This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 12.73 22:28:00.17 +15:19:24.4
79.25195 -35.11071 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 found in astcheck.225 Henrietta 1 -0 1 13.2 -0 0
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:28:00.17 +15:19:24.4: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:28:00.17 +15:19:24.4: 15.85 +/- 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,2461231.8870,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3870 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 12.29 21:43:24.65 +11:58:23.3
67.27076 -29.94016 galactic Peg Second-epoch detections are separated by 1.7" 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 | target | 21:43:24.65 +11:58:23.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.346+/-0.030 (G)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:43:24.65 +11:58:23.3: 13.21 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:43:24.65 +11:58:23.3: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 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,2461231.8870,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 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 07 10.3870 2461231.8870 12.20 21:42:44.54 +11:01:31.9
66.31954 -30.43895 galactic Peg Second-epoch detections are separated by 2.4" 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 | 21:42:44.54 +11:01:31.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:44.54 +11:01:31.9: 13.27 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:44.54 +11:01:31.9: 13.24 +/- 0.04 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,2461231.8870,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 11.91 21:42:18.39 +10:51:28.3
66.09118 -30.46726 galactic Peg Second-epoch detections are separated by 0.3" 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 | 21:42:18.39 +10:51:28.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.389+/-0.034 (G)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:18.39 +10:51:28.3: 13.09 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:18.39 +10:51:28.3: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 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,2461231.8870,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 11.82 21:42:33.33 +11:57:13.3
67.09488 -29.79567 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 | Gaia DR3 1766734870224906368 | 21:42:33.29 +11:57:14.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=0.783+/-0.030 (K)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:33.33 +11:57:13.3: 12.84 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:33.33 +11:57:13.3: 12.81 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1766734870224906368,2461231.8870,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1766734870224906368 20260710.3870 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 12.51 21:52:30.05 +17:59:40.1
73.98657 -27.41544 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 | 21:52:30.05 +17:59:40.1 (user input) | T | P | (position from user input) J-Ks=0.496+/-0.028 (K)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:52:30.05 +17:59:40.1: 13.35 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:52:30.05 +17:59:40.1: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 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,2461231.8870,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 12.33 21:43:08.67 +10:57:47.3
66.33959 -30.55442 galactic Peg Second-epoch detections are separated by 2.0" 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 | target | 21:43:08.67 +10:57:47.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.292+/-0.033 (F)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:43:08.67 +10:57:47.3: 13.34 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:43:08.67 +10:57:47.3: 13.35 +/- 0.05 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
target,2461231.8870,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 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 07 10.3870 2461231.8870 12.19 21:43:09.80 +10:44:26.4
66.14731 -30.70322 galactic Peg Second-epoch detections are separated by 2.8" and 9.9 pix
The object was found in VSX 2" Gaia DR3 1765746100034145792
Type: ROT
# Max. Min./Amp. JD0 Period
12.800 G 12.820 G K
The object was not found in astcheck.
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:43:09.80 +10:44:26.4: 13.13 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:43:09.80 +10:44:26.4: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 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
Gaia DR3 1765746100034145792,2461231.8870,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1765746100034145792 20260710.3870 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 07 10.3870 2461231.8870 12.16 21:42:00.37 +12:05:47.1
67.11680 -29.60061 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 | 21:42:00.37 +12:05:47.1 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.612+/-0.033 (K)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:00.37 +12:05:47.1: 13.13 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:00.37 +12:05:47.1: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.15 +/- 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,2461231.8870,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 12.24 21:42:56.87 +11:58:45.3
67.18990 -29.85102 galactic Peg Second-epoch detections are separated by 2.4" 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 | 21:42:56.87 +11:58:45.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:56.87 +11:58:45.3: 13.12 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:56.87 +11:58:45.3: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 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,2461231.8870,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 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 07 10.3870 2461231.8870 12.39 21:42:41.89 +10:44:30.8
66.06179 -30.61579 galactic Peg Second-epoch detections are separated by 3.7" and 8.9 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 | 21:42:41.89 +10:44:30.8 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.274+/-0.036 (F)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:41.89 +10:44:30.8: 13.47 +/- 0.06 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:41.89 +10:44:30.8: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 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,2461231.8870,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 12.19 21:43:08.67 +12:32:42.7
67.71528 -29.51300 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 | ATO J325.7774+12.5446 | 21:43:08.67 +12:32:42.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.461+/-0.033 (G)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:43:08.67 +12:32:42.7: 13.10 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:43:08.67 +12:32:42.7: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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 J325.7774+12.5446,2461231.8870,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.7774+12.5446 20260710.3870 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 07 10.3870 2461231.8870 9.58 21:43:05.04 +12:22:11.9
67.55308 -29.61796 galactic Peg Second-epoch detections are separated by 0.2" and 9.5 pix
The object was found in VSX 2" ASAS J214305+1222.1
Type: MISC
# Max. Min./Amp. JD0 Period
10.680 V Y 0.280 V 2452583.70000 141.915298000000
The object was not found in astcheck.
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:43:05.04 +12:22:11.9: 10.45 +/- 0.00 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:43:05.04 +12:22:11.9: 10.46 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.46 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J214305+1222.1,2461231.8870,9.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J214305+1222.1 20260710.3870 9.58CV 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 07 10.3870 2461231.8870 12.21 21:44:12.17 +12:52:32.7
68.19614 -29.48612 galactic Peg Second-epoch detections are separated by 3.3" 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 | 21:44:12.17 +12:52:32.7 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.027 (G)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:44:12.17 +12:52:32.7: 13.09 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:44:12.17 +12:52:32.7: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 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,2461231.8870,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 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 07 10.3870 2461231.8870 12.37 21:42:18.72 +12:18:19.7
67.35419 -29.51906 galactic Peg Second-epoch detections are separated by 1.8" 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 | 21:42:18.72 +12:18:19.7 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.304+/-0.033 (F)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:18.72 +12:18:19.7: 13.24 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:18.72 +12:18:19.7: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 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,2461231.8870,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 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 07 10.3870 2461231.8870 12.37 21:44:01.10 +12:57:42.7
68.23543 -29.39520 galactic Peg Second-epoch detections are separated by 0.3" 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 | 21:44:01.10 +12:57:42.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.697+/-0.026 (K)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:44:01.10 +12:57:42.7: 13.24 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:44:01.10 +12:57:42.7: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 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,2461231.8870,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 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 07 10.3870 2461231.8870 12.20 21:45:20.79 +10:54:05.1
66.69780 -31.00303 galactic Peg Second-epoch detections are separated by 0.8" 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 | 21:45:20.79 +10:54:05.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.339+/-0.033 (G)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:45:20.79 +10:54:05.1: 13.25 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:45:20.79 +10:54:05.1: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 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,2461231.8870,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 12.23 21:42:46.04 +10:48:27.3
66.13253 -30.58585 galactic Peg Second-epoch detections are separated by 1.8" 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 J325.6832+10.8100 | 21:42:46.04 +10:48:27.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.335+/-0.033 (G)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:46.04 +10:48:27.3: 13.24 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:46.04 +10:48:27.3: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 J325.6832+10.8100,2461231.8870,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.6832+10.8100 20260710.3870 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 12.27 21:42:38.55 +12:03:04.4
67.19557 -29.74744 galactic Peg Second-epoch detections are separated by 0.2" 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 | 21:42:38.55 +12:03:04.4 (user input) | T | P | (position from user input) J-Ks=0.489+/-0.074 (K)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:38.55 +12:03:04.4: 13.23 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:38.55 +12:03:04.4: 13.26 +/- 0.04 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,2461231.8870,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 12.17 21:42:49.56 +12:50:23.5
67.90924 -29.25942 galactic Peg Second-epoch detections are separated by 1.1" 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 | 21:42:49.56 +12:50:23.5 (user input) | T | P | (position from user input) J-Ks=0.416+/- (G)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:49.56 +12:50:23.5: 13.06 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:49.56 +12:50:23.5: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 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,2461231.8870,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 11.98 21:42:23.04 +12:00:10.0
67.10564 -29.73179 galactic Peg Second-epoch detections are separated by 1.7" 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 | 21:42:23.04 +12:00:10.0 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.689+/-0.028 (K)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:23.04 +12:00:10.0: 13.05 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:23.04 +12:00:10.0: 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,2461231.8870,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 11.88 21:41:57.97 +12:42:04.2
67.63104 -29.19429 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 | Gaia DR3 1767382546998137600 | 21:41:57.93 +12:42:05.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.388+/-0.028 (G)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:41:57.97 +12:42:04.2: 12.74 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:41:57.97 +12:42:04.2: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1767382546998137600,2461231.8870,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1767382546998137600 20260710.3870 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 11.94 21:47:55.35 +15:57:35.0
71.47831 -28.05572 galactic Peg Second-epoch detections are separated by 0.9" and 9.5 pix
The object was found in VSX 1" ASAS J214755+1557.6
Type: MISC
# Max. Min./Amp. JD0 Period
12.640 V Y 1.070 V 2452938.20000 88.952141000000
The object was not found in astcheck.
