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1985A&A...146..123U [UMB85] 27 J-Ks=0.446+/-0.028 (G)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:19:33.88 +39:00:32.0: 12.11 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:19:33.88 +39:00:32.0: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 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 06.2462* 04 19 33.88 +39 00 32.0 11.1 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
ATO J064.8912+39.0091,2461289.7462,11.14,0.05,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 J064.8912+39.0091 20260906.2462 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.77 04:34:19.63 +40:54:44.2
161.72250 -4.59848 galactic Per Second-epoch detections are separated by 1.2" and 1.3 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 J068.5832+40.9167 | 04:34:19.58 +40:54:44.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5) J-Ks=0.176+/-0.028 (F)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:34:19.63 +40:54:44.2: 12.03 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:34:19.63 +40:54:44.2: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 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 06.2462* 04 34 19.63 +40 54 44.2 10.8 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 J068.5832+40.9167,2461289.7462,10.77,0.05,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 J068.5832+40.9167 20260906.2462 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.55 04:36:02.40 +41:00:52.7
161.86490 -4.29046 galactic Per Second-epoch detections are separated by 1.5" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J069.0088+41.0119 | 04:36:02.38 +41:00:54.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.848+/-0.026 (M)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:02.40 +41:00:52.7: 11.94 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:02.40 +41:00:52.7: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2462* 04 36 02.40 +41 00 52.7 10.6 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
ATO J069.0088+41.0119,2461289.7462,10.55,0.05,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 J069.0088+41.0119 20260906.2462 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.79 04:37:12.76 +41:06:14.3
161.94690 -4.06650 galactic Per Second-epoch detections are separated by 1.9" and 1.4 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 203850108625493504 | 04:37:12.71 +41:06:15.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.790+/-0.026 (K)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:37:12.76 +41:06:14.3: 11.91 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:37:12.76 +41:06:14.3: 11.85 +/- 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 06.2462* 04 37 12.76 +41 06 14.3 10.8 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 203850108625493504,2461289.7462,10.79,0.05,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 203850108625493504 20260906.2462 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.79 04:36:48.15 +41:12:39.8
161.81534 -4.05221 galactic Per Second-epoch detections are separated by 2.1" and 1.5 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 203854712830402432 | 04:36:48.13 +41:12:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.753+/-0.024 (K)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:48.15 +41:12:39.8: 11.87 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:48.15 +41:12:39.8: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 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 06.2462* 04 36 48.15 +41 12 39.8 10.8 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 203854712830402432,2461289.7462,10.79,0.05,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 203854712830402432 20260906.2462 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.88 04:35:52.94 +41:13:06.8
161.69339 -4.17553 galactic Per Second-epoch detections are separated by 0.8" and 1.3 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 J068.9708+41.2187 | 04:35:52.99 +41:13:07.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.158+/-0.026 (M)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:52.94 +41:13:06.8: 11.85 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:52.94 +41:13:06.8: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 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 06.2462* 04 35 52.94 +41 13 06.8 10.9 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 J068.9708+41.2187,2461289.7462,10.88,0.05,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
ATO J068.9708+41.2187 20260906.2462 10.88CV 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 06.2462 2461289.7462 10.85 04:36:02.98 +41:21:44.5
161.60774 -4.05566 galactic Per Second-epoch detections are separated by 2.3" and 1.1 pix
The object was found in VSX23" Gaia DR3 203906840850464896
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.520 G 14.560 G A
ATTENTION: measured mag 10.85 is 3.7 mag brighter than the VSX record maximum brightness 14.52 - 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:02.98 +41:21:44.5: 11.83 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:02.98 +41:21:44.5: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 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 06.2462* 04 36 02.98 +41 21 44.5 10.8 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 203906840850464896,2461289.7462,10.85,0.05,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 203906840850464896 20260906.2462 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.84 04:36:45.30 +41:11:31.3
161.82350 -4.07159 galactic Per Second-epoch detections are separated by 1.5" and 1.2 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 203854678470694016 | 04:36:45.26 +41:11:31.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.071+/-0.025 (A)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:45.30 +41:11:31.3: 11.79 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:45.30 +41:11:31.3: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 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 06.2462* 04 36 45.30 +41 11 31.3 10.8 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 203854678470694016,2461289.7462,10.84,0.05,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
Gaia DR3 203854678470694016 20260906.2462 10.84CV 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 06.2462 2461289.7462 10.80 04:36:12.69 +41:30:36.9
161.51828 -3.93389 galactic Per Second-epoch detections are separated by 0.2" and 1.2 pix
The object was found in VSX 5" Gaia DR3 203910139385693824
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.670 G 13.710 G B
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:12.69 +41:30:36.9: 11.74 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:12.69 +41:30:36.9: 11.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.74 +/- 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 06.2462* 04 36 12.69 +41 30 36.9 10.8 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 203910139385693824,2461289.7462,10.80,0.05,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 203910139385693824 20260906.2462 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.58 04:35:03.80 +41:07:32.2
161.65840 -4.35209 galactic Per Second-epoch detections are separated by 1.3" and 1.4 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 203874611416040192 | 04:35:03.81 +41:07:32.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.696+/-0.029 (K)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:03.80 +41:07:32.2: 11.65 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:03.80 +41:07:32.2: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2462* 04 35 03.80 +41 07 32.2 10.6 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 203874611416040192,2461289.7462,10.58,0.05,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 203874611416040192 20260906.2462 10.58CV 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 06.2462 2461289.7462 10.62 04:35:05.16 +41:03:15.3
161.71419 -4.39699 galactic Per Second-epoch detections are separated by 0.6" and 1.1 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 J068.7714+41.0540 | 04:35:05.14 +41:03:14.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.232+/-0.028 (F)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:05.16 +41:03:15.3: 11.66 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:05.16 +41:03:15.3: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 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 06.2462* 04 35 05.16 +41 03 15.3 10.6 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
ATO J068.7714+41.0540,2461289.7462,10.62,0.05,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
ATO J068.7714+41.0540 20260906.2462 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.39 04:35:47.16 +40:46:05.3
162.01578 -4.49154 galactic Per Second-epoch detections are separated by 0.1" and 1.1 pix
The object was found in VSX 1" Gaia DR3 203816096782126464
Type: L
# Max. Min./Amp. JD0 Period
10.170 G 10.320 G M
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:47.16 +40:46:05.3: 11.59 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:47.16 +40:46:05.3: 11.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.55 +/- 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 06.2462* 04 35 47.16 +40 46 05.3 10.4 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
Gaia DR3 203816096782126464,2461289.7462,10.39,0.05,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 203816096782126464 20260906.2462 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.45 04:36:42.29 +41:07:39.5
161.86510 -4.12173 galactic Per Second-epoch detections are separated by 1.2" and 1.3 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 J069.1625+41.1204 | 04:36:42.31 +41:07:39.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.447+/-0.024 (G)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:42.29 +41:07:39.5: 11.50 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:42.29 +41:07:39.5: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2462* 04 36 42.29 +41 07 39.5 10.4 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 J069.1625+41.1204,2461289.7462,10.45,0.05,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 J069.1625+41.1204 20260906.2462 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.52 04:33:43.14 +40:56:37.4
161.62137 -4.66191 galactic Per Second-epoch detections are separated by 1.1" and 1.2 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 203876844799163648 | 04:33:43.16 +40:56:38.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.459+/-0.027 (G)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:33:43.14 +40:56:37.4: 11.47 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:33:43.14 +40:56:37.4: 11.47 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.47 +/- 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 06.2462* 04 33 43.14 +40 56 37.4 10.5 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
Gaia DR3 203876844799163648,2461289.7462,10.52,0.05,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 203876844799163648 20260906.2462 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.28 04:36:48.66 +41:08:08.6
161.87250 -4.10147 galactic Per Second-epoch detections are separated by 1.0" and 1.2 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 203851040635804544 | 04:36:48.72 +41:08:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.092+/-0.034 (M)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:48.66 +41:08:08.6: 11.43 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:48.66 +41:08:08.6: 11.39 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.41 +/- 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 06.2462* 04 36 48.66 +41 08 08.6 10.3 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 203851040635804544,2461289.7462,10.28,0.05,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 203851040635804544 20260906.2462 10.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.32 04:35:44.51 +40:56:51.3
161.87683 -4.37718 galactic Per Second-epoch detections are separated by 1.7" and 1.4 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 203821903577813376 | 04:35:44.55 +40:56:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1949AnHar.112....1C HD 276635 J-Ks=0.373+/-0.030 (G)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:44.51 +40:56:51.3: 11.23 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:44.51 +40:56:51.3: 11.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.24 +/- 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 06.2462* 04 35 44.51 +40 56 51.3 10.3 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 203821903577813376,2461289.7462,10.32,0.05,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 203821903577813376 20260906.2462 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.27 04:36:00.85 +40:51:44.0
161.97492 -4.39638 galactic Per Second-epoch detections are separated by 1.2" and 1.1 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 J069.0078+40.8561 | 04:36:00.84 +40:51:43.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.741+/-0.029 (K)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:00.85 +40:51:44.0: 11.20 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:00.85 +40:51:44.0: 11.21 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.21 +/- 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 06.2462* 04 36 00.85 +40 51 44.0 10.3 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
ATO J069.0078+40.8561,2461289.7462,10.27,0.05,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 J069.0078+40.8561 20260906.2462 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.22 04:36:24.82 +40:52:45.6
162.01300 -4.32889 galactic Per Second-epoch detections are separated by 1.0" and 1.1 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 J069.1030+40.8891 | 04:36:24.81 +40:52:45.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.139+/-0.027 (M)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:24.82 +40:52:45.6: 11.13 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:24.82 +40:52:45.6: 11.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.12 +/- 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 06.2462* 04 36 24.82 +40 52 45.6 10.2 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
ATO J069.1030+40.8891,2461289.7462,10.22,0.05,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 J069.1030+40.8891 20260906.2462 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.20 04:36:18.03 +41:07:04.2
161.82122 -4.18481 galactic Per Second-epoch detections are separated by 0.3" and 1.2 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 203848532372451200 | 04:36:18.00 +41:07:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3 1949AnHar.112....1C HD 276627 J-Ks=0.236+/-0.028 (F)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:18.03 +41:07:04.2: 11.12 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:18.03 +41:07:04.2: 11.12 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.12 +/- 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 06.2462* 04 36 18.03 +41 07 04.2 10.2 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
Gaia DR3 203848532372451200,2461289.7462,10.20,0.05,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 203848532372451200 20260906.2462 10.20CV 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 06.2462 2461289.7462 10.23 04:35:17.17 +41:14:06.3
161.60554 -4.24738 galactic Per Second-epoch detections are separated by 0.8" and 1.4 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 J068.8124+41.2322 | 04:35:17.18 +41:14:06.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 1949AnHar.112....1C HD 276624 J-Ks=0.287+/-0.027 (F)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:17.17 +41:14:06.3: 11.10 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:17.17 +41:14:06.3: 11.10 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.10 +/- 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 06.2462* 04 35 17.17 +41 14 06.3 10.2 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
ATO J068.8124+41.2322,2461289.7462,10.23,0.05,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 J068.8124+41.2322 20260906.2462 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.02 04:34:40.03 +41:05:11.2
161.63697 -4.43362 galactic Per Second-epoch detections are separated by 0.8" and 1.1 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 J068.6659+41.0967 | 04:34:40.05 +41:05:12.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.583+/-0.027 (K)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:34:40.03 +41:05:11.2: 10.99 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:34:40.03 +41:05:11.2: 10.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.99 +/- 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 06.2462* 04 34 40.03 +41 05 11.2 10.0 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
ATO J068.6659+41.0967,2461289.7462,10.02,0.05,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 J068.6659+41.0967 20260906.2462 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2462 2461289.7462 10.02 04:34:37.83 +40:56:44.2
161.73660 -4.53370 galactic Per Second-epoch detections are separated by 1.5" and 1.2 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 203871484679933312 | 04:34:37.85 +40:56:44.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.114+/-0.030 (M)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:34:37.83 +40:56:44.2: 10.93 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:34:37.83 +40:56:44.2: 10.92 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.93 +/- 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 06.2462* 04 34 37.83 +40 56 44.2 10.0 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 203871484679933312,2461289.7462,10.02,0.05,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 203871484679933312 20260906.2462 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
First image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Last image: 2461289.74639087 06.09.2026 05:54:38.171 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.58
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: 3 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): 8667
Objects passed selection criteria: 8604
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: 7019
Average stars matched: 5934.25 (84.5455 %)
Memory usage VmPeak: 239816 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 Sun Sep 6 00:59:11 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
First image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Last image: 2461289.74639087 06.09.2026 05:54:38.171 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 344
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
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 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): 71843
Objects passed selection criteria: 71565
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: 57754.8
Average stars matched: 48384.5 (83.7758 %)
Memory usage VmPeak: 570708 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 Sun Sep 6 01:00:04 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
SExtractor catalog cache: saved Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat to cache
SExtractor catalog cache: saved Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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: 2461289.74594986
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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits exists and is non-empty
wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits exists and is non-empty
wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits exists and is non-empty
wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits (1st reference image)
verification OK: wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:21:49.059 +37:59:50.85 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-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits (1st new image)
verification OK: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
Image size: 939.8'x624.3' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:21:50.246 +38:00:07.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:21:49.059 +37:59:50.85
Second-epoch image center 04:21:50.246 +38:00:07.34
Angular distance between the image centers 0.0060 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits (2nd new image)
verification OK: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
Image size: 939.7'x624.3' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:21:49.565 +38:00:07.00 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:21:49.059 +37:59:50.85
Second-epoch image center 04:21:49.565 +38:00:07.00
Angular distance between the image centers 0.0048 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 04:21:50.246 +38:00:07.34
Second-epoch second image center 04:21:49.565 +38:00:07.00
Angular distance between the image centers 0.00224 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits &> /tmp/tmp.TDhcdpftme
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits &> /tmp/tmp.bfHc714sTI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits &> /tmp/tmp.tzYcqwcrpF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits &> /tmp/tmp.cs77UA4DGq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
Found non-empty wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
The reference image (wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits) and catalog (wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat) found
'wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat' -> 'wcsmag.cat'
Read 18677 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.9661 to 76.3326 deg, Dec +32.1948 to +43.3141 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 54.9661 to 76.3326 deg, Dec 32.1948 to 43.3141 deg
Loaded 9192 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): 6385 out of 7127 total matches.
