This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ
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 04.4665 2461287.9665 12.26 22:54:26.97 +06:34:55.3
78.62528 -45.98413 galactic Psc Second-epoch detections are separated by 2.3" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.713 Luscinia 0 -0 0 13.2 -0 -0
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 22:54:26.97 +06:34:55.3: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 22:54:26.97 +06:34:55.3: 15.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461287.9665,12.26,0.05,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 20260904.4665 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.64 23:24:53.32 +09:30:55.3
90.17177 -47.77527 galactic Peg Second-epoch detections are separated by 0.4" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:24:53.32 +09:30:55.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.399+/-0.036 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:24:53.32 +09:30:55.3: 13.65 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:24:53.32 +09:30:55.3: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.64,0.05,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 20260904.4665 12.64CV 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 04.4665 2461287.9665 12.63 23:27:00.34 +09:13:29.5
90.64396 -48.28257 galactic Peg Second-epoch detections are separated by 1.2" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:27:00.34 +09:13:29.5 (user input) | T | P | (position from user input) J-Ks=0.475+/-0.036 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:00.34 +09:13:29.5: 13.76 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:00.34 +09:13:29.5: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.71 23:31:52.32 +08:55:21.0
92.03221 -49.11639 galactic Peg Second-epoch detections are separated by 2.2" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:31:52.32 +08:55:21.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.410+/-0.033 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:31:52.32 +08:55:21.0: 13.88 +/- 0.07 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:31:52.32 +08:55:21.0: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.71,0.05,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 20260904.4665 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.73 23:27:05.38 +10:07:04.6
91.30756 -47.50793 galactic Peg Second-epoch detections are separated by 1.1" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:27:05.38 +10:07:04.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.310+/-0.033 (F)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:05.38 +10:07:04.6: 13.90 +/- 0.07 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:05.38 +10:07:04.6: 13.80 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.79 23:28:02.08 +09:47:44.6
91.38555 -47.90191 galactic Peg Second-epoch detections are separated by 1.4" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:02.08 +09:47:44.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.434+/-0.035 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:02.08 +09:47:44.6: 13.99 +/- 0.08 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:02.08 +09:47:44.6: 13.92 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.79,0.05,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
target 20260904.4665 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.23 23:28:21.83 +03:15:27.3
86.30601 -53.60073 galactic Psc Second-epoch detections are separated by 0.7" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J352.0909+03.2577 | 23:28:21.83 +03:15:27.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.388+/-0.033 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:21.83 +03:15:27.3: 13.17 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:21.83 +03:15:27.3: 13.16 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.0909+03.2577,2461287.9665,12.23,0.05,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 J352.0909+03.2577 20260904.4665 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.18 23:31:31.72 +09:27:46.2
92.29670 -48.59788 galactic Peg Second-epoch detections are separated by 0.8" and 9.3 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 J352.8822+09.4629 | 23:31:31.72 +09:27:46.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.545+/-0.032 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:31:31.72 +09:27:46.2: 13.16 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:31:31.72 +09:27:46.2: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.8822+09.4629,2461287.9665,12.18,0.05,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 J352.8822+09.4629 20260904.4665 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.35 23:25:15.90 +10:12:58.3
90.79447 -47.20718 galactic Peg Second-epoch detections are separated by 1.7" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:15.90 +10:12:58.3 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.035 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:25:15.90 +10:12:58.3: 13.30 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:25:15.90 +10:12:58.3: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.35,0.05,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
target 20260904.4665 12.35CV 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 04.4665 2461287.9665 12.70 23:32:48.37 +09:08:42.0
92.50098 -49.02479 galactic Peg Second-epoch detections are separated by 0.8" and 9.3 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 | 23:32:48.37 +09:08:42.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.391+/-0.035 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:32:48.37 +09:08:42.0: 13.58 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:32:48.37 +09:08:42.0: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.33 23:17:59.88 +08:32:51.1
87.26017 -47.74758 galactic Peg Second-epoch detections are separated by 1.2" and 9.3 pix
The object was found in VSX 1" NSVS 11845209
Type: RS
# Max. Min./Amp. JD0 Period
13.074 r Y 0.238 r 2458658.91210 0.794152800000
The object was not found in astcheck.
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:17:59.88 +08:32:51.1: 13.55 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:17:59.88 +08:32:51.1: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11845209,2461287.9665,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11845209 20260904.4665 12.33CV 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 04.4665 2461287.9665 12.50 23:29:15.15 +09:32:33.7
91.60355 -48.26645 galactic Peg Second-epoch detections are separated by 1.4" and 9.3 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 | 23:29:15.15 +09:32:33.7 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.516+/-0.030 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:29:15.15 +09:32:33.7: 13.52 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:29:15.15 +09:32:33.7: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.50,0.05,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 20260904.4665 12.50CV 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 04.4665 2461287.9665 12.56 23:24:11.45 +10:03:36.5
90.34275 -47.21581 galactic Peg Second-epoch detections are separated by 0.7" and 9.3 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 | 23:24:11.45 +10:03:36.5 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.349+/-0.035 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:24:11.45 +10:03:36.5: 13.53 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:24:11.45 +10:03:36.5: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.56,0.05,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 20260904.4665 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.45 23:24:53.97 +10:11:15.8
90.65831 -47.18879 galactic Peg Second-epoch detections are separated by 1.2" and 9.3 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 | 23:24:53.97 +10:11:15.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:24:53.97 +10:11:15.8: 13.48 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:24:53.97 +10:11:15.8: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.45,0.05,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
target 20260904.4665 12.45CV 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 04.4665 2461287.9665 12.55 23:28:32.42 +09:33:03.0
91.37680 -48.17662 galactic Peg Second-epoch detections are separated by 2.1" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:32.42 +09:33:03.0 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.043 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:32.42 +09:33:03.0: 13.41 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:32.42 +09:33:03.0: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.55,0.05,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
target 20260904.4665 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.49 23:28:04.73 +10:05:18.3
91.60507 -47.64887 galactic Peg Second-epoch detections are separated by 1.6" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5775 Inuyama 113 337 355 15.3 -0 0
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:04.73 +10:05:18.3: 13.34 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:04.73 +10:05:18.3: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461287.9665,12.49,0.05,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 20260904.4665 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.44 23:28:36.28 +09:33:28.1
91.40270 -48.17796 galactic Peg Second-epoch detections are separated by 1.3" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:36.28 +09:33:28.1 (user input) | T | P | (position from user input) J-Ks=0.578+/-0.031 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:36.28 +09:33:28.1: 13.41 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:36.28 +09:33:28.1: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.44,0.05,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
target 20260904.4665 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.43 23:31:49.90 +09:30:26.6
92.42799 -48.59258 galactic Peg Second-epoch detections are separated by 1.3" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:31:49.90 +09:30:26.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.297+/-0.037 (F)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:31:49.90 +09:30:26.6: 13.39 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:31:49.90 +09:30:26.6: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.43,0.05,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 20260904.4665 12.43CV 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 04.4665 2461287.9665 12.38 23:26:59.46 +10:10:53.6
91.32054 -47.44041 galactic Peg Second-epoch detections are separated by 1.9" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:26:59.46 +10:10:53.6 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.393+/-0.033 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:26:59.46 +10:10:53.6: 13.36 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:26:59.46 +10:10:53.6: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.38,0.05,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 20260904.4665 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.40 23:28:32.73 +09:59:46.7
91.69158 -47.78413 galactic Peg Second-epoch detections are separated by 0.6" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5775 Inuyama 526 5 526 15.3 -0 0
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:32.73 +09:59:46.7: 13.35 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:32.73 +09:59:46.7: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461287.9665,12.40,0.05,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
VARIABLE_NAME 20260904.4665 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.41 23:28:58.08 +09:49:27.2
91.70845 -47.98490 galactic Peg Second-epoch detections are separated by 0.7" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:58.08 +09:49:27.2 (user input) | T | P | (position from user input) J-Ks=0.651+/-0.033 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:58.08 +09:49:27.2: 13.30 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:58.08 +09:49:27.2: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.41,0.05,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 20260904.4665 12.41CV 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 04.4665 2461287.9665 12.45 23:21:05.62 +09:11:50.3
88.73061 -47.58535 galactic Peg Second-epoch detections are separated by 0.4" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:21:05.62 +09:11:50.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.389+/-0.034 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:21:05.62 +09:11:50.3: 13.31 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:21:05.62 +09:11:50.3: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.45,0.05,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
target 20260904.4665 12.45CV 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 04.4665 2461287.9665 12.31 23:36:10.16 +08:15:50.0
93.02950 -50.18660 galactic Peg Second-epoch detections are separated by 0.2" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:36:10.16 +08:15:50.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.385+/-0.033 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:36:10.16 +08:15:50.0: 13.33 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:36:10.16 +08:15:50.0: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.31,0.05,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 20260904.4665 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.29 23:32:18.18 +09:06:33.0
92.30762 -48.99978 galactic Peg Second-epoch detections are separated by 2.6" and 9.3 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 | 23:32:18.18 +09:06:33.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.388+/-0.034 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:32:18.18 +09:06:33.0: 13.31 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:32:18.18 +09:06:33.0: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.29,0.05,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
target 20260904.4665 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.35 23:27:08.28 +10:00:55.1
91.25094 -47.60393 galactic Peg Second-epoch detections are separated by 2.6" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:27:08.28 +10:00:55.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.399+/-0.033 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:08.28 +10:00:55.1: 13.26 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:08.28 +10:00:55.1: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.35,0.05,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
target 20260904.4665 12.35CV 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 04.4665 2461287.9665 12.24 23:26:22.73 +09:29:02.7
90.62814 -47.98092 galactic Peg Second-epoch detections are separated by 0.9" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:26:22.73 +09:29:02.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.442+/-0.033 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:26:22.73 +09:29:02.7: 13.25 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:26:22.73 +09:29:02.7: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.24,0.05,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 20260904.4665 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.22 23:29:32.40 +09:38:00.6
91.76142 -48.21940 galactic Peg Second-epoch detections are separated by 0.9" and 9.3 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 | 23:29:32.40 +09:38:00.6 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.035 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:29:32.40 +09:38:00.6: 13.24 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:29:32.40 +09:38:00.6: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.22,0.05,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
target 20260904.4665 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.21 23:25:44.03 +09:20:44.1
90.31989 -48.02509 galactic Peg Second-epoch detections are separated by 1.1" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:44.03 +09:20:44.1 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.044 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:25:44.03 +09:20:44.1: 13.19 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:25:44.03 +09:20:44.1: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.24 23:31:52.88 +09:01:03.1