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:47:55.35 +15:57:35.0: 13.04 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:47:55.35 +15:57:35.0: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 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
ASAS J214755+1557.6,2461231.8870,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J214755+1557.6 20260710.3870 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 11.81 21:42:48.23 +12:13:43.5
67.37912 -29.65996 galactic Peg Second-epoch detections are separated by 0.5" 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 | ATO J325.7028+12.2297 | 21:42:48.23 +12:13:43.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.254+/-0.033 (F)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:48.23 +12:13:43.5: 12.72 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:48.23 +12:13:43.5: 12.75 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.74 +/- 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 J325.7028+12.2297,2461231.8870,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.7028+12.2297 20260710.3870 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 11.50 21:42:49.82 +12:26:41.3
67.57048 -29.52201 galactic Peg Second-epoch detections are separated by 1.8" 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 | Gaia DR3 1766800596108610304 | 21:42:49.80 +12:26:42.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.368+/-0.033 (G)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:49.82 +12:26:41.3: 12.43 +/- 0.02 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:49.82 +12:26:41.3: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1766800596108610304,2461231.8870,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1766800596108610304 20260710.3870 11.50CV 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 07 10.3870 2461231.8870 12.08 21:42:17.52 +10:53:57.2
66.12488 -30.43761 galactic Peg Second-epoch detections are separated by 1.2" and 9.7 pix
The object was found in VSX 3" Gaia DR3 1765799117110461696
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.040 G 13.080 G G
The object was not found in astcheck.
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:17.52 +10:53:57.2: 13.02 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:17.52 +10:53:57.2: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1765799117110461696,2461231.8870,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1765799117110461696 20260710.3870 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 12.21 21:44:15.49 +10:54:46.7
66.50355 -30.79392 galactic Peg Second-epoch detections are separated by 4.1" and 8.9 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 | 21:44:15.49 +10:54:46.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.345+/-0.037 (G)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:44:15.49 +10:54:46.7: 13.21 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:44:15.49 +10:54:46.7: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 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,2461231.8870,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 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 07 10.3870 2461231.8870 12.40 21:45:05.40 +10:57:29.3
66.69937 -30.91830 galactic Peg Second-epoch detections are separated by 0.3" 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 | 21:45:05.40 +10:57:29.3 (user input) | T | P | (position from user input) J-Ks=0.292+/-0.037 (F)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:45:05.40 +10:57:29.3: 13.36 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:45:05.40 +10:57:29.3: 13.34 +/- 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
target,2461231.8870,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3870 2461231.8870 12.04 21:43:36.79 +12:18:33.2
67.59915 -29.75504 galactic Peg Second-epoch detections are separated by 0.5" 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 | 21:43:36.79 +12:18:33.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.371+/-0.028 (G)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:43:36.79 +12:18:33.2: 12.92 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:43:36.79 +12:18:33.2: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 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,2461231.8870,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3870 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461201.91884477 10.06.2026 10:02:58.188 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
First image: 2461201.91884477 10.06.2026 10:02:58.188 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
Last image: 2461231.88736968 10.07.2026 09:17:38.740 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.76
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: 20 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 9849
Objects passed selection criteria: 9815
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 7328.5
Average stars matched: 6985.25 (95.3162 %)
Memory usage VmPeak: 115560 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 05:03:46 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: 2461201.91884477 10.06.2026 10:02:58.188 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
First image: 2461201.91884477 10.06.2026 10:02:58.188 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
Last image: 2461231.88736968 10.07.2026 09:17:38.740 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 133
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.48
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: 66 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 59065
Objects passed selection criteria: 58915
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 45292.5
Average stars matched: 42677.5 (94.2264 %)
Memory usage VmPeak: 159312 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 05:07:48 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
SExtractor catalog cache: saved Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.cat to cache
SExtractor catalog cache: saved Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.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/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.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: 2461231.88669264
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_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits exists and is non-empty
Saving wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits to local_wcs_cache/
'wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits' -> 'local_wcs_cache/wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits'
wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits exists and is non-empty
Saving wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits to local_wcs_cache/
'wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits' -> 'local_wcs_cache/wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits'
wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits exists and is non-empty
Saving wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits to local_wcs_cache/
'wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits' -> 'local_wcs_cache/wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits'
wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits exists and is non-empty
Saving wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits to local_wcs_cache/
'wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits' -> 'local_wcs_cache/wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits (1st reference image)
verification OK: wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
Image size: 937.2'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: 22:13:21.520 +14:00:21.77 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_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits (1st new image)
verification OK: wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
Image size: 940.9'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:13:20.645 +14:00:00.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:13:21.520 +14:00:21.77
Second-epoch image center 22:13:20.645 +14:00:00.79
Angular distance between the image centers 0.0068 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits (2nd new image)
verification OK: wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:13:23.505 +14:00:39.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:13:21.520 +14:00:21.77
Second-epoch image center 22:13:23.505 +14:00:39.60
Angular distance between the image centers 0.0094 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 22:13:20.645 +14:00:00.79
Second-epoch second image center 22:13:23.505 +14:00:39.60
Angular distance between the image centers 0.01581 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/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits &> /tmp/tmp.5fZPZVUYk2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits &> /tmp/tmp.E7n9xHiIox
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits &> /tmp/tmp.4QiW695zoA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits &> /tmp/tmp.iwAkZ8W4Dj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.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_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits and wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.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_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits and wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat
Found non-empty wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits and wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat
The reference image (wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits) and catalog (wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat) found
'wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat' -> 'wcsmag.cat'
Read 9949 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.0575 to 341.5411 deg, Dec +8.6479 to +19.2700 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 325.0575 to 341.5411 deg, Dec 8.6479 to 19.2700 deg
Loaded 7919 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): 6371 out of 6549 total matches.
Matched with Tycho-2 6549 out of 9949 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.710200
a=0.000000 b=1.000000 c=22.710200
From vast_summary.log: estimated ref. image limiting mag.: -7.76
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.95
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.95
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9949 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.0575 to 341.5411 deg, Dec +8.6479 to +19.2700 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 325.0575 to 341.5411 deg, Dec 8.6479 to 19.2700 deg
Loaded 7919 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): 6371 out of 6549 total matches.
Matched with Tycho-2 6549 out of 9949 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits:
Forced-photometry filter: calibrated wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits -> calib.txt_param_ref_wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits (aperture=6.4)
Read 10923 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.0575 to 341.5411 deg, Dec +8.6481 to +19.2842 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 325.0575 to 341.5411 deg, Dec 8.6481 to 19.2842 deg
Loaded 7932 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): 6481 out of 6677 total matches.
Matched with Tycho-2 6677 out of 10923 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits:
Forced-photometry filter: calibrated wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits -> calib.txt_param_ref_wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
2.3 pix Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
2.9 pix fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
2.8 pix fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
2.3 pix wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
2.3 pix wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
Limiting magnitude estimates:
14.9 mag. Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
15.1 mag. Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
13.6 mag. fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
13.2 mag. fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5fZPZVUYk2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits' -> 'wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
WCS_IMAGE_NAME=wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
WCS-calibrated image found: wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
Checking if the catalog wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat corresponding to the image wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits alredy exist and is non-empty...