Matched with Tycho-2 7127 out of 18677 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.973500
a=0.000000 b=1.000000 c=22.973500
From vast_summary.log: estimated ref. image limiting mag.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 18677 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.9661 to 76.3326 deg, Dec +32.1948 to +43.3141 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 54.9661 to 76.3326 deg, Dec 32.1948 to 43.3141 deg
Loaded 9192 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): 6385 out of 7127 total matches.
Matched with Tycho-2 7127 out of 18677 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Forced-photometry filter: calibrated wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits -> calib.txt_param_ref_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits (aperture=6.0)
Read 18569 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.4956 to 75.7898 deg, Dec +32.0248 to +43.3806 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 54.4956 to 75.7898 deg, Dec 32.0248 to 43.3806 deg
Loaded 9219 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): 6462 out of 7192 total matches.
Matched with Tycho-2 7192 out of 18569 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Forced-photometry filter: calibrated wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits -> calib.txt_param_ref_wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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:
2.1 pix Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
2.1 pix Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
2.4 pix fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
2.4 pix fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
Limiting magnitude estimates:
15.4 mag. Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
15.4 mag. Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
10.7 mag. fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
10.5 mag. fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
All-image limiting magnitude estimate: 10.5 (SNR ) 9.1 (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.TDhcdpftme (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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS-calibrated image found: wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Checking if the catalog wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat corresponding to the image wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat corresponding to the image wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS catalog name: wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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=1808, bad_region=4135, passed=18677
Got 18677 stars (including 13041 good ones) from the SExtractor catalog wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
util/solve_plate_with_UCAC5 got 18677 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 4850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 15316 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 15316 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 15316 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4849 stars left (next iteration limit 5335)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits N_match=4849 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.425 sigma_q2_arcsec=0.282 sigma_q3_arcsec=0.270 sigma_q4_arcsec=0.243 n_q1=2083 n_q2=782 n_q3=975 n_q4=1009 worst_quadrant_to_overall_ratio=1.313
The image catalog is written to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits -region wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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.bfHc714sTI (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-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits' -> 'wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WCS-calibrated image found: wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Checking if the catalog wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat corresponding to the image wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat corresponding to the image wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WCS catalog name: wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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=1757, bad_region=5749, passed=18569
Got 18569 stars (including 11599 good ones) from the SExtractor catalog wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat
util/solve_plate_with_UCAC5 got 18569 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 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 4877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 13812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 13812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 13812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4878 stars left (next iteration limit 5364)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits N_match=4878 sigma_overall_arcsec=0.396 sigma_q1_arcsec=0.526 sigma_q2_arcsec=0.403 sigma_q3_arcsec=0.350 sigma_q4_arcsec=0.325 n_q1=1635 n_q2=591 n_q3=1534 n_q4=1118 worst_quadrant_to_overall_ratio=1.327
The image catalog is written to wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits -region wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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.tzYcqwcrpF (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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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=26, bad_region=146, passed=588
Got 588 stars (including 421 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat
util/solve_plate_with_UCAC5 got 588 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.8'
Seting catalog search parameters based on the expected field of view 939.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013053 (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 0.010442 (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 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 408 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 405 matched stars entering correct_measured_positions(), 340 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 405 matched stars entering correct_measured_positions(), 369 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 408 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 403 matched stars entering correct_measured_positions(), 371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 403 matched stars entering correct_measured_positions(), 371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 403 stars left (next iteration limit 445)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: the 403 catalog matches do not cover the frame (153/13/188/49 per quadrant, need 25 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits N_match=403 sigma_overall_arcsec=0.855 sigma_q1_arcsec=0.689 sigma_q2_arcsec=1.505 sigma_q3_arcsec=0.825 sigma_q4_arcsec=1.501 n_q1=153 n_q2=13 n_q3=188 n_q4=49 worst_quadrant_to_overall_ratio=1.761
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits -region wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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.cs77UA4DGq (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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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=23, bad_region=146, passed=614
Got 614 stars (including 448 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat
util/solve_plate_with_UCAC5 got 614 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.7'
Seting catalog search parameters based on the expected field of view 939.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013051 (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 0.010441 (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 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 431 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 394 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
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 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 431 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 393 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 393 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 428 stars left (next iteration limit 470)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: the 428 catalog matches do not cover the frame (155/20/197/56 per quadrant, need 26 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits N_match=428 sigma_overall_arcsec=0.800 sigma_q1_arcsec=0.679 sigma_q2_arcsec=1.097 sigma_q3_arcsec=0.799 sigma_q4_arcsec=1.182 n_q1=155 n_q2=20 n_q3=197 n_q4=56 worst_quadrant_to_overall_ratio=1.478
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits -region wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits to local_wcs_cache/
'wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'local_wcs_cache/wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
Saving the final (post-refit) wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits to local_wcs_cache/
'wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits' -> 'local_wcs_cache/wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits'
Saving the final (post-refit) wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits to local_wcs_cache/
'wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits'
Saving the final (post-refit) wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits to local_wcs_cache/
'wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits sigma_overall=0.324 worst_q_ratio=1.313
ref2=Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits sigma_overall=0.396 worst_q_ratio=1.327
new1=fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits sigma_overall=0.855 worst_q_ratio=1.761
new2=fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits sigma_overall=0.800 worst_q_ratio=1.478
reference average sigma_overall=0.36 worst_q_ratio=1.32
warn-on-ratio threshold: 2.0x reference
###################################
WCS_QUALITY_RETRY: 1st new image (fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits) flagged: sigma=0.855 (ref avg 0.36), ratio=1.761 (ref avg 1.32), 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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/lib/make_outxyls_for_astrometric_calibration found 559 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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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: "out966257.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out966257.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).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
Field 1 did not solve (index index-4113.fits, field objects 1-10).
Field 1 did not solve (index index-4112.fits, field objects 1-10).
Field 1 did not solve (index index-4111.fits, field objects 1-10).
Field 1 did not solve (index index-4110.fits, field objects 1-10).
Field 1 did not solve (index index-4109.fits, field objects 1-10).
Field 1 did not solve (index index-4108.fits, field objects 1-10).
Field 1 did not solve (index index-4119.fits, field objects 11-20).
Field 1 did not solve (index index-4118.fits, field objects 11-20).
Field 1 did not solve (index index-4117.fits, field objects 11-20).
Field 1 did not solve (index index-4116.fits, field objects 11-20).
log-odds ratio 119.612 (8.85049e+51), 24 match, 0 conflict, 85 distractors, 53 index.
RA,Dec = (65.4533,38.0021), pixel scale 5.95427 arcsec/pix.
Hit/miss: Hit/miss: +---++++-++-------+---+-+----++-----+---++-----++-----+-----+--------------------++-----------------
Field 1: solved with index index-4115.fits.
Field 1 solved: writing to file ./out966257.solved to indicate this.
Field: out966257.xyls
Field center: (RA,Dec) = (65.453271, 38.000822) deg.
Field center: (RA H:M:S, Dec D:M:S) = (04:21:48.785, +38:00:02.960).
Field size: 15.7585 x 10.5397 degrees
Field rotation angle: up is -1.37496 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits' -> 'fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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 6 00:59 fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
-rw-r--r-- 1 apache apache 12K Sep 6 00:59 out966257.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits for reading... done!
Creating new image file (wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits (fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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: "out966257.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out966257.axy"...
Only searching for solutions within 15.6917 degrees of RA,Dec (65.4543,38.0017)
Field 1 did not solve (index index-4116.fits, field objects 1-100).
log-odds ratio 119.612 (8.85049e+51), 24 match, 0 conflict, 85 distractors, 53 index.
RA,Dec = (65.4533,38.0021), pixel scale 5.95427 arcsec/pix.
Hit/miss: Hit/miss: +---++++-++-------+---+-+----++-----+---++-----++-----+-----+--------------------++-----------------
Field 1: solved with index index-4115.fits.
Field 1 solved: writing to file ./out966257.solved to indicate this.
Field: out966257.xyls
Field center: (RA,Dec) = (65.453271, 38.000822) deg.
Field center: (RA H:M:S, Dec D:M:S) = (04:21:48.785, +38:00:02.960).
Field size: 15.7585 x 10.5397 degrees
Field rotation angle: up is -1.37496 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 6 00:59 fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
-rw-r--r-- 1 apache apache 12K Sep 6 00:59 out966257.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits for reading... done!