92.10238 -49.03319 galactic Peg Second-epoch detections are separated by 0.3" and 9.3 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 | 23:31:52.88 +09:01:03.1 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.374+/-0.041 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:31:52.88 +09:01:03.1: 13.19 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:31:52.88 +09:01:03.1: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.24,0.05,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 20260904.4665 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.09 23:07:26.00 +03:48:37.9
79.87069 -50.15999 galactic Psc Second-epoch detections are separated by 0.9" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:07:26.00 +03:48:37.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.263+/-0.031 (F)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:07:26.00 +03:48:37.9: 13.12 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:07:26.00 +03:48:37.9: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.19 23:26:59.52 +09:37:32.6
90.92770 -47.92930 galactic Peg Second-epoch detections are separated by 2.0" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:26:59.52 +09:37:32.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.378+/-0.037 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:26:59.52 +09:37:32.6: 13.12 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:26:59.52 +09:37:32.6: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.19,0.05,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 20260904.4665 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.04 23:28:35.26 +03:05:08.5
86.23140 -53.77598 galactic Psc Second-epoch detections are separated by 0.9" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J352.1468+03.0856 | 23:28:35.26 +03:05:08.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.669+/-0.033 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:35.26 +03:05:08.5: 13.09 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:35.26 +03:05:08.5: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.1468+03.0856,2461287.9665,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.1468+03.0856 20260904.4665 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.14 23:27:08.67 +09:43:21.7
91.04603 -47.86206 galactic Peg Second-epoch detections are separated by 1.9" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:27:08.67 +09:43:21.7 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.267+/-0.031 (F)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:08.67 +09:43:21.7: 13.03 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:08.67 +09:43:21.7: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.14,0.05,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
target 20260904.4665 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.03 23:07:10.20 +03:55:52.4
79.90402 -50.02426 galactic Psc Second-epoch detections are separated by 0.9" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:07:10.20 +03:55:52.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.730+/-0.033 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:07:10.20 +03:55:52.4: 13.02 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:07:10.20 +03:55:52.4: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461287.9665,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.72 23:25:43.52 +09:41:17.1
90.56467 -47.72450 galactic Peg Second-epoch detections are separated by 3.9" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:43.52 +09:41:17.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.491+/-0.037 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:25:43.52 +09:41:17.1: 13.97 +/- 0.07 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:25:43.52 +09:41:17.1: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.79 23:29:55.02 +09:29:47.9
91.78890 -48.38382 galactic Peg Second-epoch detections are separated by 1.9" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:29:55.02 +09:29:47.9 (user input) | T | P | (position from user input) J-Ks=0.736+/-0.033 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:29:55.02 +09:29:47.9: 13.88 +/- 0.07 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:29:55.02 +09:29:47.9: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.79,0.05,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
target 20260904.4665 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.77 23:28:18.18 +09:32:40.0
91.29497 -48.15458 galactic Peg Second-epoch detections are separated by 1.6" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:18.18 +09:32:40.0 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.359+/-0.032 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:18.18 +09:32:40.0: 13.85 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:18.18 +09:32:40.0: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.77,0.05,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
target 20260904.4665 12.77CV 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 04.4665 2461287.9665 12.71 23:29:19.43 +09:37:18.3
91.68250 -48.20486 galactic Peg Second-epoch detections are separated by 0.7" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:29:19.43 +09:37:18.3 (user input) | T | P | (position from user input) SpType: A1 1993AJ....106..591R [RRW93] Pn23l2-53 J-Ks=0.135+/-0.039 (A)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:29:19.43 +09:37:18.3: 13.77 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:29:19.43 +09:37:18.3: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.71,0.05,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 20260904.4665 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.84 23:27:08.59 +09:19:08.1
90.75656 -48.21643 galactic Peg Second-epoch detections are separated by 1.2" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:27:08.59 +09:19:08.1 (user input) | T | P | (position from user input) J-Ks=0.472+/-0.033 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:08.59 +09:19:08.1: 13.77 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:08.59 +09:19:08.1: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.70 23:26:52.24 +09:22:15.0
90.70558 -48.13859 galactic Peg Second-epoch detections are separated by 1.8" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:26:52.24 +09:22:15.0 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.034 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:26:52.24 +09:22:15.0: 13.73 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:26:52.24 +09:22:15.0: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.61 23:29:50.69 +09:50:34.5
92.00720 -48.06906 galactic Peg Second-epoch detections are separated by 2.5" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:29:50.69 +09:50:34.5 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=12.454+/- (unrealisitic color!)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:29:50.69 +09:50:34.5: 13.69 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:29:50.69 +09:50:34.5: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.61,0.05,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 20260904.4665 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.68 23:26:16.64 +09:32:22.2
90.63530 -47.92031 galactic Peg Second-epoch detections are separated by 3.1" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:26:16.64 +09:32:22.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.403+/-0.035 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:26:16.64 +09:32:22.2: 13.67 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:26:16.64 +09:32:22.2: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.63 23:24:08.38 +10:10:06.3
90.40405 -47.11509 galactic Peg Second-epoch detections are separated by 1.3" and 9.3 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 | 23:24:08.38 +10:10:06.3 (user input) | T | P | (position from user input) J-Ks=0.591+/-0.031 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:24:08.38 +10:10:06.3: 13.68 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:24:08.38 +10:10:06.3: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.65 23:30:20.94 +09:31:43.8
91.95344 -48.40492 galactic Peg Second-epoch detections are separated by 1.7" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:30:20.94 +09:31:43.8 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.464+/-0.033 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:30:20.94 +09:31:43.8: 13.68 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:30:20.94 +09:31:43.8: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.61 23:27:34.52 +09:53:26.8
91.30406 -47.76463 galactic Peg Second-epoch detections are separated by 2.2" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5775 Inuyama -334 -374 501 15.3 -0 0
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:34.52 +09:53:26.8: 13.67 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:34.52 +09:53:26.8: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461287.9665,12.61,0.05,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 20260904.4665 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.58 23:28:07.30 +09:34:52.4
91.26208 -48.10102 galactic Peg Second-epoch detections are separated by 2.5" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:07.30 +09:34:52.4 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.589+/-0.032 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:07.30 +09:34:52.4: 13.59 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:07.30 +09:34:52.4: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.58,0.05,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
target 20260904.4665 12.58CV 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 04.4665 2461287.9665 12.75 23:30:29.01 +09:25:19.9
91.92301 -48.51476 galactic Peg Second-epoch detections are separated by 1.6" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:30:29.01 +09:25:19.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.769+/-0.030 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:30:29.01 +09:25:19.9: 13.59 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:30:29.01 +09:25:19.9: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4665 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.58 23:25:55.97 +10:07:53.4
90.94707 -47.36036 galactic Peg Second-epoch detections are separated by 1.4" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:55.97 +10:07:53.4 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.423+/-0.034 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:25:55.97 +10:07:53.4: 13.58 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:25:55.97 +10:07:53.4: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.58,0.05,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
target 20260904.4665 12.58CV 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 04.4665 2461287.9665 12.37 23:28:20.73 +09:41:52.4
91.41737 -48.02431 galactic Peg Second-epoch detections are separated by 1.9" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:20.73 +09:41:52.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.458+/-0.032 (G)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:20.73 +09:41:52.4: 13.56 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:20.73 +09:41:52.4: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.37,0.05,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 20260904.4665 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4665 2461287.9665 12.62 23:31:44.32 +09:30:06.3
92.39327 -48.58708 galactic Peg Second-epoch detections are separated by 2.5" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:31:44.32 +09:30:06.3 (user input) | T | P | (position from user input) J-Ks=0.549+/-0.036 (K)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:31:44.32 +09:30:06.3: 13.63 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:31:44.32 +09:30:06.3: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9665,12.62,0.05,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
target 20260904.4665 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461241.93892009 20.07.2026 10:31:52.696 /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
First image: 2461241.93892009 20.07.2026 10:31:52.696 /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
Last image: 2461287.96675279 04.09.2026 11:11:57.441 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
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: 2 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): 4793
Objects passed selection criteria: 4766
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 2910
Average stars matched: 2738 (94.0893 %)
Memory usage VmPeak: 232048 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 Fri Sep 4 06:14:46 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: 2461241.93892009 20.07.2026 10:31:52.696 /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
First image: 2461241.93892009 20.07.2026 10:31:52.696 /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
Last image: 2461287.96675279 04.09.2026 11:11:57.441 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 79
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 6 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): 28424
Objects passed selection criteria: 28320
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 17884.8
Average stars matched: 16976.5 (94.9217 %)
Memory usage VmPeak: 257248 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 Fri Sep 4 06:15:23 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/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
SExtractor catalog cache: saved Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.cat to cache
SExtractor catalog cache: saved Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.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/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.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: 2461287.96615403
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_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits exists and is non-empty
wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits exists and is non-empty
wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits exists and is non-empty
wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits (1st reference image)
verification OK: wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:35.062 +05:59:47.09 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits (1st new image)
verification OK: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:38.312 +05:58:25.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:08:35.062 +05:59:47.09
Second-epoch image center 23:08:38.312 +05:58:25.33
Angular distance between the image centers 0.0264 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits (2nd new image)
verification OK: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:40.987 +05:57:45.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:08:35.062 +05:59:47.09
Second-epoch image center 23:08:40.987 +05:57:45.08
Angular distance between the image centers 0.0419 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 23:08:38.312 +05:58:25.33
Second-epoch second image center 23:08:40.987 +05:57:45.08
Angular distance between the image centers 0.01574 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/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits &> /tmp/tmp.huEe560nDJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits &> /tmp/tmp.k4mFxzT8F7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits &> /tmp/tmp.IoqDb7uG8y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits &> /tmp/tmp.uexOwKaR6D
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.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_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits and wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.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_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits and wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat
Found non-empty wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits and wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat
The reference image (wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits) and catalog (wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat) found
'wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat' -> 'wcsmag.cat'
Read 6525 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.1860 to 355.0874 deg, Dec +0.7201 to +11.2564 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 339.1860 to 355.0874 deg, Dec 0.7201 to 11.2564 deg
Loaded 4852 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): 3987 out of 4082 total matches.