Catalog wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat corresponding to the image wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
WCS catalog name: wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=529, bad_region=0, passed=9949
Got 9949 stars (including 9416 good ones) from the SExtractor catalog wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat
util/solve_plate_with_UCAC5 got 9949 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
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 9762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 9763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 9764 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits N_match=932 sigma_overall_arcsec=0.472 sigma_q1_arcsec=0.363 sigma_q2_arcsec=0.615 sigma_q3_arcsec=0.405 sigma_q4_arcsec=0.646 n_q1=228 n_q2=225 n_q3=204 n_q4=275 worst_quadrant_to_overall_ratio=1.369
The image catalog is written to wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits -region wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.E7n9xHiIox (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits' -> 'wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
WCS_IMAGE_NAME=wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
WCS-calibrated image found: wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
Checking if the catalog wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat corresponding to the image wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits alredy exist and is non-empty...
Catalog wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat corresponding to the image wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
WCS catalog name: wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=582, bad_region=0, passed=10923
Got 10923 stars (including 10329 good ones) from the SExtractor catalog wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat
util/solve_plate_with_UCAC5 got 10923 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
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 10708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 10709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 10709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits N_match=930 sigma_overall_arcsec=0.482 sigma_q1_arcsec=0.388 sigma_q2_arcsec=0.589 sigma_q3_arcsec=0.446 sigma_q4_arcsec=0.623 n_q1=226 n_q2=224 n_q3=203 n_q4=277 worst_quadrant_to_overall_ratio=1.293
The image catalog is written to wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits -region wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4QiW695zoA (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
Checking if the catalog wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
WCS catalog name: wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=154, bad_region=0, passed=4929
Got 4929 stars (including 4769 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat
util/solve_plate_with_UCAC5 got 4929 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 4794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 4797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 4797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits N_match=925 sigma_overall_arcsec=0.323 sigma_q1_arcsec=0.408 sigma_q2_arcsec=0.362 sigma_q3_arcsec=0.260 sigma_q4_arcsec=0.300 n_q1=213 n_q2=255 n_q3=155 n_q4=302 worst_quadrant_to_overall_ratio=1.262
The image catalog is written to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits -region wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.iwAkZ8W4Dj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
Checking if the catalog wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
WCS catalog name: wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=110, bad_region=0, passed=3666
Got 3666 stars (including 3551 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat
util/solve_plate_with_UCAC5 got 3666 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 3583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 3585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 3585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits N_match=927 sigma_overall_arcsec=0.305 sigma_q1_arcsec=0.351 sigma_q2_arcsec=0.344 sigma_q3_arcsec=0.267 sigma_q4_arcsec=0.296 n_q1=232 n_q2=216 n_q3=200 n_q4=279 worst_quadrant_to_overall_ratio=1.150
The image catalog is written to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits -region wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits sigma_overall=0.472 worst_q_ratio=1.369
ref2=Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits sigma_overall=0.482 worst_q_ratio=1.293
new1=fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits sigma_overall=0.323 worst_q_ratio=1.262
new2=fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits sigma_overall=0.305 worst_q_ratio=1.150
reference average sigma_overall=0.477 worst_q_ratio=1.331
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214_astrometric_residuals.png (932 matched stars from wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333_astrometric_residuals.png (930 matched stars from wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358_astrometric_residuals.png (925 matched stars from wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359_astrometric_residuals.png (927 matched stars from wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits'
Saving fully-calibrated image wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits'
Preparing the HTML report for the field Peg-09-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00375_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 00375_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:41:06.40 +09:07:09.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00222_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 00222_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:42:33.30 +08:58:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03648_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 03648_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 21:45:04.74 +12:41:55.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00302_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 00302_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:43:14.63 +09:02:52.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Peg-09-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
SExtractor catalog cache: saved Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.cat to cache
SExtractor catalog cache: saved Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
Creating symlink local_wcs_cache/wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits exists and is non-empty
wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits exists and is non-empty
wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits exists and is non-empty
wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits (1st reference image)
verification OK: wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
Image size: 937.2'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: 22:13:21.520 +14:00:21.77 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_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits (1st new image)
verification OK: wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
Image size: 940.9'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:13:20.645 +14:00:00.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:13:21.520 +14:00:21.77
Second-epoch image center 22:13:20.645 +14:00:00.79
Angular distance between the image centers 0.0068 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits (2nd new image)
verification OK: wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:13:23.505 +14:00:39.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:13:21.520 +14:00:21.77
Second-epoch image center 22:13:23.505 +14:00:39.60
Angular distance between the image centers 0.0094 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 22:13:20.645 +14:00:00.79
Second-epoch second image center 22:13:23.505 +14:00:39.60
Angular distance between the image centers 0.01581 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/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits &> /tmp/tmp.HYyDMi4xfk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits &> /tmp/tmp.H25ngqPdZ7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits &> /tmp/tmp.HTGLLwuzR7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits &> /tmp/tmp.akcDDAcLPQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.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_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits and wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.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_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits and wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat
Found non-empty wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits and wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat
The reference image (wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits) and catalog (wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat) found
'wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat' -> 'wcsmag.cat'
Read 60901 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.0575 to 341.5468 deg, Dec +8.6371 to +19.2735 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 325.0575 to 341.5468 deg, Dec 8.6371 to 19.2735 deg
Loaded 7933 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): 6225 out of 6878 total matches.
Matched with Tycho-2 6878 out of 60901 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.586600
a=0.000000 b=1.000000 c=22.586600
From vast_summary.log: estimated ref. image limiting mag.: -7.48
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.11
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.11
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 60901 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.0575 to 341.5468 deg, Dec +8.6371 to +19.2735 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 325.0575 to 341.5468 deg, Dec 8.6371 to 19.2735 deg
Loaded 7933 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): 6225 out of 6878 total matches.
Matched with Tycho-2 6878 out of 60901 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits:
Forced-photometry filter: calibrated wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits -> calib.txt_param_ref_wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits (aperture=5.0)
Read 67363 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.0562 to 341.5411 deg, Dec +8.6388 to +19.2844 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 325.0562 to 341.5411 deg, Dec 8.6388 to 19.2844 deg
Loaded 7939 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): 6123 out of 6870 total matches.
Matched with Tycho-2 6870 out of 67363 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits:
Forced-photometry filter: calibrated wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits -> calib.txt_param_ref_wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 89 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
2.1 pix Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
2.7 pix fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
2.6 pix fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
2.2 pix wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
2.1 pix wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
Limiting magnitude estimates:
15.1 mag. Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
15.2 mag. Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
13.7 mag. fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
13.4 mag. fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 13.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.HYyDMi4xfk (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits' -> 'wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
WCS_IMAGE_NAME=wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
WCS-calibrated image found: wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
Checking if the catalog wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat corresponding to the image wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits alredy exist and is non-empty...
Catalog wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat corresponding to the image wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits
WCS catalog name: wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=3198, bad_region=0, passed=60888
Got 60888 stars (including 57612 good ones) from the SExtractor catalog wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat
util/solve_plate_with_UCAC5 got 60888 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
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 59726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 59723 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 59723 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits N_match=926 sigma_overall_arcsec=0.464 sigma_q1_arcsec=0.361 sigma_q2_arcsec=0.580 sigma_q3_arcsec=0.404 sigma_q4_arcsec=0.601 n_q1=226 n_q2=213 n_q3=202 n_q4=285 worst_quadrant_to_overall_ratio=1.296
The image catalog is written to wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits -region wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.H25ngqPdZ7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits' -> 'wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
WCS_IMAGE_NAME=wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
WCS-calibrated image found: wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
Checking if the catalog wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat corresponding to the image wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits alredy exist and is non-empty...