Creating new image file (wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
verification OK: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
Generating wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat from image00003.cat
Catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits created.
verification OK: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
verification OK: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
Image size: 941.5'x625.0' 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: 04:21:49.031 +38:00:06.01 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 588 stars ###
'wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/correct_sextractor_wcs_catalog_usingxy2sky966654.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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=26, bad_region=146, passed=588
Got 588 stars (including 421 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat
util/solve_plate_with_UCAC5 got 588 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 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 408 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 404 matched stars entering correct_measured_positions(), 344 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.15"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 404 matched stars entering correct_measured_positions(), 373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.18"
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 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 408 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 405 matched stars entering correct_measured_positions(), 371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.18"
Accuracy estimation diagnostic: 405 matched stars entering correct_measured_positions(), 371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.14"
Excluding outliers - 405 stars left (next iteration limit 444)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: the 405 catalog matches do not cover the frame (153/13/189/50 per quadrant, need 25 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits N_match=405 sigma_overall_arcsec=2.065 sigma_q1_arcsec=1.325 sigma_q2_arcsec=12.339 sigma_q3_arcsec=1.451 sigma_q4_arcsec=3.480 n_q1=153 n_q2=13 n_q3=189 n_q4=50 worst_quadrant_to_overall_ratio=5.975
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits -region wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits): sigma 0.855->2.065, ratio 1.761->5.975; reverting to order 3
WCS_QUALITY_RETRY: 2nd new image (fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits) flagged: sigma=0.800 (ref avg 0.36), ratio=1.478 (ref avg 1.32), 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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/lib/make_outxyls_for_astrometric_calibration found 588 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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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: "out966895.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out966895.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).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
Field 1 did not solve (index index-4113.fits, field objects 1-10).
Field 1 did not solve (index index-4112.fits, field objects 1-10).
Field 1 did not solve (index index-4111.fits, field objects 1-10).
Field 1 did not solve (index index-4110.fits, field objects 1-10).
Field 1 did not solve (index index-4109.fits, field objects 1-10).
Field 1 did not solve (index index-4108.fits, field objects 1-10).
Field 1 did not solve (index index-4119.fits, field objects 11-20).
Field 1 did not solve (index index-4118.fits, field objects 11-20).
Field 1 did not solve (index index-4117.fits, field objects 11-20).
Field 1 did not solve (index index-4116.fits, field objects 11-20).
log-odds ratio 121.442 (5.51537e+52), 25 match, 0 conflict, 95 distractors, 52 index.
RA,Dec = (65.4504,38.002), pixel scale 5.9541 arcsec/pix.
Hit/miss: Hit/miss: +---++++-++-------+---+++---+-+----+------+-----+----------------+----+-------+--+--+-----+---------
Field 1: solved with index index-4115.fits.
Field 1 solved: writing to file ./out966895.solved to indicate this.
Field: out966895.xyls
Field center: (RA,Dec) = (65.450842, 38.000702) deg.
Field center: (RA H:M:S, Dec D:M:S) = (04:21:48.202, +38:00:02.527).
Field size: 15.7583 x 10.5393 degrees
Field rotation angle: up is -1.37379 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits' -> 'fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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 6 00:59 fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
-rw-r--r-- 1 apache apache 12K Sep 6 00:59 out966895.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits for reading... done!
Creating new image file (wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits (fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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: "out966895.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out966895.axy"...
Only searching for solutions within 15.6917 degrees of RA,Dec (65.4519,38.0015)
Field 1 did not solve (index index-4116.fits, field objects 1-100).
log-odds ratio 121.442 (5.51537e+52), 25 match, 0 conflict, 95 distractors, 52 index.
RA,Dec = (65.4504,38.002), pixel scale 5.9541 arcsec/pix.
Hit/miss: Hit/miss: +---++++-++-------+---+++---+-+----+------+-----+----------------+----+-------+--+--+-----+---------
Field 1: solved with index index-4115.fits.
Field 1 solved: writing to file ./out966895.solved to indicate this.
Field: out966895.xyls
Field center: (RA,Dec) = (65.450842, 38.000702) deg.
Field center: (RA H:M:S, Dec D:M:S) = (04:21:48.202, +38:00:02.527).
Field size: 15.7583 x 10.5393 degrees
Field rotation angle: up is -1.37379 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 6 00:59 fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
-rw-r--r-- 1 apache apache 12K Sep 6 00:59 out966895.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits for reading... done!
Creating new image file (wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
verification OK: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
Generating wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat from image00004.cat
Catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits created.
verification OK: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
verification OK: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
Image size: 941.5'x625.0' 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: 04:21:48.448 +38:00:05.57 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 614 stars ###
'wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/correct_sextractor_wcs_catalog_usingxy2sky967303.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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=23, bad_region=146, passed=614
Got 614 stars (including 448 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat
util/solve_plate_with_UCAC5 got 614 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 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 432 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 362 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.18"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 393 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.21"
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 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 432 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 429 matched stars entering correct_measured_positions(), 395 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.24"
Accuracy estimation diagnostic: 429 matched stars entering correct_measured_positions(), 395 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.19"
Excluding outliers - 429 stars left (next iteration limit 470)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: the 429 catalog matches do not cover the frame (155/20/198/56 per quadrant, need 26 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits N_match=429 sigma_overall_arcsec=1.982 sigma_q1_arcsec=1.183 sigma_q2_arcsec=5.999 sigma_q3_arcsec=1.425 sigma_q4_arcsec=2.807 n_q1=155 n_q2=20 n_q3=198 n_q4=56 worst_quadrant_to_overall_ratio=3.027
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits -region wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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 2nd new image (fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits): sigma 0.800->1.982, ratio 1.478->3.027; reverting to order 3
WARNING: 1st new image has sigma_overall_arcsec=2.065 -- 5.74x the reference average (0.36); plate solution may be of low accuracy
WARNING: 2nd new image has sigma_overall_arcsec=1.982 -- 5.51x the reference average (0.36); plate solution may be of low accuracy
WARNING: 1st new image has worst_quadrant_to_overall_ratio=5.975 -- 4.53x the reference average (1.32); plate solution may be of low accuracy
WARNING: 2nd new image has worst_quadrant_to_overall_ratio=3.027 -- 2.29x the reference average (1.32); plate solution may be of low accuracy
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342_astrometric_residuals.png (4849 matched stars from wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025_astrometric_residuals.png (4878 matched stars from wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181_astrometric_residuals.png (403 matched stars from wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.68 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182_astrometric_residuals.png (428 matched stars from wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.71 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits'
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits'
Preparing the HTML report for the field Per-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Per-05-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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
SExtractor catalog cache: saved Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat to cache
SExtractor catalog cache: saved Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Creating symlink local_wcs_cache/wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Creating symlink local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
Creating symlink local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits exists and is non-empty
wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits exists and is non-empty
wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits exists and is non-empty
wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits (1st reference image)
verification OK: wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:21:49.059 +37:59:50.85 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-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits (1st new image)
verification OK: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
Image size: 939.8'x624.3' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:21:50.246 +38:00:07.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:21:49.059 +37:59:50.85
Second-epoch image center 04:21:50.246 +38:00:07.34
Angular distance between the image centers 0.0060 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits (2nd new image)
verification OK: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
Image size: 939.7'x624.3' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:21:49.565 +38:00:07.00 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:21:49.059 +37:59:50.85
Second-epoch image center 04:21:49.565 +38:00:07.00
Angular distance between the image centers 0.0048 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 04:21:50.246 +38:00:07.34
Second-epoch second image center 04:21:49.565 +38:00:07.00
Angular distance between the image centers 0.00224 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits &> /tmp/tmp.kCpPEOrXOk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits &> /tmp/tmp.TnFqwp5iOh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits &> /tmp/tmp.r9nDrKJHBK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits &> /tmp/tmp.8DxjuWQyQl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
Found non-empty wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
The reference image (wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits) and catalog (wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat) found
'wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat' -> 'wcsmag.cat'
Read 137281 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.9471 to 76.3491 deg, Dec +32.1657 to +43.3179 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 54.9471 to 76.3491 deg, Dec 32.1657 to 43.3179 deg
Loaded 9244 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): 5249 out of 7194 total matches.
Matched with Tycho-2 7194 out of 137281 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.846000
a=0.000000 b=1.000000 c=22.846000
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.57
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 137281 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.9471 to 76.3491 deg, Dec +32.1657 to +43.3179 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 54.9471 to 76.3491 deg, Dec 32.1657 to 43.3179 deg
Loaded 9244 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): 5249 out of 7194 total matches.
Matched with Tycho-2 7194 out of 137281 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Forced-photometry filter: calibrated wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits -> calib.txt_param_ref_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits (aperture=4.6)
Read 140690 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.4527 to 75.8199 deg, Dec +31.9743 to +43.3811 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 54.4527 to 75.8199 deg, Dec 31.9743 to 43.3811 deg
Loaded 9291 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): 5356 out of 7280 total matches.