Matched with Tycho-2 4082 out of 6525 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.596200
a=0.000000 b=1.000000 c=22.596200
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.05
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.05
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6525 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.1860 to 355.0874 deg, Dec +0.7201 to +11.2564 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 339.1860 to 355.0874 deg, Dec 0.7201 to 11.2564 deg
Loaded 4852 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): 3987 out of 4082 total matches.
Matched with Tycho-2 4082 out of 6525 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
Forced-photometry filter: calibrated wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits -> calib.txt_param_ref_wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits (aperture=6.2)
Read 7302 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.1869 to 355.0869 deg, Dec +0.7207 to +11.2552 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 339.1869 to 355.0869 deg, Dec 0.7207 to 11.2552 deg
Loaded 4850 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): 4074 out of 4173 total matches.
Matched with Tycho-2 4173 out of 7302 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
Forced-photometry filter: calibrated wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits -> calib.txt_param_ref_wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits (aperture=6.0)
____ 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:
2.2 pix Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
2.2 pix Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
3.3 pix fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
3.1 pix fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
Limiting magnitude estimates:
15.0 mag. Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
15.2 mag. Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
12.7 mag. fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
12.4 mag. fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 10.3 (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.huEe560nDJ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits' -> 'wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.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/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
WCS_IMAGE_NAME=wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
WCS-calibrated image found: wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
Checking if the catalog wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat corresponding to the image wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits alredy exist and is non-empty...
Catalog wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat corresponding to the image wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
WCS catalog name: wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.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=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=357, bad_region=1627, passed=6523
Got 6523 stars (including 4612 good ones) from the SExtractor catalog wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat
util/solve_plate_with_UCAC5 got 6523 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4491 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4481 matched stars entering correct_measured_positions(), 4481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4481 matched stars entering correct_measured_positions(), 5224 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4491 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4481 matched stars entering correct_measured_positions(), 5224 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4481 matched stars entering correct_measured_positions(), 5224 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4481 stars left (next iteration limit 4929)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits N_match=4481 sigma_overall_arcsec=0.334 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.341 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.320 n_q1=1466 n_q2=894 n_q3=1343 n_q4=778 worst_quadrant_to_overall_ratio=1.029
The image catalog is written to wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits -region wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.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.k4mFxzT8F7 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits' -> 'wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.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/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
WCS_IMAGE_NAME=wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
WCS-calibrated image found: wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
Checking if the catalog wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat corresponding to the image wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits alredy exist and is non-empty...
Catalog wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat corresponding to the image wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
WCS catalog name: wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.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=378, bad_region=1797, passed=7302
Got 7302 stars (including 5189 good ones) from the SExtractor catalog wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat
util/solve_plate_with_UCAC5 got 7302 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 4862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 5868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 5868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 5869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4862 stars left (next iteration limit 5348)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits N_match=4862 sigma_overall_arcsec=0.321 sigma_q1_arcsec=0.297 sigma_q2_arcsec=0.328 sigma_q3_arcsec=0.318 sigma_q4_arcsec=0.331 n_q1=1586 n_q2=976 n_q3=1435 n_q4=865 worst_quadrant_to_overall_ratio=1.032
The image catalog is written to wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits -region wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.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.IoqDb7uG8y (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_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.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_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
WCS_IMAGE_NAME=wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
WCS-calibrated image found: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
Checking if the catalog wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat corresponding to the image wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat corresponding to the image wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
WCS catalog name: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.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=110, bad_region=489, passed=1132
Got 1132 stars (including 604 good ones) from the SExtractor catalog wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat
util/solve_plate_with_UCAC5 got 1132 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 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 453 to 508 (Dec 0.7 to 11.2)
Done reading UCAC5 zone files...
Matched 580 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 577 matched stars entering correct_measured_positions(), 535 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 577 matched stars entering correct_measured_positions(), 670 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 453 to 508 (Dec 0.7 to 11.2)
Done reading UCAC5 zone files...
Matched 580 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 577 matched stars entering correct_measured_positions(), 669 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 577 matched stars entering correct_measured_positions(), 669 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 577 stars left (next iteration limit 634)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=577 robust_rms=6.582 arcsec worst_quadrant_rms=9.935 arcsec
SIP_REFIT: SIP order 3 trial: matched=577 robust_rms=0.511 arcsec worst_quadrant_rms=0.571 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=577 robust_rms_before=0.977 arcsec robust_rms_before_corrected=0.565 arcsec robust_rms_after=0.511 arcsec worst_quadrant_rms_before=0.708 worst_quadrant_rms_after=0.571
verification OK: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
verification OK: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
Image size: 937.4'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:38.339 +05:58:24.80 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1132 stars ###
'wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/correct_sextractor_wcs_catalog_usingxy2sky780668.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 0.977 -> 0.511 arcsec)
WCS_QUALITY_DIAG: file=fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits N_match=577 sigma_overall_arcsec=0.495 sigma_q1_arcsec=0.434 sigma_q2_arcsec=0.608 sigma_q3_arcsec=0.539 sigma_q4_arcsec=0.502 n_q1=230 n_q2=158 n_q3=96 n_q4=93 worst_quadrant_to_overall_ratio=1.229
The image catalog is written to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits -region wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.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.uexOwKaR6D (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_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.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_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
WCS_IMAGE_NAME=wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
WCS-calibrated image found: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
Checking if the catalog wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat corresponding to the image wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat corresponding to the image wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
WCS catalog name: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.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=106, bad_region=443, passed=1104
Got 1104 stars (including 626 good ones) from the SExtractor catalog wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat
util/solve_plate_with_UCAC5 got 1104 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 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 453 to 508 (Dec 0.7 to 11.2)
Done reading UCAC5 zone files...
Matched 603 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 601 matched stars entering correct_measured_positions(), 559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 601 matched stars entering correct_measured_positions(), 665 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 453 to 508 (Dec 0.7 to 11.2)
Done reading UCAC5 zone files...