Catalog wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat corresponding to the image wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits
WCS catalog name: wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=4227, bad_region=1, passed=67340
Got 67340 stars (including 63016 good ones) from the SExtractor catalog wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat
util/solve_plate_with_UCAC5 got 67340 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
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 65814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 65812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 65812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits N_match=925 sigma_overall_arcsec=0.483 sigma_q1_arcsec=0.374 sigma_q2_arcsec=0.607 sigma_q3_arcsec=0.458 sigma_q4_arcsec=0.599 n_q1=225 n_q2=213 n_q3=201 n_q4=286 worst_quadrant_to_overall_ratio=1.255
The image catalog is written to wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits -region wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.HTGLLwuzR7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
Checking if the catalog wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
WCS catalog name: wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=847, bad_region=7, passed=30622
Got 30622 stars (including 29709 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat
util/solve_plate_with_UCAC5 got 30622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 29663 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 29664 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 29664 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits N_match=925 sigma_overall_arcsec=0.332 sigma_q1_arcsec=0.436 sigma_q2_arcsec=0.363 sigma_q3_arcsec=0.273 sigma_q4_arcsec=0.324 n_q1=211 n_q2=255 n_q3=153 n_q4=306 worst_quadrant_to_overall_ratio=1.313
The image catalog is written to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits -region wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.akcDDAcLPQ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
Checking if the catalog wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
WCS catalog name: wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=563, bad_region=9, passed=23850
Got 23850 stars (including 23229 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat
util/solve_plate_with_UCAC5 got 23850 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 23433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 23435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 23435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits N_match=928 sigma_overall_arcsec=0.322 sigma_q1_arcsec=0.403 sigma_q2_arcsec=0.372 sigma_q3_arcsec=0.264 sigma_q4_arcsec=0.286 n_q1=225 n_q2=221 n_q3=199 n_q4=283 worst_quadrant_to_overall_ratio=1.252
The image catalog is written to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits -region wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-16-40_20.00sec_-0.00C_LIGHTs_0358.fits
Saving fully-calibrated image wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-09-Q1b1x1_041819_TTUQ1b1x1_288933_aGAAHAtr/wcs_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359.fits
Preparing the HTML report for the field Peg-09-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:40:40.44 +17:10:58.4: 12.71 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:44:24.75 +14:16:53.4: 12.58 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:43:33.30 +18:30:48.4: 13.06 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:43:05.19 +10:51:06.2: 12.97 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:45:07.46 +17:14:18.4: 13.12 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:57:31.50 +14:29:47.2: 10.87 +/- 0.00 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:42:11.65 +11:00:44.1: 12.14 +/- 0.02 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:45:07.46 +17:14:18.4: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Forced photometry filter REJECTED candidate at 22:45:07.46 +17:14:18.4: ref_mag=13.14 +/- 0.03 new_mean_mag=12.8257 delta=0.32 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:44:24.75 +14:16:53.4: 12.52 +/- 0.02 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:43:05.19 +10:51:06.2: 13.02 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:43:33.30 +18:30:48.4: 13.05 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.02
Forced photometry filter REJECTED candidate at 22:44:24.75 +14:16:53.4: ref_mag=12.54 +/- 0.02 new_mean_mag=12.3937 delta=0.15 (need > 0.90)
Forced photometry reference-image weighted average: 12.99 +/- 0.03
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:57:31.50 +14:29:47.2: 10.93 +/- 0.00 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:40:40.44 +17:10:58.4: 12.67 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 22:43:05.19 +10:51:06.2: ref_mag=12.99 +/- 0.03 new_mean_mag=12.9294 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.05 +/- 0.03
Forced photometry filter REJECTED candidate at 22:43:33.30 +18:30:48.4: ref_mag=13.05 +/- 0.03 new_mean_mag=12.6640 delta=0.39 (need > 0.90)
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Forced photometry reference-image weighted average: 10.90 +/- 0.00
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:28:00.17 +15:19:24.4: 15.72 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 22:40:40.44 +17:10:58.4: ref_mag=12.68 +/- 0.02 new_mean_mag=12.3183 delta=0.36 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:57:31.50 +14:29:47.2: ref_mag=10.90 +/- 0.00 new_mean_mag=11.0330 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:42:11.65 +11:00:44.1: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry filter REJECTED candidate at 22:42:11.65 +11:00:44.1: ref_mag=12.15 +/- 0.01 new_mean_mag=11.8773 delta=0.27 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:24:48.82 +09:48:32.4: 13.09 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:28:00.17 +15:19:24.4: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:24:48.82 +09:48:32.4: 13.16 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Forced photometry filter REJECTED candidate at 22:24:48.82 +09:48:32.4: ref_mag=13.13 +/- 0.03 new_mean_mag=12.7174 delta=0.41 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:46:06.02 +18:00:47.0: 99.00 +/- 99.00 edge
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:51:06.52 +18:03:12.0: 12.66 +/- 0.02 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:51:04.20 +10:22:20.5: 12.64 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:43:11.96 +17:04:36.2: 13.42 +/- 0.06 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:14:23.15 +17:12:33.5: 12.45 +/- 0.02 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:46:06.02 +18:00:47.0: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:46:06.02 +18:00:47.0: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:39:26.85 +10:15:30.1: 14.11 +/- 0.11 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:51:04.20 +10:22:20.5: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Forced photometry filter REJECTED candidate at 21:51:04.20 +10:22:20.5: ref_mag=12.64 +/- 0.02 new_mean_mag=12.2322 delta=0.40 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:51:06.52 +18:03:12.0: 12.64 +/- 0.02 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:43:11.96 +17:04:36.2: 13.42 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:14:23.15 +17:12:33.5: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.04
Forced photometry filter REJECTED candidate at 22:43:11.96 +17:04:36.2: ref_mag=13.42 +/- 0.04 new_mean_mag=13.1805 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry filter REJECTED candidate at 22:14:23.15 +17:12:33.5: ref_mag=12.45 +/- 0.01 new_mean_mag=12.5111 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:51:06.52 +18:03:12.0: ref_mag=12.65 +/- 0.02 new_mean_mag=12.2193 delta=0.43 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:43:24.27 +13:38:20.8: 13.21 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:39:26.85 +10:15:30.1: 13.98 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Forced photometry filter REJECTED candidate at 22:39:26.85 +10:15:30.1: ref_mag=14.03 +/- 0.06 new_mean_mag=13.2123 delta=0.81 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:42:29.41 +09:45:42.1: 14.44 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:43:24.27 +13:38:20.8: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:46:03.08 +17:41:05.1: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:43:24.27 +13:38:20.8: ref_mag=13.18 +/- 0.03 new_mean_mag=13.2983 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:42:29.41 +09:45:42.1: 14.82 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.12
Forced photometry filter KEPT candidate at 22:42:29.41 +09:45:42.1: ref_mag=14.60 +/- 0.12 new_mean_mag=13.5380 delta=1.06 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:44:15.87 +16:21:58.5: 14.33 +/- 0.13 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:46:03.08 +17:41:05.1: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:46:03.08 +17:41:05.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:39:31.10 +09:52:01.8: 14.62 +/- 0.18 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:45:32.08 +15:58:45.4: 14.49 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:38:46.41 +15:54:30.7: 14.54 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:45:59.88 +17:22:23.8: 99.00 +/- 99.00 edge
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:38:21.46 +17:12:23.1: 14.59 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:44:15.87 +16:21:58.5: 14.54 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.10
Forced photometry filter REJECTED candidate at 22:44:15.87 +16:21:58.5: ref_mag=14.43 +/- 0.10 new_mean_mag=13.5778 delta=0.85 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:45:32.08 +15:58:45.4: 14.34 +/- 0.12 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:39:31.10 +09:52:01.8: 15.01 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.09
Forced photometry reference-image weighted average: 14.78 +/- 0.14
Forced photometry filter REJECTED candidate at 22:45:32.08 +15:58:45.4: ref_mag=14.40 +/- 0.09 new_mean_mag=13.6114 delta=0.79 (need > 0.90)
Forced photometry filter KEPT candidate at 22:39:31.10 +09:52:01.8: ref_mag=14.78 +/- 0.14 new_mean_mag=13.5291 delta=1.26 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:38:46.41 +15:54:30.7: 14.65 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.10