Matched with Tycho-2 7280 out of 140690 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Forced-photometry filter: calibrated wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits -> calib.txt_param_ref_wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits (aperture=4.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 118 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
1.9 pix Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
2.1 pix fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
2.2 pix fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
Limiting magnitude estimates:
15.6 mag. Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
15.6 mag. Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
11.6 mag. fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
11.5 mag. fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
All-image limiting magnitude estimate: 11.5 (SNR ) 11.5 (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.kCpPEOrXOk (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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS-calibrated image found: wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Checking if the catalog wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat corresponding to the image wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat corresponding to the image wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS catalog name: wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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=23, blended=15371, bad_region=23033, passed=137258
Got 137258 stars (including 100558 good ones) from the SExtractor catalog wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
util/solve_plate_with_UCAC5 got 137258 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 4849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 118801 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 118801 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 118801 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4849 stars left (next iteration limit 5333)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits N_match=4849 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.402 sigma_q2_arcsec=0.289 sigma_q3_arcsec=0.267 sigma_q4_arcsec=0.245 n_q1=1954 n_q2=830 n_q3=1050 n_q4=1015 worst_quadrant_to_overall_ratio=1.283
The image catalog is written to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits -region wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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.TnFqwp5iOh (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-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits' -> 'wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WCS-calibrated image found: wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Checking if the catalog wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat corresponding to the image wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat corresponding to the image wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WCS catalog name: wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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=32, blended=14565, bad_region=33452, passed=140658
Got 140658 stars (including 96569 good ones) from the SExtractor catalog wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat
util/solve_plate_with_UCAC5 got 140658 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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 4878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 113868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 113868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 113868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4878 stars left (next iteration limit 5365)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits N_match=4878 sigma_overall_arcsec=0.371 sigma_q1_arcsec=0.480 sigma_q2_arcsec=0.369 sigma_q3_arcsec=0.338 sigma_q4_arcsec=0.314 n_q1=1625 n_q2=605 n_q3=1577 n_q4=1071 worst_quadrant_to_overall_ratio=1.296
The image catalog is written to wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits -region wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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.r9nDrKJHBK (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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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=139, bad_region=1054, passed=6550
Got 6550 stars (including 5395 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat
util/solve_plate_with_UCAC5 got 6550 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.8'
Seting catalog search parameters based on the expected field of view 939.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013053 (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 0.010442 (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 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 4859 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 4822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 5593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
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 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 4860 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 5593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 5593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
Excluding outliers - 4825 stars left (next iteration limit 5307)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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: the 4825 catalog matches do not cover the frame (1996/178/1866/785 per quadrant, need 301 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits N_match=4825 sigma_overall_arcsec=0.987 sigma_q1_arcsec=0.917 sigma_q2_arcsec=1.024 sigma_q3_arcsec=1.100 sigma_q4_arcsec=0.969 n_q1=1996 n_q2=178 n_q3=1866 n_q4=785 worst_quadrant_to_overall_ratio=1.114
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits -region wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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.8DxjuWQyQl (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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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=140, bad_region=1099, passed=6717
Got 6717 stars (including 5513 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat
util/solve_plate_with_UCAC5 got 6717 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.7'
Seting catalog search parameters based on the expected field of view 939.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013051 (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 0.010441 (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 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 4851 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 4816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 5731 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
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 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 4851 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 5731 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 5731 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
Excluding outliers - 4816 stars left (next iteration limit 5298)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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: the 4816 catalog matches do not cover the frame (1981/186/1877/772 per quadrant, need 301 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits N_match=4816 sigma_overall_arcsec=0.978 sigma_q1_arcsec=0.900 sigma_q2_arcsec=0.958 sigma_q3_arcsec=1.095 sigma_q4_arcsec=0.929 n_q1=1981 n_q2=186 n_q3=1877 n_q4=772 worst_quadrant_to_overall_ratio=1.119
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits -region wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-00_20.00sec_-0.00C_LIGHT_0181.fits
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.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-05-Q2b1x1_005512_TTUQ2b1x1_895235_v3NsQysQ/wcs_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182.fits
Preparing the HTML report for the field Per-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:10.10 +41:17:31.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:30.90 +41:33:50.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:49:18.23 +40:20:35.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:55:00.26 +33:27:26.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:40.01 +40:10:23.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:24.04 +40:43:31.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:45.93 +41:02:45.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:59.60 +40:20:33.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:45:51.77 +40:37:09.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:17.59 +40:42:17.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:10.10 +41:17:31.4: 11.89 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:49:18.23 +40:20:35.6: 11.87 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:40.01 +40:10:23.0: 11.99 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:45:51.77 +40:37:09.3: 11.69 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:45.93 +41:02:45.5: 11.64 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:55:00.26 +33:27:26.8: 11.96 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:30.90 +41:33:50.8: 11.75 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:59.60 +40:20:33.2: 12.01 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:24.04 +40:43:31.9: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Forced photometry filter REJECTED candidate at 03:49:18.23 +40:20:35.6: ref_mag=11.87 +/- 0.01 new_mean_mag=10.9922 delta=0.88 (need > 0.90)
Forced photometry filter KEPT candidate at 03:46:10.10 +41:17:31.4: ref_mag=11.89 +/- 0.01 new_mean_mag=10.9411 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 03:47:40.01 +40:10:23.0: ref_mag=11.99 +/- 0.01 new_mean_mag=11.0700 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Forced photometry filter KEPT candidate at 03:45:51.77 +40:37:09.3: ref_mag=11.69 +/- 0.01 new_mean_mag=10.7811 delta=0.91 (need > 0.90)
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Forced photometry filter KEPT candidate at 03:46:45.93 +41:02:45.5: ref_mag=11.64 +/- 0.01 new_mean_mag=10.6226 delta=1.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 03:55:00.26 +33:27:26.8: ref_mag=11.96 +/- 0.01 new_mean_mag=10.9510 delta=1.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:46:59.60 +40:20:33.2: ref_mag=12.01 +/- 0.01 new_mean_mag=11.1212 delta=0.89 (need > 0.90)
Forced photometry filter KEPT candidate at 03:46:30.90 +41:33:50.8: ref_mag=11.75 +/- 0.01 new_mean_mag=10.8362 delta=0.91 (need > 0.90)
Forced photometry filter KEPT candidate at 03:47:24.04 +40:43:31.9: ref_mag=12.13 +/- 0.01 new_mean_mag=11.0673 delta=1.06 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:17.59 +40:42:17.2: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry filter KEPT candidate at 03:47:17.59 +40:42:17.2: ref_mag=12.15 +/- 0.01 new_mean_mag=11.0879 delta=1.07 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:56:51.72 +33:47:54.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:59:07.50 +34:09:14.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:56:51.72 +33:47:54.7: 12.35 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:59:07.50 +34:09:14.2: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 03:56:51.72 +33:47:54.7: ref_mag=12.35 +/- 0.01 new_mean_mag=11.4214 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 03:59:07.50 +34:09:14.2: ref_mag=12.31 +/- 0.01 new_mean_mag=11.3713 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:59:23.55 +33:37:56.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:43.13 +39:25:17.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:56:57.39 +34:09:40.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:57:02.78 +34:12:08.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:55:23.60 +33:41:55.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:57:41.38 +34:44:16.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:57:11.49 +34:09:21.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:25.64 +41:25:22.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:55:18.30 +33:30:46.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:59:23.55 +33:37:56.6: 12.37 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:43.13 +39:25:17.0: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter KEPT candidate at 03:59:23.55 +33:37:56.6: ref_mag=12.37 +/- 0.01 new_mean_mag=11.3900 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:57:02.78 +34:12:08.7: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter KEPT candidate at 03:46:43.13 +39:25:17.0: ref_mag=12.43 +/- 0.01 new_mean_mag=11.3935 delta=1.04 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:56:57.39 +34:09:40.9: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter KEPT candidate at 03:57:02.78 +34:12:08.7: ref_mag=12.66 +/- 0.01 new_mean_mag=11.5661 delta=1.09 (need > 0.90)
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter KEPT candidate at 03:56:57.39 +34:09:40.9: ref_mag=12.44 +/- 0.01 new_mean_mag=11.3407 delta=1.10 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:55:23.60 +33:41:55.9: 12.75 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:57:41.38 +34:44:16.6: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Forced photometry filter KEPT candidate at 03:55:23.60 +33:41:55.9: ref_mag=12.75 +/- 0.02 new_mean_mag=11.5105 delta=1.24 (need > 0.90)
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Forced photometry filter KEPT candidate at 03:57:41.38 +34:44:16.6: ref_mag=12.83 +/- 0.02 new_mean_mag=11.6276 delta=1.20 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:25.64 +41:25:22.1: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Forced photometry filter KEPT candidate at 03:46:25.64 +41:25:22.1: ref_mag=12.70 +/- 0.02 new_mean_mag=11.4662 delta=1.24 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:57:11.49 +34:09:21.9: 12.86 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:55:18.30 +33:30:46.1: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Forced photometry filter KEPT candidate at 03:57:11.49 +34:09:21.9: ref_mag=12.86 +/- 0.02 new_mean_mag=11.6022 delta=1.26 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:56:39.27 +33:55:18.5: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Forced photometry filter KEPT candidate at 03:55:18.30 +33:30:46.1: ref_mag=12.78 +/- 0.02 new_mean_mag=11.6808 delta=1.10 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:56:39.27 +33:55:18.5: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Forced photometry filter KEPT candidate at 03:56:39.27 +33:55:18.5: ref_mag=12.68 +/- 0.02 new_mean_mag=11.5384 delta=1.14 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:56:49.70 +33:55:14.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:21.55 +40:11:29.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:55:25.68 +33:39:58.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:05.28 +40:08:12.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:45:21.59 +40:57:51.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:54:42.00 +33:46:27.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:45:21.63 +40:54:30.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:21.55 +40:11:29.8: 12.48 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:56:49.70 +33:55:14.1: 12.65 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:05.28 +40:08:12.7: 12.41 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:55:25.68 +33:39:58.6: 12.44 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:45:21.59 +40:57:51.3: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter KEPT candidate at 03:46:21.55 +40:11:29.8: ref_mag=12.48 +/- 0.01 new_mean_mag=11.2551 delta=1.22 (need > 0.90)
Forced photometry filter KEPT candidate at 03:56:49.70 +33:55:14.1: ref_mag=12.65 +/- 0.02 new_mean_mag=11.5794 delta=1.07 (need > 0.90)