Matched 603 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 601 matched stars entering correct_measured_positions(), 668 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 601 matched stars entering correct_measured_positions(), 668 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 601 stars left (next iteration limit 661)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=601 robust_rms=6.582 arcsec worst_quadrant_rms=10.921 arcsec
SIP_REFIT: SIP order 3 trial: matched=601 robust_rms=0.504 arcsec worst_quadrant_rms=0.582 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=601 robust_rms_before=1.018 arcsec robust_rms_before_corrected=0.550 arcsec robust_rms_after=0.504 arcsec worst_quadrant_rms_before=0.732 worst_quadrant_rms_after=0.582
verification OK: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
verification OK: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
Image size: 937.4'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:41.022 +05:57:44.63 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1104 stars ###
'wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/correct_sextractor_wcs_catalog_usingxy2sky780007.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 1.018 -> 0.504 arcsec)
WCS_QUALITY_DIAG: file=fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits N_match=601 sigma_overall_arcsec=0.514 sigma_q1_arcsec=0.409 sigma_q2_arcsec=0.657 sigma_q3_arcsec=0.552 sigma_q4_arcsec=0.493 n_q1=245 n_q2=120 n_q3=165 n_q4=71 worst_quadrant_to_overall_ratio=1.277
The image catalog is written to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits -region wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.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_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits to local_wcs_cache/
'wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits' -> 'local_wcs_cache/wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits'
Saving the final (post-refit) wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits to local_wcs_cache/
'wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits' -> 'local_wcs_cache/wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits'
Saving the final (post-refit) wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits to local_wcs_cache/
'wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits' -> 'local_wcs_cache/wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits'
Saving the final (post-refit) wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits to local_wcs_cache/
'wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits' -> 'local_wcs_cache/wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits sigma_overall=0.334 worst_q_ratio=1.029
ref2=Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits sigma_overall=0.321 worst_q_ratio=1.032
new1=fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits sigma_overall=0.495 worst_q_ratio=1.229
new2=fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits sigma_overall=0.514 worst_q_ratio=1.277
reference average sigma_overall=0.3275 worst_q_ratio=1.0305
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494_astrometric_residuals.png (4481 matched stars from wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466_astrometric_residuals.png (4862 matched stars from wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740_astrometric_residuals.png (577 matched stars from wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741_astrometric_residuals.png (601 matched stars from wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits'
Saving fully-calibrated image wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits'
Preparing the HTML report for the field Psc-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Psc-07-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/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
SExtractor catalog cache: saved Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.cat to cache
SExtractor catalog cache: saved Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
Creating symlink local_wcs_cache/wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.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_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits exists and is non-empty
wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits exists and is non-empty
wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits exists and is non-empty
wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits (1st reference image)
verification OK: wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:35.062 +05:59:47.09 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits (1st new image)
verification OK: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
Image size: 937.4'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:38.339 +05:58:24.80 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:08:35.062 +05:59:47.09
Second-epoch image center 23:08:38.339 +05:58:24.80
Angular distance between the image centers 0.0266 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits (2nd new image)
verification OK: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
Image size: 937.4'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:41.022 +05:57:44.63 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:08:35.062 +05:59:47.09
Second-epoch image center 23:08:41.022 +05:57:44.63
Angular distance between the image centers 0.0420 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 23:08:38.339 +05:58:24.80
Second-epoch second image center 23:08:41.022 +05:57:44.63
Angular distance between the image centers 0.01575 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/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits &> /tmp/tmp.47rPQ5yqQY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits &> /tmp/tmp.DFkOuDO8vh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits &> /tmp/tmp.2Kv9ejN9BS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits &> /tmp/tmp.yonp4Wwjxs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.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_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits and wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.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_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits and wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat
Found non-empty wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits and wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat
The reference image (wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits) and catalog (wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat) found
'wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat' -> 'wcsmag.cat'
Read 38395 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.1738 to 355.0889 deg, Dec +0.7186 to +11.2626 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 339.1738 to 355.0889 deg, Dec 0.7186 to 11.2626 deg
Loaded 4857 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): 3909 out of 4249 total matches.
Matched with Tycho-2 4249 out of 38395 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.475500
a=0.000000 b=1.000000 c=22.475500
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.21
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 38395 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.1738 to 355.0889 deg, Dec +0.7186 to +11.2626 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 339.1738 to 355.0889 deg, Dec 0.7186 to 11.2626 deg
Loaded 4857 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): 3909 out of 4249 total matches.
Matched with Tycho-2 4249 out of 38395 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
Forced-photometry filter: calibrated wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits -> calib.txt_param_ref_wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits (aperture=4.8)
Read 39732 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.1750 to 355.0869 deg, Dec +0.7187 to +11.2591 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 339.1750 to 355.0869 deg, Dec 0.7187 to 11.2591 deg
Loaded 4854 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): 3927 out of 4255 total matches.
Matched with Tycho-2 4255 out of 39732 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
Forced-photometry filter: calibrated wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits -> calib.txt_param_ref_wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 55 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
2.1 pix Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
2.7 pix fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
2.6 pix fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
Limiting magnitude estimates:
15.2 mag. Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
15.3 mag. Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
13.0 mag. fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
12.9 mag. fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.47rPQ5yqQY (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits' -> 'wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.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/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
WCS_IMAGE_NAME=wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
WCS-calibrated image found: wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
Checking if the catalog wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat corresponding to the image wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits alredy exist and is non-empty...
Catalog wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat corresponding to the image wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits
WCS catalog name: wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.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=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1495, bad_region=8205, passed=38382
Got 38382 stars (including 29018 good ones) from the SExtractor catalog wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat
util/solve_plate_with_UCAC5 got 38382 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 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 453 to 508 (Dec 0.7 to 11.3)
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: 4861 matched stars entering correct_measured_positions(), 4861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 32185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 32185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 32185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4862 stars left (next iteration limit 5347)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.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_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits N_match=4862 sigma_overall_arcsec=0.333 sigma_q1_arcsec=0.312 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.336 sigma_q4_arcsec=0.310 n_q1=1574 n_q2=992 n_q3=1413 n_q4=883 worst_quadrant_to_overall_ratio=1.042
The image catalog is written to wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits -region wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.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.DFkOuDO8vh (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits' -> 'wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.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/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
WCS_IMAGE_NAME=wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
WCS-calibrated image found: wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
Checking if the catalog wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat corresponding to the image wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits alredy exist and is non-empty...
Catalog wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat corresponding to the image wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits
WCS catalog name: wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.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=8, blended=1603, bad_region=7717, passed=39724
Got 39724 stars (including 30783 good ones) from the SExtractor catalog wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat
util/solve_plate_with_UCAC5 got 39724 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 33924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 33924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 33924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4864 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.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_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits N_match=4864 sigma_overall_arcsec=0.315 sigma_q1_arcsec=0.289 sigma_q2_arcsec=0.319 sigma_q3_arcsec=0.318 sigma_q4_arcsec=0.325 n_q1=1595 n_q2=953 n_q3=1462 n_q4=854 worst_quadrant_to_overall_ratio=1.031
The image catalog is written to wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits -region wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.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.2Kv9ejN9BS (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_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.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_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
WCS_IMAGE_NAME=wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
WCS-calibrated image found: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
Checking if the catalog wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat corresponding to the image wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat corresponding to the image wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
WCS catalog name: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.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=1, blended=655, bad_region=2344, passed=7097
Got 7097 stars (including 4659 good ones) from the SExtractor catalog wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat
util/solve_plate_with_UCAC5 got 7097 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 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 453 to 508 (Dec 0.7 to 11.2)
Done reading UCAC5 zone files...
Matched 4472 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4453 matched stars entering correct_measured_positions(), 4453 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4453 matched stars entering correct_measured_positions(), 5294 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
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 453 to 508 (Dec 0.7 to 11.2)
Done reading UCAC5 zone files...
Matched 4472 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4453 matched stars entering correct_measured_positions(), 5294 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
Accuracy estimation diagnostic: 4453 matched stars entering correct_measured_positions(), 5294 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
Excluding outliers - 4453 stars left (next iteration limit 4898)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4453 robust_rms=5.834 arcsec worst_quadrant_rms=9.800 arcsec
SIP_REFIT: SIP order 3 trial: matched=4453 robust_rms=0.995 arcsec worst_quadrant_rms=1.129 arcsec
SIP_REFIT: SIP order 5 trial: matched=4453 robust_rms=0.978 arcsec worst_quadrant_rms=1.137 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4453 robust_rms_before=1.010 arcsec robust_rms_before_corrected=0.995 arcsec robust_rms_after=0.995 arcsec worst_quadrant_rms_before=1.124 worst_quadrant_rms_after=1.129
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.124 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits N_match=4453 sigma_overall_arcsec=0.909 sigma_q1_arcsec=0.828 sigma_q2_arcsec=1.011 sigma_q3_arcsec=0.830 sigma_q4_arcsec=1.040 n_q1=1861 n_q2=1049 n_q3=802 n_q4=741 worst_quadrant_to_overall_ratio=1.144
The image catalog is written to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits -region wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.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.yonp4Wwjxs (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_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.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_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
WCS_IMAGE_NAME=wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
WCS-calibrated image found: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
Checking if the catalog wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat corresponding to the image wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat corresponding to the image wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
WCS catalog name: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.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=728, bad_region=2211, passed=7231
Got 7231 stars (including 4838 good ones) from the SExtractor catalog wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat
util/solve_plate_with_UCAC5 got 7231 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 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 453 to 508 (Dec 0.7 to 11.2)
Done reading UCAC5 zone files...
Matched 4645 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4629 matched stars entering correct_measured_positions(), 4629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4629 matched stars entering correct_measured_positions(), 5472 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 453 to 508 (Dec 0.7 to 11.2)
Done reading UCAC5 zone files...