Forced photometry filter KEPT candidate at 22:38:46.41 +15:54:30.7: ref_mag=14.60 +/- 0.10 new_mean_mag=13.4634 delta=1.14 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:45:59.88 +17:22:23.8: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:45:59.88 +17:22:23.8: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:38:21.46 +17:12:23.1: 14.74 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.11
Forced photometry filter REJECTED candidate at 22:38:21.46 +17:12:23.1: ref_mag=14.66 +/- 0.11 new_mean_mag=13.7672 delta=0.89 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:43:24.65 +11:58:23.3: 13.21 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:43:24.65 +11:58:23.3: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry filter KEPT candidate at 21:43:24.65 +11:58:23.3: ref_mag=13.20 +/- 0.03 new_mean_mag=12.2725 delta=0.93 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:44.54 +11:01:31.9: 13.27 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:18.39 +10:51:28.3: 13.09 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:18.39 +10:51:28.3: 13.01 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:44.54 +11:01:31.9: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.03
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:42:37.00 +10:06:03.5: 13.07 +/- 0.04 detection
Forced photometry filter KEPT candidate at 21:42:18.39 +10:51:28.3: ref_mag=13.04 +/- 0.03 new_mean_mag=11.9063 delta=1.14 (need > 0.90)
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Forced photometry filter KEPT candidate at 21:42:44.54 +11:01:31.9: ref_mag=13.25 +/- 0.03 new_mean_mag=12.1871 delta=1.06 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:33.33 +11:57:13.3: 12.84 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:42:37.00 +10:06:03.5: 13.08 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:52:30.05 +17:59:40.1: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry filter REJECTED candidate at 22:42:37.00 +10:06:03.5: ref_mag=13.08 +/- 0.03 new_mean_mag=12.3787 delta=0.70 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:33.33 +11:57:13.3: 12.81 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter KEPT candidate at 21:42:33.33 +11:57:13.3: ref_mag=12.82 +/- 0.02 new_mean_mag=11.7976 delta=1.02 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:43:18.03 +10:38:36.9: 12.98 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:52:30.05 +17:59:40.1: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 21:52:30.05 +17:59:40.1: ref_mag=13.38 +/- 0.03 new_mean_mag=12.4597 delta=0.92 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:43:08.67 +10:57:47.3: 13.34 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:43:18.03 +10:38:36.9: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Forced photometry filter REJECTED candidate at 22:43:18.03 +10:38:36.9: ref_mag=12.98 +/- 0.03 new_mean_mag=12.3285 delta=0.65 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:43:08.67 +10:57:47.3: 13.35 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 21:43:08.67 +10:57:47.3: ref_mag=13.35 +/- 0.03 new_mean_mag=12.3353 delta=1.01 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:43:09.80 +10:44:26.4: 13.13 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:00.37 +12:05:47.1: 13.13 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:43:09.80 +10:44:26.4: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Forced photometry filter KEPT candidate at 21:43:09.80 +10:44:26.4: ref_mag=13.19 +/- 0.03 new_mean_mag=12.1858 delta=1.00 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:42:03.21 +08:53:53.9: 13.63 +/- 0.08 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:00.37 +12:05:47.1: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.03
Forced photometry filter KEPT candidate at 21:42:00.37 +12:05:47.1: ref_mag=13.15 +/- 0.03 new_mean_mag=12.1674 delta=0.99 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:42:03.21 +08:53:53.9: 13.82 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.06
Forced photometry filter REJECTED candidate at 22:42:03.21 +08:53:53.9: ref_mag=13.72 +/- 0.06 new_mean_mag=12.8952 delta=0.83 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:56.87 +11:58:45.3: 13.12 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:42:18.43 +10:37:40.5: 12.81 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:56.87 +11:58:45.3: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Forced photometry filter KEPT candidate at 21:42:56.87 +11:58:45.3: ref_mag=13.09 +/- 0.03 new_mean_mag=12.1768 delta=0.92 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:42:18.43 +10:37:40.5: 12.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter REJECTED candidate at 22:42:18.43 +10:37:40.5: ref_mag=12.82 +/- 0.02 new_mean_mag=12.3266 delta=0.49 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:41.89 +10:44:30.8: 13.47 +/- 0.06 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:40:48.04 +10:07:02.2: 14.27 +/- 0.13 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:41.89 +10:44:30.8: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Forced photometry filter KEPT candidate at 21:42:41.89 +10:44:30.8: ref_mag=13.48 +/- 0.04 new_mean_mag=12.3862 delta=1.09 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:40:48.04 +10:07:02.2: 14.24 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.08
Forced photometry filter REJECTED candidate at 22:40:48.04 +10:07:02.2: ref_mag=14.25 +/- 0.08 new_mean_mag=13.4029 delta=0.85 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:43:08.67 +12:32:42.7: 13.10 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:43:08.67 +12:32:42.7: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Forced photometry filter KEPT candidate at 21:43:08.67 +12:32:42.7: ref_mag=13.10 +/- 0.03 new_mean_mag=12.1608 delta=0.94 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:43:05.04 +12:22:11.9: 10.45 +/- 0.00 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:43:05.04 +12:22:11.9: 10.46 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.46 +/- 0.00
Forced photometry filter KEPT candidate at 21:43:05.04 +12:22:11.9: ref_mag=10.46 +/- 0.00 new_mean_mag=9.5420 delta=0.92 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:44:12.17 +12:52:32.7: 13.09 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:44:01.10 +12:57:42.7: 13.24 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:18.72 +12:18:19.7: 13.24 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:44:12.17 +12:52:32.7: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Forced photometry filter KEPT candidate at 21:44:12.17 +12:52:32.7: ref_mag=13.13 +/- 0.03 new_mean_mag=12.2128 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:44:01.10 +12:57:42.7: 13.36 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:18.72 +12:18:19.7: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry filter KEPT candidate at 21:44:01.10 +12:57:42.7: ref_mag=13.30 +/- 0.03 new_mean_mag=12.3485 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Forced photometry filter KEPT candidate at 21:42:18.72 +12:18:19.7: ref_mag=13.28 +/- 0.03 new_mean_mag=12.3591 delta=0.92 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:47:02.11 +10:54:23.8: 12.96 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:42:46.30 +10:10:57.9: 12.65 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:47:02.11 +10:54:23.8: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter REJECTED candidate at 21:47:02.11 +10:54:23.8: ref_mag=13.00 +/- 0.02 new_mean_mag=12.1699 delta=0.83 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:42:46.30 +10:10:57.9: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry filter REJECTED candidate at 22:42:46.30 +10:10:57.9: ref_mag=12.65 +/- 0.02 new_mean_mag=12.0090 delta=0.64 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:45:20.79 +10:54:05.1: 13.25 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:45:20.79 +10:54:05.1: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Forced photometry filter KEPT candidate at 21:45:20.79 +10:54:05.1: ref_mag=13.28 +/- 0.03 new_mean_mag=12.1953 delta=1.08 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:46.04 +10:48:27.3: 13.24 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:38.55 +12:03:04.4: 13.23 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:46.04 +10:48:27.3: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry filter KEPT candidate at 21:42:46.04 +10:48:27.3: ref_mag=13.20 +/- 0.03 new_mean_mag=12.2286 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:38.55 +12:03:04.4: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Forced photometry filter KEPT candidate at 21:42:38.55 +12:03:04.4: ref_mag=13.25 +/- 0.03 new_mean_mag=12.1902 delta=1.06 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:49.56 +12:50:23.5: 13.06 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:49.56 +12:50:23.5: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Forced photometry filter KEPT candidate at 21:42:49.56 +12:50:23.5: ref_mag=13.09 +/- 0.03 new_mean_mag=12.1599 delta=0.93 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:23.04 +12:00:10.0: 13.05 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:41:57.97 +12:42:04.2: 12.74 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:23.04 +12:00:10.0: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 21:42:23.04 +12:00:10.0: ref_mag=13.03 +/- 0.02 new_mean_mag=11.9701 delta=1.06 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:41:57.97 +12:42:04.2: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Forced photometry filter KEPT candidate at 21:41:57.97 +12:42:04.2: ref_mag=12.74 +/- 0.02 new_mean_mag=11.8125 delta=0.92 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:37:02.31 +09:08:50.0: 14.10 +/- 0.11 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:37:02.31 +09:08:50.0: 14.04 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.08
Forced photometry filter KEPT candidate at 22:37:02.31 +09:08:50.0: ref_mag=14.07 +/- 0.08 new_mean_mag=13.0055 delta=1.06 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:42:20.33 +10:42:59.0: 13.38 +/- 0.06 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:42:20.33 +10:42:59.0: 13.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.04