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:54:42.00 +33:46:27.9: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter KEPT candidate at 03:46:05.28 +40:08:12.7: ref_mag=12.41 +/- 0.01 new_mean_mag=11.3291 delta=1.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter KEPT candidate at 03:55:25.68 +33:39:58.6: ref_mag=12.44 +/- 0.01 new_mean_mag=11.2995 delta=1.14 (need > 0.90)
Forced photometry filter KEPT candidate at 03:45:21.59 +40:57:51.3: ref_mag=12.47 +/- 0.01 new_mean_mag=11.3462 delta=1.12 (need > 0.90)
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter KEPT candidate at 03:54:42.00 +33:46:27.9: ref_mag=12.41 +/- 0.01 new_mean_mag=11.4697 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:55:03.98 +33:53:48.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:45:21.63 +40:54:30.8: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter KEPT candidate at 03:45:21.63 +40:54:30.8: ref_mag=12.39 +/- 0.01 new_mean_mag=11.3879 delta=1.00 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:55:03.98 +33:53:48.1: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter KEPT candidate at 03:55:03.98 +33:53:48.1: ref_mag=12.40 +/- 0.01 new_mean_mag=11.4241 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:47.71 +40:01:46.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:23.71 +40:48:46.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:55.94 +41:11:10.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:34.46 +40:00:38.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:57:17.20 +34:29:03.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:58.63 +40:32:52.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:45:35.21 +41:09:16.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:47.71 +40:01:46.3: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter KEPT candidate at 03:46:47.71 +40:01:46.3: ref_mag=12.39 +/- 0.01 new_mean_mag=11.3573 delta=1.03 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:34.46 +40:00:38.4: 12.31 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:55.94 +41:11:10.5: 12.31 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:57:17.20 +34:29:03.9: 12.32 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:23.71 +40:48:46.4: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter KEPT candidate at 03:46:55.94 +41:11:10.5: ref_mag=12.31 +/- 0.01 new_mean_mag=11.2673 delta=1.04 (need > 0.90)
Forced photometry filter KEPT candidate at 03:46:34.46 +40:00:38.4: ref_mag=12.31 +/- 0.01 new_mean_mag=11.3121 delta=0.99 (need > 0.90)
Forced photometry filter KEPT candidate at 03:57:17.20 +34:29:03.9: ref_mag=12.32 +/- 0.01 new_mean_mag=11.2976 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 03:47:23.71 +40:48:46.4: ref_mag=12.34 +/- 0.01 new_mean_mag=11.2890 delta=1.05 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:58.63 +40:32:52.3: 12.30 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:45:35.21 +41:09:16.3: 12.31 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:35.67 +39:54:12.5: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter KEPT candidate at 03:46:58.63 +40:32:52.3: ref_mag=12.30 +/- 0.01 new_mean_mag=11.1944 delta=1.11 (need > 0.90)
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 03:45:35.21 +41:09:16.3: ref_mag=12.31 +/- 0.01 new_mean_mag=11.2378 delta=1.07 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:35.67 +39:54:12.5: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Forced photometry filter KEPT candidate at 03:47:35.67 +39:54:12.5: ref_mag=12.27 +/- 0.01 new_mean_mag=11.2784 delta=1.00 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:40.26 +40:37:01.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:58:18.31 +34:40:02.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:56:15.99 +33:41:14.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:49:26.69 +40:29:14.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:40.26 +40:37:01.4: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:58:18.31 +34:40:02.9: 12.24 +/- 0.01 detection
Forced photometry filter KEPT candidate at 03:47:40.26 +40:37:01.4: ref_mag=12.26 +/- 0.01 new_mean_mag=11.2875 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:56:15.99 +33:41:14.8: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 03:58:18.31 +34:40:02.9: ref_mag=12.24 +/- 0.01 new_mean_mag=11.2910 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 03:56:15.99 +33:41:14.8: ref_mag=12.26 +/- 0.01 new_mean_mag=11.3619 delta=0.90 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:49:26.69 +40:29:14.2: 12.23 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:49:11.51 +40:09:57.7: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter KEPT candidate at 03:49:26.69 +40:29:14.2: ref_mag=12.23 +/- 0.01 new_mean_mag=11.2755 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:49:11.51 +40:09:57.7: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter KEPT candidate at 03:49:11.51 +40:09:57.7: ref_mag=12.20 +/- 0.01 new_mean_mag=11.2255 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:43.31 +40:16:52.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:45:59.43 +41:02:44.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:58:02.97 +34:10:35.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:43.31 +40:16:52.9: 12.20 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:58:02.97 +34:10:35.6: 12.15 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:45:59.43 +41:02:44.4: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter KEPT candidate at 03:46:43.31 +40:16:52.9: ref_mag=12.20 +/- 0.01 new_mean_mag=11.2187 delta=0.98 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:58:02.97 +34:10:35.6: ref_mag=12.15 +/- 0.01 new_mean_mag=11.2820 delta=0.86 (need > 0.90)
Forced photometry filter KEPT candidate at 03:45:59.43 +41:02:44.4: ref_mag=12.18 +/- 0.01 new_mean_mag=11.0703 delta=1.10 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:05.31 +40:50:49.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:05.31 +40:50:49.5: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 03:47:05.31 +40:50:49.5: ref_mag=12.13 +/- 0.01 new_mean_mag=11.0721 delta=1.06 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:50:19.13 +40:46:01.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:49:08.50 +40:09:38.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:50:19.13 +40:46:01.8: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 03:50:19.13 +40:46:01.8: ref_mag=12.13 +/- 0.01 new_mean_mag=11.2266 delta=0.90 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:49:08.50 +40:09:38.9: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry filter REJECTED candidate at 03:49:08.50 +40:09:38.9: ref_mag=12.10 +/- 0.01 new_mean_mag=11.2375 delta=0.86 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:38.31 +40:21:56.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:56:21.79 +33:52:29.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:06.06 +40:55:57.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:38.31 +40:21:56.9: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry filter KEPT candidate at 03:47:38.31 +40:21:56.9: ref_mag=12.08 +/- 0.01 new_mean_mag=11.0751 delta=1.01 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:06.06 +40:55:57.3: 12.07 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:56:21.79 +33:52:29.7: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry filter KEPT candidate at 03:47:06.06 +40:55:57.3: ref_mag=12.07 +/- 0.01 new_mean_mag=11.0024 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry filter KEPT candidate at 03:56:21.79 +33:52:29.7: ref_mag=12.06 +/- 0.01 new_mean_mag=11.1179 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:54:52.08 +33:36:03.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:54:52.08 +33:36:03.6: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry filter KEPT candidate at 03:54:52.08 +33:36:03.6: ref_mag=12.05 +/- 0.01 new_mean_mag=11.1356 delta=0.91 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:54:28.78 +33:32:04.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:54:28.78 +33:32:04.1: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry filter REJECTED candidate at 03:54:28.78 +33:32:04.1: ref_mag=12.05 +/- 0.01 new_mean_mag=11.1637 delta=0.89 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:57:06.30 +33:44:36.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:45:28.18 +40:17:19.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:57.42 +41:31:43.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:57:06.30 +33:44:36.4: 12.04 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:45:28.18 +40:17:19.2: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry filter KEPT candidate at 03:57:06.30 +33:44:36.4: ref_mag=12.04 +/- 0.01 new_mean_mag=11.0943 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry filter KEPT candidate at 03:45:28.18 +40:17:19.2: ref_mag=12.02 +/- 0.01 new_mean_mag=11.0969 delta=0.92 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:57.42 +41:31:43.1: 12.01 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:51.21 +41:01:55.3: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry filter KEPT candidate at 03:46:57.42 +41:31:43.1: ref_mag=12.01 +/- 0.01 new_mean_mag=11.0073 delta=1.00 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:51.21 +41:01:55.3: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry filter KEPT candidate at 03:46:51.21 +41:01:55.3: ref_mag=11.98 +/- 0.01 new_mean_mag=10.9999 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:57:10.83 +33:39:24.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:57:10.83 +33:39:24.0: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Forced photometry filter REJECTED candidate at 03:57:10.83 +33:39:24.0: ref_mag=11.97 +/- 0.01 new_mean_mag=11.0759 delta=0.90 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:45:41.87 +41:03:22.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:48:46.48 +41:05:35.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:49:18.57 +40:20:56.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:45:13.32 +41:27:03.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:45:41.87 +41:03:22.2: 11.96 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:48:46.48 +41:05:35.7: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Forced photometry filter REJECTED candidate at 03:45:41.87 +41:03:22.2: ref_mag=11.96 +/- 0.01 new_mean_mag=11.0758 delta=0.88 (need > 0.90)
Forced photometry filter KEPT candidate at 03:48:46.48 +41:05:35.7: ref_mag=11.94 +/- 0.01 new_mean_mag=11.0197 delta=0.92 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:49:18.57 +40:20:56.5: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Forced photometry filter REJECTED candidate at 03:49:18.57 +40:20:56.5: ref_mag=11.88 +/- 0.01 new_mean_mag=11.0879 delta=0.79 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:44.25 +41:34:03.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:45:13.32 +41:27:03.1: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Forced photometry filter REJECTED candidate at 03:45:13.32 +41:27:03.1: ref_mag=11.88 +/- 0.01 new_mean_mag=11.0045 delta=0.88 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:44.25 +41:34:03.8: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Forced photometry filter REJECTED candidate at 03:46:44.25 +41:34:03.8: ref_mag=11.84 +/- 0.01 new_mean_mag=10.9592 delta=0.88 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:56:13.55 +33:55:19.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:56.17 +39:31:06.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:56:35.20 +34:18:10.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:56:13.55 +33:55:19.7: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Forced photometry filter REJECTED candidate at 03:56:13.55 +33:55:19.7: ref_mag=11.79 +/- 0.01 new_mean_mag=10.9205 delta=0.87 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:56.17 +39:31:06.8: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Forced photometry filter REJECTED candidate at 03:46:56.17 +39:31:06.8: ref_mag=11.79 +/- 0.01 new_mean_mag=10.9306 delta=0.86 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:01.92 +40:26:13.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:56:35.20 +34:18:10.0: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Forced photometry filter REJECTED candidate at 03:56:35.20 +34:18:10.0: ref_mag=11.77 +/- 0.01 new_mean_mag=10.9024 delta=0.87 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:01.92 +40:26:13.5: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Forced photometry filter KEPT candidate at 03:47:01.92 +40:26:13.5: ref_mag=11.77 +/- 0.01 new_mean_mag=10.8567 delta=0.91 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:45:46.99 +41:04:19.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:14.45 +41:28:11.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:07.07 +40:08:26.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:31.81 +40:28:12.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:45:46.99 +41:04:19.0: 11.75 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:14.45 +41:28:11.3: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Forced photometry filter KEPT candidate at 03:45:46.99 +41:04:19.0: ref_mag=11.75 +/- 0.01 new_mean_mag=10.8133 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 11.68 +/- 0.01
Forced photometry filter KEPT candidate at 03:46:14.45 +41:28:11.3: ref_mag=11.68 +/- 0.01 new_mean_mag=10.7254 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:07.07 +40:08:26.0: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 0.01
Forced photometry filter KEPT candidate at 03:46:07.07 +40:08:26.0: ref_mag=11.65 +/- 0.01 new_mean_mag=10.7197 delta=0.93 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:31.81 +40:28:12.0: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Forced photometry filter REJECTED candidate at 03:46:31.81 +40:28:12.0: ref_mag=11.60 +/- 0.01 new_mean_mag=10.7654 delta=0.84 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:21.96 +41:31:04.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:21.96 +41:31:04.2: 11.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.01
Forced photometry filter REJECTED candidate at 03:46:21.96 +41:31:04.2: ref_mag=11.30 +/- 0.01 new_mean_mag=10.4182 delta=0.88 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:03:08.57 +35:54:48.7: 12.39 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:33:48.29 +41:05:11.2: 12.36 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:19:27.16 +39:14:05.6: 12.33 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:01:19.83 +34:21:27.8: 12.34 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:59:49.97 +33:56:26.8: 12.30 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:03:08.57 +35:54:48.7: 12.37 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:33:48.29 +41:05:11.2: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter KEPT candidate at 04:03:08.57 +35:54:48.7: ref_mag=12.38 +/- 0.01 new_mean_mag=11.4233 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 04:33:48.29 +41:05:11.2: ref_mag=12.34 +/- 0.01 new_mean_mag=11.0993 delta=1.25 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:19:27.16 +39:14:05.6: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 04:19:27.16 +39:14:05.6: ref_mag=12.31 +/- 0.01 new_mean_mag=11.2467 delta=1.07 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:01:19.83 +34:21:27.8: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 04:01:19.83 +34:21:27.8: ref_mag=12.32 +/- 0.01 new_mean_mag=11.3434 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:59:49.97 +33:56:26.8: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 03:59:49.97 +33:56:26.8: ref_mag=12.31 +/- 0.01 new_mean_mag=11.2421 delta=1.07 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:00:31.63 +34:05:38.5: 12.22 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:00:31.63 +34:05:38.5: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry filter KEPT candidate at 04:00:31.63 +34:05:38.5: ref_mag=12.21 +/- 0.01 new_mean_mag=11.2528 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:28.14 +40:59:21.3: 12.18 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:28.14 +40:59:21.3: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter KEPT candidate at 04:35:28.14 +40:59:21.3: ref_mag=12.18 +/- 0.01 new_mean_mag=10.8973 delta=1.28 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:19:33.88 +39:00:32.0: 12.11 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:34:19.63 +40:54:44.2: 12.03 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:02.40 +41:00:52.7: 11.94 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:19:33.88 +39:00:32.0: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry filter KEPT candidate at 04:19:33.88 +39:00:32.0: ref_mag=12.12 +/- 0.01 new_mean_mag=11.1406 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:34:19.63 +40:54:44.2: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry filter KEPT candidate at 04:34:19.63 +40:54:44.2: ref_mag=12.05 +/- 0.01 new_mean_mag=10.7627 delta=1.29 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:37:12.76 +41:06:14.3: 11.91 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:02.40 +41:00:52.7: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry filter KEPT candidate at 04:36:02.40 +41:00:52.7: ref_mag=11.93 +/- 0.01 new_mean_mag=10.5570 delta=1.38 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:37:12.76 +41:06:14.3: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.00