Matched 4645 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4628 matched stars entering correct_measured_positions(), 5472 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
Accuracy estimation diagnostic: 4628 matched stars entering correct_measured_positions(), 5472 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Excluding outliers - 4628 stars left (next iteration limit 5091)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4628 robust_rms=6.106 arcsec worst_quadrant_rms=15.957 arcsec
SIP_REFIT: SIP order 3 trial: matched=4628 robust_rms=0.955 arcsec worst_quadrant_rms=1.087 arcsec
SIP_REFIT: SIP order 5 trial: matched=4628 robust_rms=0.943 arcsec worst_quadrant_rms=1.089 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4628 robust_rms_before=0.965 arcsec robust_rms_before_corrected=0.940 arcsec robust_rms_after=0.955 arcsec worst_quadrant_rms_before=1.102 worst_quadrant_rms_after=1.087
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.102 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits N_match=4628 sigma_overall_arcsec=0.889 sigma_q1_arcsec=0.824 sigma_q2_arcsec=1.077 sigma_q3_arcsec=0.851 sigma_q4_arcsec=0.973 n_q1=1940 n_q2=751 n_q3=1341 n_q4=596 worst_quadrant_to_overall_ratio=1.211
The image catalog is written to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits -region wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.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_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.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_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-05_20.00sec_-0.00C_LIGHT_0740.fits
Saving fully-calibrated image wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.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_2026-09-04_CI_Psc-07-Q2b1x1_061240_TTUQ2b1x1_760782_8BrzcSTJ/wcs_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741.fits
Preparing the HTML report for the field Psc-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 22:54:26.97 +06:34:55.3: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:19:42.30 +07:58:56.1: 12.58 +/- 0.02 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:31:31.72 +09:27:46.2: 13.16 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:21.83 +03:15:27.3: 13.17 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:42.88 +09:27:34.6: 12.79 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:00.34 +09:13:29.5: 13.76 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:02.08 +09:47:44.6: 13.99 +/- 0.08 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:05.38 +10:07:04.6: 13.90 +/- 0.07 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:31:52.32 +08:55:21.0: 13.88 +/- 0.07 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:24:53.32 +09:30:55.3: 13.65 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 22:54:26.97 +06:34:55.3: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:19:42.30 +07:58:56.1: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter REJECTED candidate at 23:19:42.30 +07:58:56.1: ref_mag=12.54 +/- 0.01 new_mean_mag=12.2718 delta=0.27 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:21.83 +03:15:27.3: 13.16 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:31:52.32 +08:55:21.0: 13.78 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:31:31.72 +09:27:46.2: 13.07 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:42.88 +09:27:34.6: 12.81 +/- 0.02 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:00.34 +09:13:29.5: 13.47 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:05.38 +10:07:04.6: 13.80 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:02.08 +09:47:44.6: 13.92 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter KEPT candidate at 23:28:21.83 +03:15:27.3: ref_mag=13.17 +/- 0.03 new_mean_mag=12.2322 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry reference-image weighted average: 13.84 +/- 0.04
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Forced photometry filter KEPT candidate at 23:31:31.72 +09:27:46.2: ref_mag=13.11 +/- 0.02 new_mean_mag=12.1804 delta=0.93 (need > 0.90)
Forced photometry filter KEPT candidate at 23:31:52.32 +08:55:21.0: ref_mag=13.82 +/- 0.05 new_mean_mag=12.7061 delta=1.12 (need > 0.90)
Forced photometry filter KEPT candidate at 23:27:00.34 +09:13:29.5: ref_mag=13.56 +/- 0.03 new_mean_mag=12.6336 delta=0.93 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:27:42.88 +09:27:34.6: ref_mag=12.80 +/- 0.02 new_mean_mag=11.9167 delta=0.88 (need > 0.90)
Forced photometry filter KEPT candidate at 23:27:05.38 +10:07:04.6: ref_mag=13.84 +/- 0.04 new_mean_mag=12.7230 delta=1.12 (need > 0.90)
Forced photometry filter KEPT candidate at 23:28:02.08 +09:47:44.6: ref_mag=13.95 +/- 0.05 new_mean_mag=12.7672 delta=1.18 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:24:53.32 +09:30:55.3: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Forced photometry filter KEPT candidate at 23:24:53.32 +09:30:55.3: ref_mag=13.63 +/- 0.04 new_mean_mag=12.6274 delta=1.00 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:25:15.90 +10:12:58.3: 13.30 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:32:48.37 +09:08:42.0: 13.58 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:25:15.90 +10:12:58.3: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:32:48.37 +09:08:42.0: 13.66 +/- 0.05 detection
Forced photometry filter KEPT candidate at 23:25:15.90 +10:12:58.3: ref_mag=13.27 +/- 0.03 new_mean_mag=12.3454 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Forced photometry filter KEPT candidate at 23:32:48.37 +09:08:42.0: ref_mag=13.62 +/- 0.04 new_mean_mag=12.6910 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:17:59.88 +08:32:51.1: 13.55 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:17:59.88 +08:32:51.1: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter KEPT candidate at 23:17:59.88 +08:32:51.1: ref_mag=13.49 +/- 0.03 new_mean_mag=12.3182 delta=1.17 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:29:15.15 +09:32:33.7: 13.52 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:29:15.15 +09:32:33.7: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry filter KEPT candidate at 23:29:15.15 +09:32:33.7: ref_mag=13.47 +/- 0.03 new_mean_mag=12.4905 delta=0.98 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:24:11.45 +10:03:36.5: 13.53 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:24:11.45 +10:03:36.5: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry filter KEPT candidate at 23:24:11.45 +10:03:36.5: ref_mag=13.51 +/- 0.03 new_mean_mag=12.5433 delta=0.96 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:24:53.97 +10:11:15.8: 13.48 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:24:53.97 +10:11:15.8: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter KEPT candidate at 23:24:53.97 +10:11:15.8: ref_mag=13.43 +/- 0.03 new_mean_mag=12.4405 delta=0.99 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:32.42 +09:33:03.0: 13.41 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:32.42 +09:33:03.0: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Forced photometry filter KEPT candidate at 23:28:32.42 +09:33:03.0: ref_mag=13.46 +/- 0.03 new_mean_mag=12.5217 delta=0.94 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:30:36.38 +09:40:32.2: 13.38 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:30:36.38 +09:40:32.2: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter REJECTED candidate at 23:30:36.38 +09:40:32.2: ref_mag=13.36 +/- 0.03 new_mean_mag=12.4641 delta=0.90 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:04.73 +10:05:18.3: 13.34 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:36.28 +09:33:28.1: 13.41 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:31:49.90 +09:30:26.6: 13.39 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:04.73 +10:05:18.3: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter KEPT candidate at 23:28:04.73 +10:05:18.3: ref_mag=13.42 +/- 0.03 new_mean_mag=12.4800 delta=0.94 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:26:59.46 +10:10:53.6: 13.36 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:36.28 +09:33:28.1: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter KEPT candidate at 23:28:36.28 +09:33:28.1: ref_mag=13.40 +/- 0.03 new_mean_mag=12.4360 delta=0.96 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:31:49.90 +09:30:26.6: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:13.16 +09:52:39.6: 13.37 +/- 0.04 detection
Forced photometry filter KEPT candidate at 23:31:49.90 +09:30:26.6: ref_mag=13.33 +/- 0.03 new_mean_mag=12.3819 delta=0.95 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:26:59.46 +10:10:53.6: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Forced photometry filter KEPT candidate at 23:26:59.46 +10:10:53.6: ref_mag=13.29 +/- 0.03 new_mean_mag=12.3873 delta=0.90 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:32.73 +09:59:46.7: 13.35 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:13.16 +09:52:39.6: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter REJECTED candidate at 23:28:13.16 +09:52:39.6: ref_mag=13.27 +/- 0.03 new_mean_mag=12.4159 delta=0.86 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:32.73 +09:59:46.7: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 23:28:32.73 +09:59:46.7: ref_mag=13.35 +/- 0.03 new_mean_mag=12.3926 delta=0.96 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:58.08 +09:49:27.2: 13.30 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:58.08 +09:49:27.2: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Forced photometry filter KEPT candidate at 23:28:58.08 +09:49:27.2: ref_mag=13.32 +/- 0.03 new_mean_mag=12.3919 delta=0.92 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:21:05.62 +09:11:50.3: 13.31 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:36:10.16 +08:15:50.0: 13.33 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:21:05.62 +09:11:50.3: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter KEPT candidate at 23:21:05.62 +09:11:50.3: ref_mag=13.31 +/- 0.02 new_mean_mag=12.3799 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:36:10.16 +08:15:50.0: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Forced photometry filter KEPT candidate at 23:36:10.16 +08:15:50.0: ref_mag=13.23 +/- 0.03 new_mean_mag=12.3021 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:32:18.18 +09:06:33.0: 13.31 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:32:18.18 +09:06:33.0: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Forced photometry filter KEPT candidate at 23:32:18.18 +09:06:33.0: ref_mag=13.26 +/- 0.03 new_mean_mag=12.2900 delta=0.97 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:08.28 +10:00:55.1: 13.26 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:08.28 +10:00:55.1: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Forced photometry filter KEPT candidate at 23:27:08.28 +10:00:55.1: ref_mag=13.25 +/- 0.03 new_mean_mag=12.3490 delta=0.90 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:26:22.73 +09:29:02.7: 13.25 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:26:22.73 +09:29:02.7: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 23:26:22.73 +09:29:02.7: ref_mag=13.21 +/- 0.02 new_mean_mag=12.2396 delta=0.97 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:29:32.40 +09:38:00.6: 13.24 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:29:32.40 +09:38:00.6: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 23:29:32.40 +09:38:00.6: ref_mag=13.19 +/- 0.02 new_mean_mag=12.2169 delta=0.97 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:25:44.03 +09:20:44.1: 13.19 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:25:44.03 +09:20:44.1: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 23:25:44.03 +09:20:44.1: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1992 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:31:52.88 +09:01:03.1: 13.19 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:07:26.00 +03:48:37.9: 13.12 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:26:59.52 +09:37:32.6: 13.12 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:31:52.88 +09:01:03.1: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 23:31:52.88 +09:01:03.1: ref_mag=13.15 +/- 0.02 new_mean_mag=12.2247 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:07:26.00 +03:48:37.9: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 23:07:26.00 +03:48:37.9: ref_mag=13.10 +/- 0.02 new_mean_mag=12.0891 delta=1.01 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:26:59.52 +09:37:32.6: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 23:26:59.52 +09:37:32.6: ref_mag=13.09 +/- 0.02 new_mean_mag=12.1851 delta=0.91 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:25:29.07 +09:21:15.5: 13.10 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:35.26 +03:05:08.5: 13.09 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:25:29.07 +09:21:15.5: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter REJECTED candidate at 23:25:29.07 +09:21:15.5: ref_mag=13.07 +/- 0.02 new_mean_mag=12.1862 delta=0.89 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:35.26 +03:05:08.5: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 23:28:35.26 +03:05:08.5: ref_mag=13.11 +/- 0.02 new_mean_mag=12.0403 delta=1.07 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:08.67 +09:43:21.7: 13.03 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:07:10.20 +03:55:52.4: 13.02 +/- 0.03 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:08.67 +09:43:21.7: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 23:27:08.67 +09:43:21.7: ref_mag=13.05 +/- 0.02 new_mean_mag=12.1054 delta=0.94 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:07:10.20 +03:55:52.4: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 23:07:10.20 +03:55:52.4: ref_mag=13.03 +/- 0.02 new_mean_mag=12.0258 delta=1.00 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:25:43.52 +09:41:17.1: 13.97 +/- 0.07 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:25:43.52 +09:41:17.1: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.04
Forced photometry filter KEPT candidate at 23:25:43.52 +09:41:17.1: ref_mag=13.89 +/- 0.04 new_mean_mag=12.7096 delta=1.18 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:29:55.02 +09:29:47.9: 13.88 +/- 0.07 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:29:55.02 +09:29:47.9: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Forced photometry filter KEPT candidate at 23:29:55.02 +09:29:47.9: ref_mag=13.87 +/- 0.05 new_mean_mag=12.7822 delta=1.09 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:18.18 +09:32:40.0: 13.85 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:18.18 +09:32:40.0: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter KEPT candidate at 23:28:18.18 +09:32:40.0: ref_mag=13.76 +/- 0.04 new_mean_mag=12.7353 delta=1.03 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:29:19.43 +09:37:18.3: 13.77 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:29:19.43 +09:37:18.3: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry filter KEPT candidate at 23:29:19.43 +09:37:18.3: ref_mag=13.81 +/- 0.04 new_mean_mag=12.7121 delta=1.10 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:08.59 +09:19:08.1: 13.77 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:08.59 +09:19:08.1: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Forced photometry filter KEPT candidate at 23:27:08.59 +09:19:08.1: ref_mag=13.83 +/- 0.04 new_mean_mag=12.8100 delta=1.02 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:26:52.24 +09:22:15.0: 13.73 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:29:50.69 +09:50:34.5: 13.69 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:26:16.64 +09:32:22.2: 13.67 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:26:52.24 +09:22:15.0: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Forced photometry filter KEPT candidate at 23:26:52.24 +09:22:15.0: ref_mag=13.67 +/- 0.04 new_mean_mag=12.6939 delta=0.98 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:29:50.69 +09:50:34.5: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Forced photometry filter KEPT candidate at 23:29:50.69 +09:50:34.5: ref_mag=13.58 +/- 0.04 new_mean_mag=12.6095 delta=0.97 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:26:16.64 +09:32:22.2: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Forced photometry filter KEPT candidate at 23:26:16.64 +09:32:22.2: ref_mag=13.67 +/- 0.04 new_mean_mag=12.6611 delta=1.01 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:24:08.38 +10:10:06.3: 13.68 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:24:08.38 +10:10:06.3: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 23:24:08.38 +10:10:06.3: ref_mag=13.57 +/- 0.03 new_mean_mag=12.6242 delta=0.94 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:30:20.94 +09:31:43.8: 13.68 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:30:20.94 +09:31:43.8: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Forced photometry filter KEPT candidate at 23:30:20.94 +09:31:43.8: ref_mag=13.66 +/- 0.04 new_mean_mag=12.6391 delta=1.02 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:27:34.52 +09:53:26.8: 13.67 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:27:34.52 +09:53:26.8: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Forced photometry filter KEPT candidate at 23:27:34.52 +09:53:26.8: ref_mag=13.61 +/- 0.04 new_mean_mag=12.5999 delta=1.01 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:07.30 +09:34:52.4: 13.59 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:07.30 +09:34:52.4: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Forced photometry filter KEPT candidate at 23:28:07.30 +09:34:52.4: ref_mag=13.54 +/- 0.03 new_mean_mag=12.5733 delta=0.97 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:30:29.01 +09:25:19.9: 13.59 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:25:55.97 +10:07:53.4: 13.58 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:28:20.73 +09:41:52.4: 13.56 +/- 0.05 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:30:29.01 +09:25:19.9: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Forced photometry filter KEPT candidate at 23:30:29.01 +09:25:19.9: ref_mag=13.64 +/- 0.04 new_mean_mag=12.7419 delta=0.90 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:25:55.97 +10:07:53.4: 13.55 +/- 0.04 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:28:20.73 +09:41:52.4: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter KEPT candidate at 23:25:55.97 +10:07:53.4: ref_mag=13.56 +/- 0.03 new_mean_mag=12.5872 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 23:28:20.73 +09:41:52.4: ref_mag=13.45 +/- 0.03 new_mean_mag=12.3590 delta=1.10 (need > 0.90)
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-20_05-31-52_20.00sec_5.00C_LIGHT_0494.fits at 23:31:44.32 +09:30:06.3: 13.63 +/- 0.06 detection
Forced photometry on wcs_Psc-07-Q2b1x1_2026-07-22_05-03-25_20.00sec_4.90C_LIGHT_0466.fits at 23:31:44.32 +09:30:06.3: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Forced photometry filter KEPT candidate at 23:31:44.32 +09:30:06.3: ref_mag=13.60 +/- 0.04 new_mean_mag=12.6102 delta=0.99 (need > 0.90)
Adding exclusion_list_local.txt__out04085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53494.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 54s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 22s
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Considering the candidate 53489_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
The candidate 53489_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741 did not pass the final checks
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Considering the candidate 53494_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 53494_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06569_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06569_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 07893_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 07893_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 09108_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 09108_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 04466_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 04466_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 05607_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 05607_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06940_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
The candidate 06940_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741 did not pass the final checks
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Considering the candidate 33357_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 33357_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06903_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06903_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 04085_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 04085_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 08146_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 08146_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 10694_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 10694_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06574_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06574_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 04663_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 04663_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 04213_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 04213_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06565_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06565_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06022_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
The candidate 06022_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741 did not pass the final checks