Forced photometry filter REJECTED candidate at 22:42:20.33 +10:42:59.0: ref_mag=13.41 +/- 0.04 new_mean_mag=12.8395 delta=0.57 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:43:04.88 +10:11:07.9: 13.10 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:43:04.88 +10:11:07.9: 13.06 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry filter REJECTED candidate at 22:43:04.88 +10:11:07.9: ref_mag=13.08 +/- 0.03 new_mean_mag=12.4814 delta=0.59 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:47:55.35 +15:57:35.0: 13.04 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:47:55.35 +15:57:35.0: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 21:47:55.35 +15:57:35.0: ref_mag=13.01 +/- 0.02 new_mean_mag=11.9229 delta=1.09 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:48.23 +12:13:43.5: 12.72 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:48.23 +12:13:43.5: 12.75 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Forced photometry filter KEPT candidate at 21:42:48.23 +12:13:43.5: ref_mag=12.74 +/- 0.02 new_mean_mag=11.7548 delta=0.98 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:49.82 +12:26:41.3: 12.43 +/- 0.02 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:42:17.52 +10:53:57.2: 13.02 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:49.82 +12:26:41.3: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter KEPT candidate at 21:42:49.82 +12:26:41.3: ref_mag=12.41 +/- 0.01 new_mean_mag=11.4846 delta=0.92 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:42:17.52 +10:53:57.2: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 21:42:17.52 +10:53:57.2: ref_mag=13.00 +/- 0.02 new_mean_mag=12.0839 delta=0.92 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:44:15.49 +10:54:46.7: 13.21 +/- 0.04 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:44:15.49 +10:54:46.7: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Forced photometry filter KEPT candidate at 21:44:15.49 +10:54:46.7: ref_mag=13.24 +/- 0.03 new_mean_mag=12.2063 delta=1.04 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:45:05.40 +10:57:29.3: 13.36 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:45:05.40 +10:57:29.3: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 21:45:05.40 +10:57:29.3: ref_mag=13.35 +/- 0.03 new_mean_mag=12.3779 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 21:43:36.79 +12:18:33.2: 12.92 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-10_05-02-58_20.00sec_5.00C_LIGHT_0214.fits at 22:40:05.96 +09:25:02.5: 14.30 +/- 0.13 detection
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 21:43:36.79 +12:18:33.2: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter KEPT candidate at 21:43:36.79 +12:18:33.2: ref_mag=12.92 +/- 0.02 new_mean_mag=11.9726 delta=0.94 (need > 0.90)
Forced photometry on wcs_Peg-09-Q1b1x1_2026-06-11_04-38-38_20.00sec_5.00C_LIGHT_0333.fits at 22:40:05.96 +09:25:02.5: 14.15 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.08
Forced photometry filter KEPT candidate at 22:40:05.96 +09:25:02.5: ref_mag=14.20 +/- 0.08 new_mean_mag=13.2923 delta=0.91 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out71280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out09926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80278.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 53s
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: 16s
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Considering the candidate 79859_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 79859_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 79861_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 79861_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 79863_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 79863_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80035_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80035_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80118_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80118_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:43:09.73 +10:13:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80166_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80166_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80169_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80169_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80190_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80190_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:10:44.31 +11:38:22.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 80247_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80247_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:43:41.00 +17:42:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80260_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80260_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80278_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 80278_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
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Considering the candidate 80303_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80303_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:39:01.38 +09:57:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80319_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80319_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80321_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80321_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80346_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80346_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80361_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80361_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80366_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80366_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80403_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80403_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:41:33.04 +10:54:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80559_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80559_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:41:49.47 +08:50:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80575_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80575_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80576_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80576_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80620_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80620_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80737_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80737_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80750_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80750_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:42:29.41 +09:45:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.278 2716617156032293248 340.62258557618 +09.76260408696 14.0693 13.4628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80771_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80771_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80798_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80798_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:39:31.10 +09:52:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.000 2717054177544564096 339.87951418911 +09.86771808783 14.0371 13.3462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80925_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80925_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 80930_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80930_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:38:46.41 +15:54:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.129 2733513213777734656 339.69336020803 +15.90856081402 14.2832 13.5021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80935_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 80935_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 81084_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 81084_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 16609_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 16609_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
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Considering the candidate 71003_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71003_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:41:37.10 +10:06:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11461_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 11461_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
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Considering the candidate 10533_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 10533_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
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Considering the candidate 16501_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 16501_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
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Considering the candidate 05331_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 05331_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:40:33.84 +09:55:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48325_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 48325_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
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Considering the candidate 06174_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 06174_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11061_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 11061_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
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Considering the candidate 02481_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 02481_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:40:43.11 +09:17:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08910_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 08910_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09926_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 09926_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
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Considering the candidate 17379_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 17379_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
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Considering the candidate 00702_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 00702_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72276_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 72276_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:43:21.45 +09:25:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16668_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 16668_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