Forced photometry filter KEPT candidate at 04:37:12.76 +41:06:14.3: ref_mag=11.87 +/- 0.00 new_mean_mag=10.7796 delta=1.09 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:48.15 +41:12:39.8: 11.87 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:48.15 +41:12:39.8: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Forced photometry filter KEPT candidate at 04:36:48.15 +41:12:39.8: ref_mag=11.87 +/- 0.01 new_mean_mag=10.7376 delta=1.13 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:52.94 +41:13:06.8: 11.85 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:52.94 +41:13:06.8: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.00
Forced photometry filter KEPT candidate at 04:35:52.94 +41:13:06.8: ref_mag=11.84 +/- 0.00 new_mean_mag=10.8228 delta=1.02 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:02.98 +41:21:44.5: 11.83 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:02.98 +41:21:44.5: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.00
Forced photometry filter KEPT candidate at 04:36:02.98 +41:21:44.5: ref_mag=11.80 +/- 0.00 new_mean_mag=10.8294 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:45.30 +41:11:31.3: 11.79 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:12.69 +41:30:36.9: 11.74 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:05.16 +41:03:15.3: 11.66 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:03.80 +41:07:32.2: 11.65 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:45.30 +41:11:31.3: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Forced photometry filter KEPT candidate at 04:36:45.30 +41:11:31.3: ref_mag=11.79 +/- 0.01 new_mean_mag=10.8285 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:12.69 +41:30:36.9: 11.74 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:03.80 +41:07:32.2: 11.62 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:05.16 +41:03:15.3: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.74 +/- 0.00
Forced photometry filter KEPT candidate at 04:36:12.69 +41:30:36.9: ref_mag=11.74 +/- 0.00 new_mean_mag=10.7277 delta=1.01 (need > 0.90)
Forced photometry reference-image weighted average: 11.63 +/- 0.00
Forced photometry reference-image weighted average: 11.67 +/- 0.00
Forced photometry filter KEPT candidate at 04:35:03.80 +41:07:32.2: ref_mag=11.63 +/- 0.00 new_mean_mag=10.5828 delta=1.05 (need > 0.90)
Forced photometry filter KEPT candidate at 04:35:05.16 +41:03:15.3: ref_mag=11.67 +/- 0.00 new_mean_mag=10.6182 delta=1.05 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:47.16 +40:46:05.3: 11.59 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:42.29 +41:07:39.5: 11.50 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:47.16 +40:46:05.3: 11.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.00
Forced photometry filter KEPT candidate at 04:35:47.16 +40:46:05.3: ref_mag=11.55 +/- 0.00 new_mean_mag=10.3732 delta=1.18 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:42.29 +41:07:39.5: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.00
Forced photometry filter KEPT candidate at 04:36:42.29 +41:07:39.5: ref_mag=11.49 +/- 0.00 new_mean_mag=10.4403 delta=1.05 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:33:43.14 +40:56:37.4: 11.47 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:33:43.14 +40:56:37.4: 11.47 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.00
Forced photometry filter KEPT candidate at 04:33:43.14 +40:56:37.4: ref_mag=11.47 +/- 0.00 new_mean_mag=10.5046 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:48.66 +41:08:08.6: 11.43 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:44.51 +40:56:51.3: 11.23 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:48.66 +41:08:08.6: 11.39 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.00
Forced photometry filter KEPT candidate at 04:36:48.66 +41:08:08.6: ref_mag=11.41 +/- 0.00 new_mean_mag=10.2692 delta=1.14 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:44.51 +40:56:51.3: 11.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.00
Forced photometry filter KEPT candidate at 04:35:44.51 +40:56:51.3: ref_mag=11.24 +/- 0.00 new_mean_mag=10.2945 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:00.85 +40:51:44.0: 11.20 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:24.82 +40:52:45.6: 11.13 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:00.85 +40:51:44.0: 11.21 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.00
Forced photometry filter KEPT candidate at 04:36:00.85 +40:51:44.0: ref_mag=11.21 +/- 0.00 new_mean_mag=10.2619 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:24.82 +40:52:45.6: 11.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.00
Forced photometry filter KEPT candidate at 04:36:24.82 +40:52:45.6: ref_mag=11.12 +/- 0.00 new_mean_mag=10.1925 delta=0.93 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:36:18.03 +41:07:04.2: 11.12 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:36:18.03 +41:07:04.2: 11.12 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.00
Forced photometry filter KEPT candidate at 04:36:18.03 +41:07:04.2: ref_mag=11.12 +/- 0.00 new_mean_mag=10.1941 delta=0.93 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:17.17 +41:14:06.3: 11.10 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:17.17 +41:14:06.3: 11.10 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.10 +/- 0.00
Forced photometry filter KEPT candidate at 04:35:17.17 +41:14:06.3: ref_mag=11.10 +/- 0.00 new_mean_mag=10.1717 delta=0.93 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:34:40.03 +41:05:11.2: 10.99 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:34:40.03 +41:05:11.2: 10.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.99 +/- 0.00
Forced photometry filter KEPT candidate at 04:34:40.03 +41:05:11.2: ref_mag=10.99 +/- 0.00 new_mean_mag=10.0132 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:34:37.83 +40:56:44.2: 10.93 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q2b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:34:37.83 +40:56:44.2: 10.92 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.00
Forced photometry filter KEPT candidate at 04:34:37.83 +40:56:44.2: ref_mag=10.93 +/- 0.00 new_mean_mag=10.0182 delta=0.91 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out150074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out150792.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out151160.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out103317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70221.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 42s
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: 15s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184626_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 184626_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184628_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 184628_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184671_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 184671_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184677_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 184677_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184690_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 184690_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184705_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 184705_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184707_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 184707_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184711_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 184711_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184715_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 184715_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184730_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 184730_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184741_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 184741_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150074_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150074_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:45.93 +41:02:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.62, MAG_FAINT_SEARCH_LIMIT=11.60)GAIADR2_OUTPUT=# 0.800 225089379038083328 056.69117242158 +41.04581080627 11.3245 10.5604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150141_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150141_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:45:51.77 +40:37:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 0.291 225051652045446912 056.46577759762 +40.61918872849 11.5116 10.9440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150241_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150241_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:30.90 +41:33:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)GAIADR2_OUTPUT=# 0.993 231163149989600768 056.62901282070 +41.56391753149 11.6611 11.1695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150466_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150466_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150473_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150473_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:10.10 +41:17:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 0.497 225108586131393152 056.54221969871 +41.29196288302 11.5844 10.7748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150595_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150595_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:55:00.26 +33:27:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 0.502 218502617192120704 058.75094833366 +33.45752677724 11.6535 10.8844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150643_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150643_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:47:40.01 +40:10:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 0.969 224792747117984000 056.91685953217 +40.17329853743 11.8629 11.3251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150711_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150711_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150909_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150909_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:47:24.04 +40:43:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 0.082 224888237128485248 056.85015260200 +40.72554777524 11.7965 10.9178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150972_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150972_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:47:17.59 +40:42:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 2.087 224888168409016704 056.82258651723 +40.70500184896 11.7829 10.9139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151283_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151283_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:59:07.50 +34:09:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 0.547 218599232478302976 059.78141936967 +34.15388566512 11.7658 10.7854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151403_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151403_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:56:51.72 +33:47:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 0.706 218540275465188608 059.21539763919 +33.79835120960 11.7391 10.7114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151448_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151448_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:59:23.55 +33:37:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.502 218567625817199744 059.84801594070 +33.63249470821 12.1633 11.6107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151589_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151589_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:56:57.39 +34:09:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 1.110 218654968271912960 059.23895445743 +34.16163515620 12.0746 11.2477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151618_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151618_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:43.13 +39:25:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 1.057 224665890963274112 056.67946081545 +39.42161187544 12.0883 11.1989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152240_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 152240_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103744_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 103744_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152852_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 152852_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152802_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 152802_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:57:41.38 +34:44:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 1.332 218884044648234240 059.42207885139 +34.73818911907 12.4405 11.6134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152611_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 152611_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:55:18.30 +33:30:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 0.580 218509008103430016 058.82609366216 +33.51290008075 12.4118 11.5323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152464_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 152464_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:55:23.60 +33:41:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.608 218524504345372288 058.84851442847 +33.69878507684 12.3852 11.5825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152335_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 152335_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:25.64 +41:25:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 0.562 231161328923509504 056.60697181421 +41.42268911781 12.3403 11.4885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152222_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 152222_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:56:39.27 +33:55:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 1.057 218545184610247168 059.16390535736 +33.92162628270 12.3231 11.5340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152165_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 152165_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:56:49.70 +33:55:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.58, MAG_FAINT_SEARCH_LIMIT=12.56)GAIADR2_OUTPUT=# 1.064 218545876102500096 059.20706419875 +33.92087841726 12.2611 11.4551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151706_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151706_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:21.55 +40:11:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 0.640 224836766240608512 056.58969873884 +40.19144824633 