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Considering the candidate 04507_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 04507_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06530_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06530_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06721_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06721_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 04214_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 04214_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 05285_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
The candidate 05285_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741 did not pass the final checks
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Considering the candidate 04858_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 04858_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 05468_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 05468_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 08032_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 08032_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 11702_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 11702_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 08306_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 08306_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 04794_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 04794_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06860_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06860_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06202_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06202_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 07444_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 07444_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 08693_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 08693_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 35286_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 35286_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06277_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06277_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 07410_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
The candidate 07410_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741 did not pass the final checks
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Considering the candidate 32629_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 32629_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 05852_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 05852_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 35884_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 35884_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06060_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06060_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06797_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06797_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06596_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06596_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06278_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06278_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 07545_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 07545_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 07336_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 07336_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 05386_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 05386_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06647_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06647_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 04296_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 04296_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06659_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06659_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 05244_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 05244_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
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Considering the candidate 06441_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06441_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07081_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 07081_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04413_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 04413_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05988_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 05988_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06730_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
Preparing report for the candidate 06730_fd_Psc-07-Q2b1x1_2026-09-04_06-11-57_20.00sec_0.00C_LIGHT_0741
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 79s
Prepared the HTML report for the field Psc-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:25:15.90 +10:12:58.3
23:24:53.97 +10:11:15.8
23:26:59.46 +10:10:53.6
23:24:08.38 +10:10:06.3
23:25:55.97 +10:07:53.4
23:27:05.38 +10:07:04.6
23:28:04.73 +10:05:18.3
23:24:11.45 +10:03:36.5
23:27:08.28 +10:00:55.1
23:28:32.73 +09:59:46.7
23:27:34.52 +09:53:26.8
23:29:50.69 +09:50:34.5
23:28:58.08 +09:49:27.2
23:28:02.08 +09:47:44.6
23:27:08.67 +09:43:21.7
23:28:20.73 +09:41:52.4
23:25:43.52 +09:41:17.1
23:29:32.40 +09:38:00.6
23:26:59.52 +09:37:32.6
23:29:19.43 +09:37:18.3
23:28:07.30 +09:34:52.4
23:28:36.28 +09:33:28.1
23:28:32.42 +09:33:03.0
23:24:53.32 +09:30:55.3
23:29:15.15 +09:32:33.7
23:28:18.18 +09:32:40.0
23:26:16.64 +09:32:22.2
23:30:20.94 +09:31:43.8
23:31:49.90 +09:30:26.6
23:31:44.32 +09:30:06.3
23:29:55.02 +09:29:47.9
23:26:22.73 +09:29:02.7
23:31:31.72 +09:27:46.2
23:30:29.01 +09:25:19.9
23:26:52.24 +09:22:15.0
23:25:44.03 +09:20:44.1
23:27:08.59 +09:19:08.1
23:27:00.34 +09:13:29.5
23:21:05.62 +09:11:50.3
23:32:48.37 +09:08:42.0
23:32:18.18 +09:06:33.0
23:31:52.88 +09:01:03.1
23:31:52.32 +08:55:21.0
23:17:59.88 +08:32:51.1
23:36:10.16 +08:15:50.0
23:28:35.26 +03:05:08.5
23:28:21.83 +03:15:27.3
23:07:26.00 +03:48:37.9
23:07:10.20 +03:55:52.4
22:54:26.97 +06:34:55.3
########### Completed Psc-07-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 ####
22:54:26.97 +06:34:55.3
23:24:53.32 +09:30:55.3
23:27:00.34 +09:13:29.5
23:31:52.32 +08:55:21.0
23:27:05.38 +10:07:04.6
23:28:02.08 +09:47:44.6
23:28:21.83 +03:15:27.3
23:31:31.72 +09:27:46.2
23:25:15.90 +10:12:58.3
23:32:48.37 +09:08:42.0
23:17:59.88 +08:32:51.1
23:29:15.15 +09:32:33.7
23:24:11.45 +10:03:36.5
23:24:53.97 +10:11:15.8
23:28:32.42 +09:33:03.0
23:28:04.73 +10:05:18.3
23:28:36.28 +09:33:28.1
23:31:49.90 +09:30:26.6
23:26:59.46 +10:10:53.6
23:28:32.73 +09:59:46.7
23:28:58.08 +09:49:27.2
23:21:05.62 +09:11:50.3
23:36:10.16 +08:15:50.0
23:32:18.18 +09:06:33.0
23:27:08.28 +10:00:55.1
23:26:22.73 +09:29:02.7
23:29:32.40 +09:38:00.6
23:25:44.03 +09:20:44.1
23:31:52.88 +09:01:03.1
23:07:26.00 +03:48:37.9
23:26:59.52 +09:37:32.6
23:28:35.26 +03:05:08.5
23:27:08.67 +09:43:21.7
23:07:10.20 +03:55:52.4
23:25:43.52 +09:41:17.1
23:29:55.02 +09:29:47.9
23:28:18.18 +09:32:40.0
23:29:19.43 +09:37:18.3
23:27:08.59 +09:19:08.1
23:26:52.24 +09:22:15.0
23:29:50.69 +09:50:34.5
23:26:16.64 +09:32:22.2
23:24:08.38 +10:10:06.3
23:30:20.94 +09:31:43.8
23:27:34.52 +09:53:26.8
23:28:07.30 +09:34:52.4
23:30:29.01 +09:25:19.9
23:25:55.97 +10:07:53.4
23:28:20.73 +09:41:52.4
23:31:44.32 +09:30:06.3
###################################################################################
22:54:26.97 +06:34:55.3 -- asteroid (will NOT add it to exclusion list)
23:24:53.32 +09:30:55.3 -- not an asteroid (will add it to exclusion list)
23:27:00.34 +09:13:29.5 -- not an asteroid (will add it to exclusion list)
23:31:52.32 +08:55:21.0 -- not an asteroid (will add it to exclusion list)
23:27:05.38 +10:07:04.6 -- not an asteroid (will add it to exclusion list)
23:28:02.08 +09:47:44.6 -- not an asteroid (will add it to exclusion list)
23:28:21.83 +03:15:27.3 -- not an asteroid (will add it to exclusion list)
23:31:31.72 +09:27:46.2 -- not an asteroid (will add it to exclusion list)
23:25:15.90 +10:12:58.3 -- not an asteroid (will add it to exclusion list)
23:32:48.37 +09:08:42.0 -- not an asteroid (will add it to exclusion list)
23:17:59.88 +08:32:51.1 -- not an asteroid (will add it to exclusion list)
23:29:15.15 +09:32:33.7 -- not an asteroid (will add it to exclusion list)
23:24:11.45 +10:03:36.5 -- not an asteroid (will add it to exclusion list)
23:24:53.97 +10:11:15.8 -- not an asteroid (will add it to exclusion list)
23:28:32.42 +09:33:03.0 -- not an asteroid (will add it to exclusion list)
23:28:04.73 +10:05:18.3 -- asteroid (will NOT add it to exclusion list)
23:28:36.28 +09:33:28.1 -- not an asteroid (will add it to exclusion list)
23:31:49.90 +09:30:26.6 -- not an asteroid (will add it to exclusion list)
23:26:59.46 +10:10:53.6 -- not an asteroid (will add it to exclusion list)
23:28:32.73 +09:59:46.7 -- asteroid (will NOT add it to exclusion list)
23:28:58.08 +09:49:27.2 -- not an asteroid (will add it to exclusion list)
23:21:05.62 +09:11:50.3 -- not an asteroid (will add it to exclusion list)
23:36:10.16 +08:15:50.0 -- not an asteroid (will add it to exclusion list)
23:32:18.18 +09:06:33.0 -- not an asteroid (will add it to exclusion list)
23:27:08.28 +10:00:55.1 -- not an asteroid (will add it to exclusion list)
23:26:22.73 +09:29:02.7 -- not an asteroid (will add it to exclusion list)
23:29:32.40 +09:38:00.6 -- not an asteroid (will add it to exclusion list)
23:25:44.03 +09:20:44.1 -- not an asteroid (will add it to exclusion list)
23:31:52.88 +09:01:03.1 -- not an asteroid (will add it to exclusion list)
23:07:26.00 +03:48:37.9 -- not an asteroid (will add it to exclusion list)
23:26:59.52 +09:37:32.6 -- not an asteroid (will add it to exclusion list)
23:28:35.26 +03:05:08.5 -- not an asteroid (will add it to exclusion list)
23:27:08.67 +09:43:21.7 -- not an asteroid (will add it to exclusion list)
23:07:10.20 +03:55:52.4 -- not an asteroid (will add it to exclusion list)
23:25:43.52 +09:41:17.1 -- not an asteroid (will add it to exclusion list)
23:29:55.02 +09:29:47.9 -- not an asteroid (will add it to exclusion list)
23:28:18.18 +09:32:40.0 -- not an asteroid (will add it to exclusion list)
23:29:19.43 +09:37:18.3 -- not an asteroid (will add it to exclusion list)
23:27:08.59 +09:19:08.1 -- not an asteroid (will add it to exclusion list)
23:26:52.24 +09:22:15.0 -- not an asteroid (will add it to exclusion list)
23:29:50.69 +09:50:34.5 -- not an asteroid (will add it to exclusion list)
23:26:16.64 +09:32:22.2 -- not an asteroid (will add it to exclusion list)
23:24:08.38 +10:10:06.3 -- not an asteroid (will add it to exclusion list)
23:30:20.94 +09:31:43.8 -- not an asteroid (will add it to exclusion list)
23:27:34.52 +09:53:26.8 -- asteroid (will NOT add it to exclusion list)
23:28:07.30 +09:34:52.4 -- not an asteroid (will add it to exclusion list)
23:30:29.01 +09:25:19.9 -- not an asteroid (will add it to exclusion list)