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Considering the candidate 08815_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 08815_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09946_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 09946_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
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Considering the candidate 72170_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 72170_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
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Considering the candidate 19876_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 19876_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05238_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 05238_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:41:23.78 +09:53:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04161_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 04161_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:37:41.53 +09:41:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71946_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71946_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:39:28.96 +09:24:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18652_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 18652_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
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Considering the candidate 71865_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71865_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:41:38.23 +09:43:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21755_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 21755_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18552_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 18552_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22271_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 22271_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10602_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 10602_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06590_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 06590_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10654_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 10654_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10291_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 10291_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17057_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 17057_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21576_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 21576_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02666_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 02666_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:38:44.07 +09:20:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16821_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 16821_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20813_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 20813_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71566_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71566_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:40:54.44 +09:17:11.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71504_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71504_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:39:21.80 +09:21:03.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71477_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71477_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:41:09.57 +09:35:39.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71293_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71293_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:38:22.51 +09:26:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71280_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71280_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:37:02.31 +09:08:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.644 2716864644932416896 339.25942754836 +09.14763509143 13.7991 13.2199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09314_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 09314_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71091_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71091_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:41:36.30 +09:55:28.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71087_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71087_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:38:31.03 +08:55:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71083_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71083_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:38:15.45 +09:03:38.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71069_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71069_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71066_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 71066_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:38:54.04 +09:10:05.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40170_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 40170_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18046_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 18046_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19308_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 19308_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10726_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 10726_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20093_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 20093_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 21:45:04.75 +12:41:56.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10762_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 10762_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55563_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 55563_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 21:58:30.91 +16:35:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10946_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 10946_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02815_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 02815_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:37:55.20 +09:23:01.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18493_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
Preparing report for the candidate 18493_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72633_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359
The candidate 72633_fd_Peg-09-Q1b1x1_2026-07-10_04-17-38_20.00sec_-0.00C_LIGHTs_0359 did not pass the final checks
**** FOUND 22:40:05.96 +09:25:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 2.325 2716974978347595392 340.02489354698 +09.41800432746 13.8591 13.2700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 72s
Prepared the HTML report for the field Peg-09-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:43:09.80 +10:44:26.4
21:42:41.89 +10:44:30.8
21:42:46.04 +10:48:27.3
21:42:18.39 +10:51:28.3
21:45:20.79 +10:54:05.1
21:42:17.52 +10:53:57.2
21:44:15.49 +10:54:46.7
21:45:05.40 +10:57:29.3
21:43:08.67 +10:57:47.3
21:42:44.54 +11:01:31.9
21:42:33.33 +11:57:13.3
21:43:24.65 +11:58:23.3
21:42:56.87 +11:58:45.3
21:42:23.04 +12:00:10.0
21:42:38.55 +12:03:04.4
21:42:00.37 +12:05:47.1
21:42:48.23 +12:13:43.5
21:43:36.79 +12:18:33.2
21:42:18.72 +12:18:19.7
21:43:05.04 +12:22:11.9
21:42:49.82 +12:26:41.3
21:43:08.67 +12:32:42.7
21:41:57.97 +12:42:04.2
21:42:49.56 +12:50:23.5
21:44:12.17 +12:52:32.7
21:44:01.10 +12:57:42.7
21:47:55.35 +15:57:35.0
21:52:30.05 +17:59:40.1
22:28:00.17 +15:19:24.4
########### Completed Peg-09-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
22:28:00.17 +15:19:24.4
21:43:24.65 +11:58:23.3
21:42:44.54 +11:01:31.9
21:42:18.39 +10:51:28.3
21:42:33.33 +11:57:13.3
21:52:30.05 +17:59:40.1
21:43:08.67 +10:57:47.3
21:43:09.80 +10:44:26.4
21:42:00.37 +12:05:47.1
21:42:56.87 +11:58:45.3
21:42:41.89 +10:44:30.8
21:43:08.67 +12:32:42.7
21:43:05.04 +12:22:11.9
21:44:12.17 +12:52:32.7
21:42:18.72 +12:18:19.7
21:44:01.10 +12:57:42.7
21:45:20.79 +10:54:05.1
21:42:46.04 +10:48:27.3
21:42:38.55 +12:03:04.4
21:42:49.56 +12:50:23.5
21:42:23.04 +12:00:10.0
21:41:57.97 +12:42:04.2
21:47:55.35 +15:57:35.0
21:42:48.23 +12:13:43.5
21:42:49.82 +12:26:41.3
21:42:17.52 +10:53:57.2
21:44:15.49 +10:54:46.7
21:45:05.40 +10:57:29.3
21:43:36.79 +12:18:33.2
###################################################################################
22:28:00.17 +15:19:24.4 -- asteroid (will NOT add it to exclusion list)
21:43:24.65 +11:58:23.3 -- not an asteroid (will add it to exclusion list)
21:42:44.54 +11:01:31.9 -- not an asteroid (will add it to exclusion list)
21:42:18.39 +10:51:28.3 -- not an asteroid (will add it to exclusion list)
21:42:33.33 +11:57:13.3 -- not an asteroid (will add it to exclusion list)
21:52:30.05 +17:59:40.1 -- not an asteroid (will add it to exclusion list)
21:43:08.67 +10:57:47.3 -- not an asteroid (will add it to exclusion list)
21:43:09.80 +10:44:26.4 -- not an asteroid (will add it to exclusion list)
21:42:00.37 +12:05:47.1 -- not an asteroid (will add it to exclusion list)
21:42:56.87 +11:58:45.3 -- not an asteroid (will add it to exclusion list)
21:42:41.89 +10:44:30.8 -- not an asteroid (will add it to exclusion list)
21:43:08.67 +12:32:42.7 -- not an asteroid (will add it to exclusion list)
21:43:05.04 +12:22:11.9 -- not an asteroid (will add it to exclusion list)
21:44:12.17 +12:52:32.7 -- not an asteroid (will add it to exclusion list)
21:42:18.72 +12:18:19.7 -- not an asteroid (will add it to exclusion list)
21:44:01.10 +12:57:42.7 -- not an asteroid (will add it to exclusion list)
21:45:20.79 +10:54:05.1 -- not an asteroid (will add it to exclusion list)
21:42:46.04 +10:48:27.3 -- not an asteroid (will add it to exclusion list)
21:42:38.55 +12:03:04.4 -- not an asteroid (will add it to exclusion list)
21:42:49.56 +12:50:23.5 -- not an asteroid (will add it to exclusion list)
21:42:23.04 +12:00:10.0 -- not an asteroid (will add it to exclusion list)
21:41:57.97 +12:42:04.2 -- not an asteroid (will add it to exclusion list)