12.0498 11.1375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151644_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151644_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:55:25.68 +33:39:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 1.078 218524126388260096 058.85667209604 +33.66640112186 12.1784 11.4315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151636_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151636_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:45:21.59 +40:57:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 0.440 225096624643269888 056.34011964854 +40.96424036289 12.0649 11.2294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151620_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151620_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:05.28 +40:08:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 2.438 224836177826437120 056.52111423167 +40.13684608736 12.2915 11.6367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151532_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151532_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:54:42.00 +33:46:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 1.635 218529245989051136 058.67508879470 +33.77396843883 12.1161 11.3786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151506_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151506_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:45:21.63 +40:54:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 0.598 225069995846040832 056.34000062883 +40.90869250632 12.2490 11.6576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151505_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151505_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:55:03.98 +33:53:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 0.556 218553671465625472 058.76674763879 +33.89662212936 11.9996 11.1377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151405_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 151405_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151369_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 151369_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151321_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 151321_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151316_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151316_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:57:17.20 +34:29:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.248 218668643447474560 059.32131493465 +34.48460682737 12.1946 11.6738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151277_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151277_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:34.46 +40:00:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 0.869 224831543560435456 056.64388079261 +40.01074623867 12.0094 11.1796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151262_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151262_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:58.63 +40:32:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 0.285 224882464692502144 056.74438033639 +40.54781963163 11.7908 10.8421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151258_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151258_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:45:35.21 +41:09:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 0.981 225100541653425280 056.39703574366 +41.15441150148 12.2241 11.6688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151195_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151195_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:47:35.67 +39:54:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 1.415 224785329712583936 056.89890762229 +39.90380022436 11.8824 11.0078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151160_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151160_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:47:40.26 +40:37:01.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151131_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151131_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:58:18.31 +34:40:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 0.772 218696303036962048 059.57604410773 +34.66740516033 11.9955 11.3944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151123_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151123_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:56:15.99 +33:41:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 1.689 218533777176164480 059.06715287590 +33.68760949851 12.1245 11.7477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151113_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151113_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:49:26.69 +40:29:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 0.842 224826527038676480 057.36103593877 +40.48747151135 11.8735 11.0373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151059_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151059_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:49:11.51 +40:09:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 1.765 224801306990810752 057.29731895247 +40.16606760657 11.6608 10.6222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151046_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 151046_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:43.31 +40:16:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.25, MAG_FAINT_SEARCH_LIMIT=12.23)GAIADR2_OUTPUT=# 1.628 224843294590853632 056.67987036584 +40.28141875772 11.8507 10.9679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150990_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150990_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:45:59.43 +41:02:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 0.693 225095941747773056 056.49774857436 +41.04583504973 12.0347 11.4963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150942_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150942_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150908_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150908_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:47:05.31 +40:50:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 0.419 225083297364422400 056.77222223054 +40.84699320428 11.9393 11.2922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150900_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150900_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:50:19.13 +40:46:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 0.490 230840473387435392 057.57955465221 +40.76723735430 11.8651 11.1404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150876_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150876_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150836_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150836_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:47:38.31 +40:21:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 1.273 224864941225969280 056.90961581434 +40.36615905274 11.9116 11.3099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150810_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150810_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:47:06.06 +40:55:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 1.216 225084877912371712 056.77497334208 +40.93284854610 11.6832 10.7889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150792_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150792_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:56:21.79 +33:52:29.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150766_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150766_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:54:52.08 +33:36:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 0.348 218522236602437632 058.71709715678 +33.60094727633 11.8459 11.2726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150761_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150761_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150729_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150729_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:57:06.30 +33:44:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 0.541 218539485191214848 059.27635888376 +33.74332453602 11.3357 10.2863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150710_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150710_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:45:28.18 +40:17:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 0.055 224852017665820800 056.36740087229 +40.28865709295 11.9518 11.5291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150679_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150679_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:57.42 +41:31:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)GAIADR2_OUTPUT=# 0.585 231116661263584768 056.73924579367 +41.52880146199 11.5730 10.6629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150602_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150602_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:51.21 +41:01:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 1.319 225088554404363776 056.71380277047 +41.03185436605 11.7827 11.1991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150597_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150597_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150586_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150586_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150538_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150538_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:48:46.48 +41:05:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 0.528 230904726097497600 057.19349296008 +41.09318366598 11.2077 10.1073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150509_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150509_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150455_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150455_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150395_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150395_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150312_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150312_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150301_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150301_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150297_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150297_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150285_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150285_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:47:01.92 +40:26:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 0.690 224857519522479616 056.75777472458 +40.43716900244 11.2169 10.2186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150248_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150248_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:45:46.99 +41:04:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 0.958 225098862325532032 056.44543918000 +41.07195802099 11.3424 10.4476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150131_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150131_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:14.45 +41:28:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.73, MAG_FAINT_SEARCH_LIMIT=11.71)GAIADR2_OUTPUT=# 0.403 231162428435132032 056.56022887024 +41.46991650941 11.5607 11.1201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150099_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150099_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:46:07.07 +40:08:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 1.169 224836216484823552 056.52955777935 +40.14087133223 11.4897 10.9542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150033_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 150033_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149656_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 149656_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148562_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 148562_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:58:57.92 +35:47:28.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148561_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 148561_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 03:57:51.50 +40:00:35.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119964_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 119964_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38126_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 38126_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67406_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 67406_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103317_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 103317_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106459_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 106459_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121094_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 121094_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39428_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 39428_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70221_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 70221_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41002_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 41002_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38827_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 38827_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36938_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 36938_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35237_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 35237_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35264_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 35264_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32701_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 32701_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35528_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 35528_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29899_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 29899_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36758_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 36758_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38265_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 38265_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42719_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 42719_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36626_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 36626_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40493_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 40493_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36336_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 36336_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39873_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 39873_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41282_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 41282_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40610_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 40610_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36786_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 36786_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34999_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 34999_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37721_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 37721_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40045_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