23:25:55.97 +10:07:53.4 -- not an asteroid (will add it to exclusion list)
23:28:20.73 +09:41:52.4 -- not an asteroid (will add it to exclusion list)
23:31:44.32 +09:30:06.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
23:07:10.20 +03:55:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:26.00 +03:48:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:59.88 +08:32:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:05.62 +09:11:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:08.38 +10:10:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:11.45 +10:03:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:53.32 +09:30:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:53.97 +10:11:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:15.90 +10:12:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:43.52 +09:41:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:44.03 +09:20:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:55.97 +10:07:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:16.64 +09:32:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:22.73 +09:29:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:52.24 +09:22:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:59.46 +10:10:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:59.52 +09:37:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:00.34 +09:13:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:05.38 +10:07:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:08.28 +10:00:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:08.59 +09:19:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:08.67 +09:43:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:02.08 +09:47:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:07.30 +09:34:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:18.18 +09:32:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:20.73 +09:41:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:21.83 +03:15:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:32.42 +09:33:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:35.26 +03:05:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:36.28 +09:33:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:58.08 +09:49:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:15.15 +09:32:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:19.43 +09:37:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:32.40 +09:38:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:50.69 +09:50:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:55.02 +09:29:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:20.94 +09:31:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:29.01 +09:25:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:31.72 +09:27:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:44.32 +09:30:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:49.90 +09:30:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:52.32 +08:55:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:52.88 +09:01:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:18.18 +09:06:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:48.37 +09:08:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:10.16 +08:15:50.0 -- 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)
23:07:10.20 +03:55:52.4 -- not a known variable star
23:07:26.00 +03:48:37.9 -- not a known variable star
23:17:59.88 +08:32:51.1 -- a known variable star
23:21:05.62 +09:11:50.3 -- not a known variable star
23:24:08.38 +10:10:06.3 -- not a known variable star
23:24:11.45 +10:03:36.5 -- not a known variable star
23:24:53.32 +09:30:55.3 -- not a known variable star
23:24:53.97 +10:11:15.8 -- not a known variable star
23:25:15.90 +10:12:58.3 -- not a known variable star
23:25:43.52 +09:41:17.1 -- not a known variable star
23:25:44.03 +09:20:44.1 -- not a known variable star
23:25:55.97 +10:07:53.4 -- not a known variable star
23:26:16.64 +09:32:22.2 -- not a known variable star
23:26:22.73 +09:29:02.7 -- not a known variable star
23:26:52.24 +09:22:15.0 -- not a known variable star
23:26:59.46 +10:10:53.6 -- not a known variable star
23:26:59.52 +09:37:32.6 -- not a known variable star
23:27:00.34 +09:13:29.5 -- not a known variable star
23:27:05.38 +10:07:04.6 -- not a known variable star
23:27:08.28 +10:00:55.1 -- not a known variable star
23:27:08.59 +09:19:08.1 -- not a known variable star
23:27:08.67 +09:43:21.7 -- not a known variable star
23:28:02.08 +09:47:44.6 -- not a known variable star
23:28:07.30 +09:34:52.4 -- not a known variable star
23:28:18.18 +09:32:40.0 -- not a known variable star
23:28:20.73 +09:41:52.4 -- not a known variable star
23:28:21.83 +03:15:27.3 -- not a known variable star
23:28:32.42 +09:33:03.0 -- not a known variable star
23:28:35.26 +03:05:08.5 -- not a known variable star
23:28:36.28 +09:33:28.1 -- not a known variable star
23:28:58.08 +09:49:27.2 -- not a known variable star
23:29:15.15 +09:32:33.7 -- not a known variable star
23:29:19.43 +09:37:18.3 -- not a known variable star
23:29:32.40 +09:38:00.6 -- not a known variable star
23:29:50.69 +09:50:34.5 -- not a known variable star
23:29:55.02 +09:29:47.9 -- not a known variable star
23:30:20.94 +09:31:43.8 -- not a known variable star
23:30:29.01 +09:25:19.9 -- not a known variable star
23:31:31.72 +09:27:46.2 -- not a known variable star
23:31:44.32 +09:30:06.3 -- not a known variable star
23:31:49.90 +09:30:26.6 -- not a known variable star
23:31:52.32 +08:55:21.0 -- not a known variable star
23:31:52.88 +09:01:03.1 -- not a known variable star
23:32:18.18 +09:06:33.0 -- not a known variable star
23:32:48.37 +09:08:42.0 -- not a known variable star
23:36:10.16 +08:15:50.0 -- not a known variable star
Found 45 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
46 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 46 (excluding asteroids and hot pixels, 45 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461287.96615403 -observatory V36
11:20:40.44 +05:40:52.8 Mercury (-1.1mag)
13:28:44.60 -13:25:14.1 Venus (-4.7mag)
07:06:18.57 +23:09:05.6 Mars (1.2mag)
09:06:42.32 +17:07:24.8 Jupiter (-1.8mag)
00:52:22.01 +02:43:10.0 Saturn (0.5mag)
04:13:38.31 +21:01:51.9 Uranus (5.7mag)
00:14:00.63 -00:01:26.3 Neptune (7.7mag)
20:25:47.60 -23:38:56.5 Pluto (14.5mag)
04:46:48.39 +27:21:29.6 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Sep 4 06:14 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461287.96615403:
09:06:38.35 +17:07:45.4 Io (6.2mag)
09:06:33.89 +17:08:06.8 Europa (6.3mag)
09:06:45.51 +17:07:12.0 Ganymede (5.7mag)
09:06:22.16 +17:09:01.8 Callisto (6.9mag)
09:04:23.36 +17:22:37.8 Himalia (15.7mag)
09:06:44.46 +17:07:15.1 Thebe (16.6mag)
09:04:02.02 +17:16:47.4 Elara (17.7mag)
09:10:39.62 +16:35:52.3 Pasiphae (17.9mag)
09:07:59.61 +17:24:25.2 Carme (19.0mag)
00:52:30.95 +02:43:16.0 Titan (8.3mag)
00:52:25.97 +02:42:53.0 Rhea (9.6mag)
00:52:44.20 +02:45:50.6 Iapetus (11.0mag)
00:52:27.25 +02:42:25.5 Hyperion (14.3mag)
00:51:11.78 +02:33:10.5 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 4 06:14 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461287.96615403:
21:41:38.59 -01:54:27.8 JWST
17:26:03.17 +36:48:55.3 Chandra
06:59:02.32 -01:00:50.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 4 06:14 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461287.96615403 -observatory V36
03:38:38.52 +19:12:14.2 17.4mag P/1996 R2 (Lagerkvist)
18:02:00.04 -34:15:44.6 14.3mag P/2010 H2 (Vales)
07:17:17.74 -70:08:50.9 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:15:20.60 +33:37:39.9 17.7mag C/2017 K2 (PANSTARRS)
04:47:04.16 +45:02:34.3 15.7mag P/2021 N1 (ZTF)
04:47:04.19 +45:02:34.2 15.7mag P/2021 N1 (ZTF)
22:15:45.96 +29:00:27.1 17.4mag C/2022 E2 (ATLAS)
07:07:59.63 +26:01:57.2 16.9mag C/2022 N2 (PANSTARRS)
10:46:53.08 +27:19:48.1 17.1mag C/2022 QE78 (ATLAS)
09:46:51.77 +05:14:52.8 18.0mag C/2022 R6 (PANSTARRS)
15:30:23.27 -15:24:00.6 14.8mag C/2023 R1 (PANSTARRS)
08:35:52.24 +32:43:20.2 15.8mag C/2024 E1 (Wierzchos)
15:06:16.53 +15:21:21.9 17.9mag C/2024 G6 (ATLAS)
18:35:30.33 +43:16:24.6 13.7mag C/2024 J3 (ATLAS)
20:30:06.26 +49:26:12.3 17.4mag C/2024 R4 (PANSTARRS)
05:34:02.96 -12:59:28.1 15.1mag C/2024 T5 (ATLAS)
07:10:35.93 +19:06:18.3 17.8mag C/2025 J1 (Borisov)
11:13:27.59 +18:59:17.4 16.9mag C/2025 V2 (Rankin)
13:17:19.65 +00:20:35.0 16.8mag C/2025 Y1 (ATLAS)
16:34:21.17 +74:29:01.6 16.2mag C/2026 A2 (Bok)
03:07:03.35 +46:12:46.3 17.4mag C/2026 B2 (Sun-Gao)
12:10:39.78 +11:03:00.9 17.5mag A/2026 E1
22:23:38.27 -34:47:34.7 13.3mag 10P/Tempel
11:46:17.07 -05:15:26.5 16.3mag 29P/Schwassmann-Wachmann
12:02:52.27 -04:11:45.9 17.6mag 63P/Wild
00:46:10.31 -06:53:19.4 15.4mag 65P/Gunn
06:33:47.37 +19:27:38.7 17.1mag 78P/Gehrels
03:16:57.46 +14:57:14.7 16.7mag 88P/Howell
05:28:53.65 +27:32:37.4 17.5mag 112P/Urata-Niijima
07:23:19.58 +25:31:15.1 17.9mag 114P/Wiseman-Skiff
10:21:33.06 +21:27:47.2 14.8mag 123P/West-Hartley
12:40:24.61 -20:20:43.6 17.4mag 124P/Mrkos
06:13:56.17 +20:43:24.7 15.9mag 128P/Shoemaker-Holt
23:53:46.76 +02:31:10.8 17.3mag 139P/Vaisala-Oterma
02:42:03.83 -17:53:49.6 15.4mag 161P/Hartley-IRAS
09:44:02.62 +15:42:27.8 12.0mag 169P/NEAT
03:21:52.65 +08:41:40.7 14.4mag 220P/McNaught
04:40:20.85 +35:25:03.1 15.2mag 260P/McNaught
08:24:12.92 +35:59:30.3 17.3mag 295P/LINEAR
15:23:26.69 +00:04:11.0 17.9mag 391P/Kowalski
09:25:19.79 +16:59:43.8 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.0K Sep 4 06:14 comets.txt
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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 4 06:14 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
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
-rw-r--r-- 1 apache apache 190K Sep 4 06:14 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:12:40.320 +04:03:41.65 AT 2026yfu 2026-08-06.43 21.27
17:57:17.885 +25:16:17.44 AT 2026yft 2026-08-06.41 20.23
15:51:50.093 +15:05:39.28 AT 2026yfs 2026-08-07.27 20.99
00:57:22.776 -24:27:56.06 AT 2026yfr 2026-06-23.81 20.08
00:30:20.591 -54:41:49.80 AT 2026yfq 2026-07-20.77 19.38
02:32:12.791 -22:10:48.74 AT 2026yfp 2026-07-20.79 19.5
01:41:52.083 -42:11:48.39 AT 2026yfo 2026-07-20.75 20.09
23:56:49.152 -38:37:39.87 AT 2026yfn 2026-07-27.78 19.61
23:42:35.374 -40:35:39.21 AT 2026yfm 2026-08-06.67 20.01
00:59:35.904 -40:19:34.17 AT 2026yfl 2026-08-06.70 20.35
00:09:47.092 -52:13:41.85 AT 2026yfk 2026-08-06.71 19.78
01:29:51.734 -23:34:18.41 AT 2026yfj 2026-08-06.73 19.55
02:10:09.536 -24:08:21.00 AT 2026yfi 2026-07-20.77 20.04
03:25:21.580 -50:44:20.31 AT 2026yfh 2026-08-06.77 20.01
04:26:28.926 -21:02:33.55 AT 2026yfg 2026-08-06.78 19.34
02:45:19.042 -55:38:20.40 AT 2026yff 2026-08-06.78 19.68
03:57:14.486 -09:10:35.02 AT 2026yfe 2026-08-06.79 19.58
04:48:25.059 -18:04:11.02 AT 2026yfd 2026-08-06.79 19.24
03:12:28.807 -53:09:31.17 AT 2026yfc 2026-08-06.80 20.22
03:12:34.990 -53:15:23.14 AT 2026yfb 2026-08-06.80 19.82
-rw-r--r-- 1 apache apache 88K Sep 4 06:14 tns_transients_list.txt