21:47:55.35 +15:57:35.0 -- not an asteroid (will add it to exclusion list)
21:42:48.23 +12:13:43.5 -- not an asteroid (will add it to exclusion list)
21:42:49.82 +12:26:41.3 -- not an asteroid (will add it to exclusion list)
21:42:17.52 +10:53:57.2 -- not an asteroid (will add it to exclusion list)
21:44:15.49 +10:54:46.7 -- not an asteroid (will add it to exclusion list)
21:45:05.40 +10:57:29.3 -- not an asteroid (will add it to exclusion list)
21:43:36.79 +12:18:33.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:41:57.97 +12:42:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:00.37 +12:05:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:17.52 +10:53:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:18.39 +10:51:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:18.72 +12:18:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:23.04 +12:00:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:33.33 +11:57:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:38.55 +12:03:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:41.89 +10:44:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:44.54 +11:01:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:46.04 +10:48:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:48.23 +12:13:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:49.56 +12:50:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:49.82 +12:26:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:56.87 +11:58:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:05.04 +12:22:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:08.67 +10:57:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:08.67 +12:32:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:09.80 +10:44:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:24.65 +11:58:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:36.79 +12:18:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:01.10 +12:57:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:12.17 +12:52:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:15.49 +10:54:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:05.40 +10:57:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:20.79 +10:54:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:55.35 +15:57:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:30.05 +17:59:40.1 -- 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)
21:41:57.97 +12:42:04.2 -- not a known variable star
21:42:00.37 +12:05:47.1 -- not a known variable star
21:42:17.52 +10:53:57.2 -- a known variable star
21:42:18.39 +10:51:28.3 -- not a known variable star
21:42:18.72 +12:18:19.7 -- not a known variable star
21:42:23.04 +12:00:10.0 -- not a known variable star
21:42:33.33 +11:57:13.3 -- not a known variable star
21:42:38.55 +12:03:04.4 -- not a known variable star
21:42:41.89 +10:44:30.8 -- not a known variable star
21:42:44.54 +11:01:31.9 -- not a known variable star
21:42:46.04 +10:48:27.3 -- not a known variable star
21:42:48.23 +12:13:43.5 -- not a known variable star
21:42:49.56 +12:50:23.5 -- not a known variable star
21:42:49.82 +12:26:41.3 -- not a known variable star
21:42:56.87 +11:58:45.3 -- not a known variable star
21:43:05.04 +12:22:11.9 -- a known variable star
21:43:08.67 +10:57:47.3 -- not a known variable star
21:43:08.67 +12:32:42.7 -- not a known variable star
21:43:09.80 +10:44:26.4 -- a known variable star
21:43:24.65 +11:58:23.3 -- not a known variable star
21:43:36.79 +12:18:33.2 -- not a known variable star
21:44:01.10 +12:57:42.7 -- not a known variable star
21:44:12.17 +12:52:32.7 -- not a known variable star
21:44:15.49 +10:54:46.7 -- not a known variable star
21:45:05.40 +10:57:29.3 -- not a known variable star
21:45:20.79 +10:54:05.1 -- not a known variable star
21:47:55.35 +15:57:35.0 -- a known variable star
21:52:30.05 +17:59:40.1 -- not a known variable star
Found 24 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
28 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
21:41:57.97 +12:42:04.2
21:42:00.37 +12:05:47.1
21:42:17.52 +10:53:57.2
21:42:18.39 +10:51:28.3
21:42:18.72 +12:18:19.7
21:42:23.04 +12:00:10.0
21:42:33.33 +11:57:13.3
21:42:38.55 +12:03:04.4
21:42:41.89 +10:44:30.8
21:42:44.54 +11:01:31.9
21:42:46.04 +10:48:27.3
21:42:48.23 +12:13:43.5
21:42:49.56 +12:50:23.5
21:42:49.82 +12:26:41.3
21:42:56.87 +11:58:45.3
21:43:05.04 +12:22:11.9
21:43:08.67 +10:57:47.3
21:43:08.67 +12:32:42.7
21:43:09.80 +10:44:26.4
21:43:24.65 +11:58:23.3
21:43:36.79 +12:18:33.2
21:44:01.10 +12:57:42.7
21:44:12.17 +12:52:32.7
21:44:15.49 +10:54:46.7
21:45:05.40 +10:57:29.3
21:45:20.79 +10:54:05.1
21:47:55.35 +15:57:35.0
21:52:30.05 +17:59:40.1
22:37:02.31 +09:08:50.0
22:40:05.96 +09:25:02.5
22:42:29.41 +09:45:42.1
22:39:31.10 +09:52:01.8
22:38:46.41 +15:54:30.7
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461231.88669264 -observatory V36
07:32:11.17 +17:07:56.3 Mercury (5.1mag)
10:11:47.97 +12:40:02.8 Venus (-4.1mag)
04:24:16.77 +21:25:28.8 Mars (1.3mag)
08:16:42.55 +20:11:22.8 Jupiter (-1.8mag)
00:55:51.15 +03:20:29.7 Saturn (0.7mag)
04:07:14.46 +20:45:04.5 Uranus (5.8mag)
00:17:01.49 +00:20:41.0 Neptune (7.8mag)
20:30:54.74 -23:18:01.6 Pluto (14.4mag)
03:13:58.09 +22:34:02.0 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 361 Jul 10 05:03 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461231.88669264:
08:16:49.67 +20:10:57.8 Io (6.1mag)
08:16:46.04 +20:11:11.6 Europa (6.3mag)
08:16:59.75 +20:10:20.5 Ganymede (5.6mag)
08:17:10.38 +20:09:39.9 Callisto (6.8mag)
08:15:13.94 +19:55:33.3 Himalia (15.7mag)
08:16:42.79 +20:11:22.7 Thebe (16.6mag)
08:14:35.27 +20:00:02.3 Elara (17.6mag)
08:20:14.84 +20:05:31.8 Pasiphae (17.8mag)
08:21:40.28 +20:16:28.1 Carme (19.0mag)
00:55:41.10 +03:20:20.1 Titan (8.5mag)
00:55:45.90 +03:20:32.1 Rhea (9.8mag)
00:55:20.39 +03:19:38.2 Iapetus (11.2mag)
00:56:00.25 +03:20:49.0 Hyperion (14.5mag)
00:55:51.82 +03:17:43.2 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 05:04 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.88669264:
17:46:02.42 -32:57:47.8 JWST
16:20:13.27 +47:37:15.2 Chandra
04:50:15.67 +49:54:53.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 05:03 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.88669264 -observatory V36
02:36:19.18 +14:25:57.1 17.9mag P/1996 R2 (Lagerkvist)
18:17:54.70 -34:21:48.9 13.7mag P/2010 H2 (Vales)
06:25:42.61 -68:08:25.0 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:49.11 +32:26:51.2 17.6mag C/2017 K2 (PANSTARRS)
17:03:06.35 +16:02:53.8 18.0mag C/2021 G2 (ATLAS)
01:48:00.34 +08:17:31.7 15.4mag P/2021 N1 (ZTF)
22:59:30.62 +32:17:08.0 17.3mag C/2022 E2 (ATLAS)
06:12:26.40 +26:55:33.7 16.7mag C/2022 N2 (PANSTARRS)
09:55:32.75 +29:46:45.6 16.8mag C/2022 QE78 (ATLAS)
09:09:45.48 +04:59:59.7 17.8mag C/2022 R6 (PANSTARRS)
18:07:11.78 +21:17:33.2 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:35.00 -11:23:18.7 17.7mag P/2023 B1 (PANSTARRS)
21:49:11.53 +67:37:16.3 17.8mag C/2023 H5 (Lemmon)
16:30:48.93 -10:04:54.7 13.9mag C/2023 R1 (PANSTARRS)
08:00:42.70 +65:42:37.1 17.9mag C/2024 A1 (ATLAS)
07:32:51.67 +30:00:18.6 14.6mag C/2024 E1 (Wierzchos)
15:16:18.54 +15:19:45.5 17.5mag C/2024 G6 (ATLAS)
19:41:15.89 +39:23:59.9 13.8mag C/2024 J3 (ATLAS)
21:47:32.80 +46:00:30.9 17.8mag C/2024 R4 (PANSTARRS)
04:49:40.35 -13:47:39.5 15.7mag C/2024 T5 (ATLAS)
06:34:36.16 +29:03:50.7 18.0mag C/2025 J1 (Borisov)
07:14:21.89 -12:53:33.8 16.5mag C/2025 R3 (PANSTARRS)
09:56:07.94 +22:26:07.4 17.6mag C/2025 V2 (Rankin)
12:44:37.72 +03:56:10.9 17.1mag C/2025 Y1 (ATLAS)
16:51:51.14 +79:07:15.6 17.4mag C/2026 A2 (Bok)
02:46:18.81 +45:14:29.4 16.7mag C/2026 B2 (Sun-Gao)
11:25:32.01 +04:33:01.5 16.9mag A/2026 E1
21:19:05.24 -15:05:19.1 7.3mag 10P/Tempel
11:13:28.28 -01:53:19.1 16.1mag 29P/Schwassmann-Wachmann
04:00:13.35 +29:33:25.3 17.8mag 47P/Ashbrook-Jackson
10:08:08.97 +14:00:01.5 17.0mag 63P/Wild
00:48:22.65 -05:05:33.7 15.5mag 65P/Gunn
08:27:03.72 +34:13:02.2 17.9mag 76P/West-Kohoutek-Ikemura
04:27:28.92 +20:10:50.5 13.7mag 78P/Gehrels
02:22:23.43 +10:36:51.9 16.2mag 88P/Howell
06:35:38.06 +30:31:58.5 15.7mag 93P/Lovas
04:21:06.68 +31:07:28.8 16.9mag 114P/Wiseman-Skiff
08:08:46.76 +30:41:59.1 15.2mag 123P/West-Hartley
10:48:11.78 +01:10:22.3 16.8mag 124P/Mrkos
04:51:47.03 +20:48:50.5 16.2mag 128P/Shoemaker-Holt
05:36:19.27 +19:42:49.9 17.8mag 131P/Mueller
00:01:33.28 +02:56:11.9 17.9mag 139P/Vaisala-Oterma
07:13:41.46 +17:00:48.2 15.5mag 141P-D/Machholz
03:16:51.85 -21:06:11.1 15.5mag 161P/Hartley-IRAS
05:33:11.28 +33:57:22.7 15.3mag 162P/SidingSpring
19:04:23.03 +15:06:11.2 14.7mag 169P/NEAT
01:41:06.75 +07:36:09.6 17.7mag 220P/McNaught
16:35:57.78 -08:23:11.9 17.0mag 235P/LINEAR
08:45:21.54 +33:17:46.7 17.9mag 240P/NEAT
20:42:09.46 -49:34:41.9 17.8mag 259P/Garradd
01:59:24.13 +12:06:39.5 15.7mag 260P/McNaught
05:37:19.85 +36:50:45.1 17.4mag 295P/LINEAR
15:06:36.66 +06:03:13.9 17.6mag 391P/Kowalski
08:34:38.08 +19:40:31.4 17.9mag 450P/LONEOS
07:51:49.27 +39:12:48.0 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 05:03 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
-rw-r--r-- 1 apache apache 5.6K Jul 10 05:03 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 10 05:03 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:36:21.258 +13:42:31.91 AT 2026sqg 2026-07-06.96 17.376
10:38:47.961 +53:30:34.10 SN 2026sqf 2026-07-08.25 12.9
13:40:20.447 +40:38:15.61 AT 2026sqe 2026-07-03.20 20.3209
20:26:11.475 -21:05:59.62 AT 2026sqd 2026-07-07.33 20.2909
20:38:05.960 -15:39:19.94 AT 2026sqc 2026-07-07.33 22.2834
21:50:20.218 -14:25:11.02 AT 2026sqb 2026-07-07.39 21.5547
20:32:17.644 -16:37:51.49 AT 2026sqa 2026-07-07.33 21.6569
20:38:02.144 -16:39:15.94 AT 2026spz 2026-07-07.33 22.7762
20:36:24.191 -15:13:43.37 AT 2026spy 2026-07-07.33 22.1739
20:41:10.988 -25:49:45.49 AT 2026spx 2026-07-07.33 22.8645
21:17:15.336 -23:31:53.39 AT 2026spw 2026-07-07.32 21.9459
20:27:45.431 -19:59:58.81 AT 2026spv 2026-07-07.33 21.6485
21:55:34.604 -14:11:57.66 AT 2026spu 2026-07-07.39 23.0585
21:10:34.181 -22:59:24.76 AT 2026spt 2026-07-07.32 22.3526
21:05:55.405 -19:04:02.26 AT 2026sps 2026-07-07.32 21.4424
20:59:14.423 -27:33:25.12 AT 2026spr 2026-07-07.32 23.4151
20:31:34.503 -19:06:25.71 AT 2026spq 2026-07-07.33 22.7105
20:54:43.024 -26:43:41.99 AT 2026spp 2026-07-07.32 22.8017
21:07:49.748 -22:55:35.56 AT 2026spo 2026-07-07.32 22.494
20:57:55.962 -26:08:04.97 AT 2026spn 2026-07-07.32 22.7486
-rw-r--r-- 1 apache apache 30K Jul 10 05:03 tns_transients_list.txt
