This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT
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 10.3417 2461231.8417 13.73 23:10:55.61 +21:40:12.8
93.94449 -35.48125 galactic Peg Second-epoch detections are separated by 1.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.978 Aidamina -1 -0 1 14.2 -0 0
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:10:55.61 +21:40:12.8: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:10:55.61 +21:40:12.8: 16.18 +/- 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,2461231.8417,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3417 13.73CV 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 10.3417 2461231.8417 13.18 23:01:26.85 +21:13:24.1
91.31798 -34.80846 galactic Peg Second-epoch detections are separated by 1.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:01:26.85 +21:13:24.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.446+/-0.031 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:01:26.85 +21:13:24.1: 14.13 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:01:26.85 +21:13:24.1: 14.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.10 +/- 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,2461231.8417,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.37 23:02:34.54 +21:47:11.4
91.93486 -34.45023 galactic Peg Second-epoch detections are separated by 1.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:02:34.54 +21:47:11.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.564+/-0.028 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:34.54 +21:47:11.4: 14.46 +/- 0.07 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:34.54 +21:47:11.4: 14.35 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8417,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.37CV 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 10.3417 2461231.8417 13.11 23:06:12.24 +21:32:16.1
92.68301 -35.07856 galactic Peg Second-epoch detections are separated by 1.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:06:12.24 +21:32:16.1 (user input) | T | P | (position from user input) J-Ks=0.467+/-0.029 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:06:12.24 +21:32:16.1: 13.98 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:06:12.24 +21:32:16.1: 14.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8417,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.11 23:06:59.27 +22:06:38.1
93.21212 -34.66296 galactic Peg Second-epoch detections are separated by 0.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:06:59.27 +22:06:38.1 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.381+/-0.038 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:06:59.27 +22:06:38.1: 14.00 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:06:59.27 +22:06:38.1: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 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,2461231.8417,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.03 23:03:55.48 +23:47:03.9
93.42844 -32.85559 galactic Peg Second-epoch detections are separated by 1.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:03:55.48 +23:47:03.9 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.032 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:55.48 +23:47:03.9: 13.86 +/- 0.04 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:55.48 +23:47:03.9: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461231.8417,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.23 23:03:27.64 +25:03:03.4
94.03295 -31.69196 galactic Peg Second-epoch detections are separated by 0.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:03:27.64 +25:03:03.4 (user input) | T | P | (position from user input) J-Ks=0.460+/-0.034 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:27.64 +25:03:03.4: 14.06 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:27.64 +25:03:03.4: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 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,2461231.8417,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.23CV 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 10.3417 2461231.8417 13.37 23:04:43.53 +21:50:41.0
92.49768 -34.64379 galactic Peg Second-epoch detections are separated by 1.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:04:43.53 +21:50:41.0 (user input) | T | P | (position from user input) J-Ks=0.446+/-0.030 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:04:43.53 +21:50:41.0: 14.33 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:04:43.53 +21:50:41.0: 14.38 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8417,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.37CV 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 10.3417 2461231.8417 13.34 23:05:15.26 +19:57:04.7
91.49086 -36.35509 galactic Peg Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:05:15.26 +19:57:04.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.341+/-0.033 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:05:15.26 +19:57:04.7: 14.24 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:05:15.26 +19:57:04.7: 14.28 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8417,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.21 23:04:25.10 +21:33:07.2
92.24832 -34.86470 galactic Peg Second-epoch detections are separated by 1.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:04:25.10 +21:33:07.2 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.640+/-0.031 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:04:25.10 +21:33:07.2: 14.39 +/- 0.07 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:04:25.10 +21:33:07.2: 14.29 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8417,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.21CV 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 10.3417 2461231.8417 13.41 23:03:13.89 +23:23:48.0
93.04005 -33.11910 galactic Peg Second-epoch detections are separated by 2.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:03:13.89 +23:23:48.0 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.034 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:13.89 +23:23:48.0: 14.38 +/- 0.07 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:13.89 +23:23:48.0: 14.44 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8417,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.28 23:03:09.96 +22:10:44.5