Preparing report for the candidate 40045_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48342_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 48342_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 04:14:53.34 +40:28:59.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31473_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182
The candidate 31473_fd_Per-05-Q2b1x1_2026-09-06_00-54-38_20.00sec_-0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 04:36:41.22 +41:15:51.6 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 59s
Prepared the HTML report for the field Per-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:01:19.83 +34:21:27.8
03:59:49.97 +33:56:26.8
04:03:08.57 +35:54:48.7
04:00:31.63 +34:05:38.5
03:46:55.94 +41:11:10.5
03:47:23.71 +40:48:46.4
03:46:47.71 +40:01:46.3
03:57:02.78 +34:12:08.7
03:57:11.49 +34:09:21.9
04:36:12.69 +41:30:36.9
04:36:02.98 +41:21:44.5
04:35:17.17 +41:14:06.3
04:36:48.15 +41:12:39.8
04:35:52.94 +41:13:06.8
04:36:45.30 +41:11:31.3
04:36:48.66 +41:08:08.6
04:36:42.29 +41:07:39.5
04:35:03.80 +41:07:32.2
04:36:18.03 +41:07:04.2
04:37:12.76 +41:06:14.3
04:34:40.03 +41:05:11.2
04:33:48.29 +41:05:11.2
04:35:05.16 +41:03:15.3
04:36:02.40 +41:00:52.7
04:35:28.14 +40:59:21.3
04:35:44.51 +40:56:51.3
04:34:37.83 +40:56:44.2
04:33:43.14 +40:56:37.4
04:36:24.82 +40:52:45.6
04:34:19.63 +40:54:44.2
04:36:00.85 +40:51:44.0
04:35:47.16 +40:46:05.3
04:19:27.16 +39:14:05.6
04:19:33.88 +39:00:32.0
########### Completed Per-05-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 ####
03:57:02.78 +34:12:08.7
03:57:11.49 +34:09:21.9
03:46:47.71 +40:01:46.3
03:47:23.71 +40:48:46.4
03:46:55.94 +41:11:10.5
04:03:08.57 +35:54:48.7
04:33:48.29 +41:05:11.2
04:19:27.16 +39:14:05.6
04:01:19.83 +34:21:27.8
03:59:49.97 +33:56:26.8
04:00:31.63 +34:05:38.5
04:35:28.14 +40:59:21.3
04:19:33.88 +39:00:32.0
04:34:19.63 +40:54:44.2
04:36:02.40 +41:00:52.7
04:37:12.76 +41:06:14.3
04:36:48.15 +41:12:39.8
04:35:52.94 +41:13:06.8
04:36:02.98 +41:21:44.5
04:36:45.30 +41:11:31.3
04:36:12.69 +41:30:36.9
04:35:03.80 +41:07:32.2
04:35:05.16 +41:03:15.3
04:35:47.16 +40:46:05.3
04:36:42.29 +41:07:39.5
04:33:43.14 +40:56:37.4
04:36:48.66 +41:08:08.6
04:35:44.51 +40:56:51.3
04:36:00.85 +40:51:44.0
04:36:24.82 +40:52:45.6
04:36:18.03 +41:07:04.2
04:35:17.17 +41:14:06.3
04:34:40.03 +41:05:11.2
04:34:37.83 +40:56:44.2
###################################################################################
03:57:02.78 +34:12:08.7 -- not an asteroid (will add it to exclusion list)
03:57:11.49 +34:09:21.9 -- not an asteroid (will add it to exclusion list)
03:46:47.71 +40:01:46.3 -- not an asteroid (will add it to exclusion list)
03:47:23.71 +40:48:46.4 -- not an asteroid (will add it to exclusion list)
03:46:55.94 +41:11:10.5 -- not an asteroid (will add it to exclusion list)
04:03:08.57 +35:54:48.7 -- asteroid (will NOT add it to exclusion list)
04:33:48.29 +41:05:11.2 -- not an asteroid (will add it to exclusion list)
04:19:27.16 +39:14:05.6 -- not an asteroid (will add it to exclusion list)
04:01:19.83 +34:21:27.8 -- not an asteroid (will add it to exclusion list)
03:59:49.97 +33:56:26.8 -- not an asteroid (will add it to exclusion list)
04:00:31.63 +34:05:38.5 -- not an asteroid (will add it to exclusion list)
04:35:28.14 +40:59:21.3 -- not an asteroid (will add it to exclusion list)
04:19:33.88 +39:00:32.0 -- not an asteroid (will add it to exclusion list)
04:34:19.63 +40:54:44.2 -- not an asteroid (will add it to exclusion list)
04:36:02.40 +41:00:52.7 -- not an asteroid (will add it to exclusion list)
04:37:12.76 +41:06:14.3 -- not an asteroid (will add it to exclusion list)
04:36:48.15 +41:12:39.8 -- not an asteroid (will add it to exclusion list)
04:35:52.94 +41:13:06.8 -- not an asteroid (will add it to exclusion list)
04:36:02.98 +41:21:44.5 -- not an asteroid (will add it to exclusion list)
04:36:45.30 +41:11:31.3 -- not an asteroid (will add it to exclusion list)
04:36:12.69 +41:30:36.9 -- not an asteroid (will add it to exclusion list)
04:35:03.80 +41:07:32.2 -- not an asteroid (will add it to exclusion list)
04:35:05.16 +41:03:15.3 -- not an asteroid (will add it to exclusion list)
04:35:47.16 +40:46:05.3 -- not an asteroid (will add it to exclusion list)
04:36:42.29 +41:07:39.5 -- not an asteroid (will add it to exclusion list)
04:33:43.14 +40:56:37.4 -- not an asteroid (will add it to exclusion list)
04:36:48.66 +41:08:08.6 -- not an asteroid (will add it to exclusion list)
04:35:44.51 +40:56:51.3 -- not an asteroid (will add it to exclusion list)
04:36:00.85 +40:51:44.0 -- not an asteroid (will add it to exclusion list)
04:36:24.82 +40:52:45.6 -- not an asteroid (will add it to exclusion list)
04:36:18.03 +41:07:04.2 -- not an asteroid (will add it to exclusion list)
04:35:17.17 +41:14:06.3 -- not an asteroid (will add it to exclusion list)
04:34:40.03 +41:05:11.2 -- not an asteroid (will add it to exclusion list)
04:34:37.83 +40:56:44.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:46:47.71 +40:01:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:55.94 +41:11:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:23.71 +40:48:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:02.78 +34:12:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:11.49 +34:09:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:59:49.97 +33:56:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:31.63 +34:05:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:01:19.83 +34:21:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:19:27.16 +39:14:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:19:33.88 +39:00:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:43.14 +40:56:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:48.29 +41:05:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:34:19.63 +40:54:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:34:37.83 +40:56:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:34:40.03 +41:05:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:03.80 +41:07:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:05.16 +41:03:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:17.17 +41:14:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:28.14 +40:59:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:44.51 +40:56:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:47.16 +40:46:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:52.94 +41:13:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:00.85 +40:51:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:02.40 +41:00:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:02.98 +41:21:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:12.69 +41:30:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:18.03 +41:07:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:24.82 +40:52:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:42.29 +41:07:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:45.30 +41:11:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:48.15 +41:12:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:48.66 +41:08:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:12.76 +41:06:14.3 -- 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)
03:46:47.71 +40:01:46.3 -- not a known variable star
03:46:55.94 +41:11:10.5 -- not a known variable star
03:47:23.71 +40:48:46.4 -- not a known variable star
03:57:02.78 +34:12:08.7 -- not a known variable star
03:57:11.49 +34:09:21.9 -- not a known variable star
03:59:49.97 +33:56:26.8 -- a known variable star
04:00:31.63 +34:05:38.5 -- a known variable star
04:01:19.83 +34:21:27.8 -- not a known variable star
04:19:27.16 +39:14:05.6 -- not a known variable star
04:19:33.88 +39:00:32.0 -- not a known variable star
04:33:43.14 +40:56:37.4 -- not a known variable star
04:33:48.29 +41:05:11.2 -- not a known variable star
04:34:19.63 +40:54:44.2 -- not a known variable star
04:34:37.83 +40:56:44.2 -- not a known variable star
04:34:40.03 +41:05:11.2 -- not a known variable star
04:35:03.80 +41:07:32.2 -- not a known variable star
04:35:05.16 +41:03:15.3 -- not a known variable star
04:35:17.17 +41:14:06.3 -- not a known variable star
04:35:28.14 +40:59:21.3 -- not a known variable star
04:35:44.51 +40:56:51.3 -- not a known variable star
04:35:47.16 +40:46:05.3 -- a known variable star
04:35:52.94 +41:13:06.8 -- not a known variable star
04:36:00.85 +40:51:44.0 -- not a known variable star
04:36:02.40 +41:00:52.7 -- not a known variable star
04:36:02.98 +41:21:44.5 -- a known variable star
04:36:12.69 +41:30:36.9 -- a known variable star
04:36:18.03 +41:07:04.2 -- not a known variable star
04:36:24.82 +40:52:45.6 -- not a known variable star
04:36:42.29 +41:07:39.5 -- not a known variable star
04:36:45.30 +41:11:31.3 -- not a known variable star
04:36:48.15 +41:12:39.8 -- not a known variable star
04:36:48.66 +41:08:08.6 -- not a known variable star
04:37:12.76 +41:06:14.3 -- not a known variable star
Found 28 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
33 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
Adding identified Gaia sources from exclusion_list_apass.txt
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
03:46:47.71 +40:01:46.3
03:46:55.94 +41:11:10.5
03:47:23.71 +40:48:46.4
03:57:02.78 +34:12:08.7
03:57:11.49 +34:09:21.9
03:59:49.97 +33:56:26.8
04:00:31.63 +34:05:38.5
04:01:19.83 +34:21:27.8
04:19:27.16 +39:14:05.6
04:19:33.88 +39:00:32.0
04:33:43.14 +40:56:37.4
04:33:48.29 +41:05:11.2
04:34:19.63 +40:54:44.2
04:34:37.83 +40:56:44.2
04:34:40.03 +41:05:11.2
04:35:03.80 +41:07:32.2
04:35:05.16 +41:03:15.3
04:35:17.17 +41:14:06.3
04:35:28.14 +40:59:21.3
04:35:44.51 +40:56:51.3
04:35:47.16 +40:46:05.3
04:35:52.94 +41:13:06.8
04:36:00.85 +40:51:44.0
04:36:02.40 +41:00:52.7
04:36:02.98 +41:21:44.5
04:36:12.69 +41:30:36.9
04:36:18.03 +41:07:04.2
04:36:24.82 +40:52:45.6
04:36:42.29 +41:07:39.5
04:36:45.30 +41:11:31.3
04:36:48.15 +41:12:39.8
04:36:48.66 +41:08:08.6
04:37:12.76 +41:06:14.3
03:46:45.93 +41:02:45.5
03:46:07.07 +40:08:26.0
03:46:14.45 +41:28:11.3
03:45:51.77 +40:37:09.3
03:46:30.90 +41:33:50.8
03:45:46.99 +41:04:19.0
03:47:01.92 +40:26:13.5
03:46:10.10 +41:17:31.4
03:48:46.48 +41:05:35.7
03:55:00.26 +33:27:26.8
03:46:51.21 +41:01:55.3
03:47:40.01 +40:10:23.0
03:46:57.42 +41:31:43.1
03:45:28.18 +40:17:19.2
03:57:06.30 +33:44:36.4
03:54:52.08 +33:36:03.6
03:47:06.06 +40:55:57.3
03:47:38.31 +40:21:56.9
03:50:19.13 +40:46:01.8
03:47:05.31 +40:50:49.5
03:47:24.04 +40:43:31.9
03:47:17.59 +40:42:17.2
03:45:59.43 +41:02:44.4
03:46:43.31 +40:16:52.9
03:49:11.51 +40:09:57.7
03:49:26.69 +40:29:14.2
03:56:15.99 +33:41:14.8
03:58:18.31 +34:40:02.9
03:47:35.67 +39:54:12.5
03:45:35.21 +41:09:16.3
03:46:58.63 +40:32:52.3
03:46:34.46 +40:00:38.4
03:59:07.50 +34:09:14.2
03:57:17.20 +34:29:03.9
03:56:51.72 +33:47:54.7
03:59:23.55 +33:37:56.6
03:55:03.98 +33:53:48.1
03:45:21.63 +40:54:30.8
03:54:42.00 +33:46:27.9
03:56:57.39 +34:09:40.9
03:46:43.13 +39:25:17.0
03:46:05.28 +40:08:12.7
03:45:21.59 +40:57:51.3
03:55:25.68 +33:39:58.6
03:46:21.55 +40:11:29.8
03:56:49.70 +33:55:14.1
03:56:39.27 +33:55:18.5
03:46:25.64 +41:25:22.1
03:55:23.60 +33:41:55.9
03:55:18.30 +33:30:46.1
03:57:41.38 +34:44:16.6
03:56:21.79 +33:52:29.7
03:47:40.26 +40:37:01.4
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461289.74594986 -observatory V36
11:32:13.33 +04:16:59.6 Mercury (-1.0mag)
13:33:23.46 -14:07:03.3 Venus (-4.7mag)
07:11:08.85 +23:02:48.3 Mars (1.2mag)
09:08:10.97 +17:01:12.2 Jupiter (-1.8mag)
00:51:58.37 +02:40:20.1 Saturn (0.5mag)
04:13:40.39 +21:01:57.1 Uranus (5.7mag)
00:13:50.74 -00:02:33.5 Neptune (7.7mag)
20:25:39.99 -23:39:22.4 Pluto (14.5mag)
06:42:20.44 +26:29:30.9 Moon (-9.7mag)
-rw-r--r-- 1 apache apache 362 Sep 6 00:59 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461289.74594986:
09:08:07.11 +17:01:32.5 Io (6.2mag)
09:08:21.61 +17:00:20.7 Europa (6.3mag)
09:08:27.89 +16:59:49.1 Ganymede (5.7mag)
09:07:44.51 +17:03:21.6 Callisto (6.9mag)
09:05:55.19 +17:17:15.8 Himalia (15.7mag)
09:08:09.07 +17:01:21.8 Thebe (16.6mag)
09:05:33.02 +17:11:18.0 Elara (17.7mag)
09:12:06.04 +16:29:06.0 Pasiphae (17.9mag)
09:09:20.58 +17:18:41.7 Carme (19.0mag)
00:51:59.63 +02:40:40.5 Titan (8.3mag)
00:51:54.89 +02:40:25.9 Rhea (9.6mag)
00:52:16.29 +02:42:55.5 Iapetus (11.0mag)
00:52:09.96 +02:39:40.7 Hyperion (14.3mag)
00:50:46.25 +02:30:10.2 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 6 00:59 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461289.74594986:
21:56:21.49 -00:04:48.0 JWST
14:48:35.94 +53:32:54.0 Chandra
05:05:46.83 +46:06:43.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 6 00:59 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461289.74594986 -observatory V36
03:39:47.14 +19:17:26.8 17.4mag P/1996 R2 (Lagerkvist)
18:02:33.21 -34:13:50.3 14.3mag P/2010 H2 (Vales)
07:18:40.28 -70:14:37.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:15:34.13 +33:40:23.3 17.7mag C/2017 K2 (PANSTARRS)
04:49:52.29 +45:19:10.4 15.7mag P/2021 N1 (ZTF)
04:49:52.29 +45:19:10.4 15.7mag P/2021 N1 (ZTF)
04:49:52.29 +45:19:10.4 15.7mag P/2021 N1 (ZTF)
04:49:52.29 +45:19:10.4 15.7mag P/2021 N1 (ZTF)
22:14:19.64 +28:47:50.0 17.4mag C/2022 E2 (ATLAS)
07:09:23.13 +25:59:54.9 16.9mag C/2022 N2 (PANSTARRS)
10:48:31.68 +27:15:51.1 17.1mag C/2022 QE78 (ATLAS)
09:48:00.03 +05:14:19.2 18.0mag C/2022 R6 (PANSTARRS)
15:29:49.91 -15:33:25.0 14.8mag C/2023 R1 (PANSTARRS)
08:37:27.90 +32:49:41.5 15.8mag C/2024 E1 (Wierzchos)
15:06:28.05 +15:20:06.9 17.9mag C/2024 G6 (ATLAS)
18:34:17.29 +43:12:48.7 13.7mag C/2024 J3 (ATLAS)
20:27:37.07 +49:21:18.9 17.4mag C/2024 R4 (PANSTARRS)
05:35:02.42 -13:00:46.0 15.1mag C/2024 T5 (ATLAS)
07:11:15.58 +18:45:10.2 17.8mag C/2025 J1 (Borisov)
11:16:17.66 +18:51:02.8 16.8mag C/2025 V2 (Rankin)
13:18:45.87 +00:12:02.9 16.8mag C/2025 Y1 (ATLAS)
16:38:41.66 +74:12:17.5 16.1mag C/2026 A2 (Bok)
03:06:17.54 +46:09:58.1 17.4mag C/2026 B2 (Sun-Gao)
12:12:18.00 +11:11:48.4 17.5mag A/2026 E1
22:25:08.20 -34:57:42.0 13.4mag 10P/Tempel
01:17:50.71 +36:48:41.9 18.0mag 11P/Tempel-Swift-LINEAR
11:47:28.12 -05:23:22.4 16.3mag 29P/Schwassmann-Wachmann
12:06:27.17 -04:45:42.2 17.6mag 63P/Wild
00:45:14.40 -07:00:08.4 15.4mag 65P/Gunn
06:37:17.28 +19:19:51.4 17.1mag 78P/Gehrels
03:17:11.81 +14:59:01.5 16.7mag 88P/Howell
05:34:44.64 +28:13:41.6 17.5mag 112P/Urata-Niijima
07:28:40.21 +25:04:54.7 17.9mag 114P/Wiseman-Skiff
10:25:32.55 +21:05:22.9 14.8mag 123P/West-Hartley
12:44:17.50 -20:58:16.7 17.4mag 124P/Mrkos
06:16:08.15 +20:40:15.9 15.9mag 128P/Shoemaker-Holt
02:36:05.86 -17:43:38.4 15.3mag 161P/Hartley-IRAS
09:39:40.43 +14:26:01.2 12.0mag 169P/NEAT
03:23:31.85 +08:33:33.1 14.5mag 220P/McNaught
04:45:13.44 +35:59:18.7 15.2mag 260P/McNaught
08:29:02.77 +35:48:39.1 17.3mag 295P/LINEAR
15:24:33.60 -00:07:51.2 17.9mag 391P/Kowalski
09:26:52.55 +16:54:15.0 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.1K Sep 6 00:59 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 6 00:59 asassn_transients_list.txt
############################################################
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 6 00:59 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:48:01.050 +02:29:57.95 AT 2026ymz 2026-08-05.73 21.98
22:56:40.110 +02:46:51.37 AT 2026ymy 2026-08-04.80 21.96
01:44:34.660 +05:27:13.55 AT 2026ymx 2026-08-01.88 21.27
01:29:50.630 +00:07:42.35 AT 2026ymw 2026-07-21.86 22.34
01:20:55.160 +01:31:29.58 AT 2026ymv 2026-07-20.88 22.17
23:25:01.600 +02:19:39.37 AT 2026ymu 2026-07-20.78 22.49
22:52:58.240 +03:42:25.38 AT 2026ymt 2026-08-05.73 21.81
23:42:43.162 +19:31:30.19 AT 2026yms 2026-08-09.94 19.57
21:20:13.290 -37:42:51.98 AT 2026ymr 2026-08-09.45 19.171
17:37:51.010 -21:58:53.20 AT 2026ymq 2026-08-09.59 14.86
22:57:17.960 +47:07:41.80 AT 2026ymp 2026-08-09.33 14.3
21:11:14.725 +16:08:57.69 AT 2026ymo 2026-08-04.97 19.97
00:45:33.395 +25:23:53.86 AT 2026ymn 2026-08-10.09 19.737
16:42:12.700 +21:20:23.08 AT 2026ymm 2026-08-09.32 19.568
00:16:26.794 -31:27:04.55 AT 2026yml 2026-08-09.54 18.69
20:46:11.408 +21:33:49.40 SN 2026ymk 2026-08-10.01 19.906
16:27:21.310 +63:36:15.74 AT 2026ymj 2026-08-08.31 19.192
00:43:25.659 +22:56:56.07 SN 2026ymi 2026-08-10.10 19.196
00:25:21.922 +28:26:14.78 AT 2026ymh 2026-08-09.50 19.349
00:12:57.521 -28:42:47.48 AT 2026ymg 2026-08-09.53 18.729
-rw-r--r-- 1 apache apache 88K Sep 6 00:59 tns_transients_list.txt