92.31276 -34.17567 galactic Peg Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2841776969804223872 | 23:03:12.92 +22:10:47.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.590+/-0.029 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:09.96 +22:10:44.5: 14.22 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:09.96 +22:10:44.5: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.20 +/- 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
Gaia DR3 2841776969804223872,2461231.8417,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2841776969804223872 20260710.3417 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.18 23:00:47.14 +23:52:46.0
92.73724 -32.42482 galactic Peg Second-epoch detections are separated by 2.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:00:47.14 +23:52:46.0 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.333+/-0.033 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:00:47.14 +23:52:46.0: 14.09 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:00:47.14 +23:52:46.0: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 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,2461231.8417,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.39 23:02:25.74 +22:27:31.5
92.29891 -33.84831 galactic Peg Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:02:25.74 +22:27:31.5 (user input) | T | P | (position from user input) J-Ks=0.541+/-0.028 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:25.74 +22:27:31.5: 14.49 +/- 0.08 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:25.74 +22:27:31.5: 14.45 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8417,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.39CV 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 10.3417 2461231.8417 13.39 23:06:18.67 +22:10:44.1
93.08447 -34.52813 galactic Peg Second-epoch detections are separated by 1.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:06:18.67 +22:10:44.1 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.726+/-0.029 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:06:18.67 +22:10:44.1: 14.36 +/- 0.07 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:06:18.67 +22:10:44.1: 14.31 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8417,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.39CV 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 10.3417 2461231.8417 13.24 23:02:27.28 +23:29:46.0
92.91158 -32.94579 galactic Peg Second-epoch detections are separated by 1.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:02:27.28 +23:29:46.0 (user input) | T | P | (position from user input) J-Ks=0.221+/-0.033 (F)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:27.28 +23:29:46.0: 14.10 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:27.28 +23:29:46.0: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.12 +/- 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,2461231.8417,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.24CV 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 10.3417 2461231.8417 13.13 23:07:16.96 +21:43:02.1
93.05688 -35.04133 galactic Peg Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:07:16.96 +21:43:02.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.400+/-0.036 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:07:16.96 +21:43:02.1: 14.06 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:07:16.96 +21:43:02.1: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.04 +/- 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,2461231.8417,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.14 23:03:22.17 +23:20:04.8
93.03738 -33.18868 galactic Peg Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:03:22.17 +23:20:04.8 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.030 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:22.17 +23:20:04.8: 14.18 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:22.17 +23:20:04.8: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461231.8417,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.25 23:02:56.89 +20:25:02.9
91.19646 -35.68171 galactic Peg Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:02:56.89 +20:25:02.9 (user input) | T | P | (position from user input) J-Ks=0.588+/-0.030 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:56.89 +20:25:02.9: 14.20 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:56.89 +20:25:02.9: 14.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.19 +/- 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,2461231.8417,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.38 23:04:58.44 +21:44:38.7
92.49959 -34.75977 galactic Peg Second-epoch detections are separated by 0.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:04:58.44 +21:44:38.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.577+/-0.028 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:04:58.44 +21:44:38.7: 14.31 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:04:58.44 +21:44:38.7: 14.30 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.30 +/- 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,2461231.8417,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 12.79 23:05:43.11 +21:50:29.8
92.74112 -34.75802 galactic Peg Second-epoch detections are separated by 0.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:05:43.11 +21:50:29.8 (user input) | T | P | (position from user input) J-Ks=0.606+/-0.029 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:05:43.11 +21:50:29.8: 13.72 +/- 0.04 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:05:43.11 +21:50:29.8: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8417,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 12.93 23:02:59.63 +22:08:32.2
92.24899 -34.18818 galactic Peg Second-epoch detections are separated by 1.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:02:59.63 +22:08:32.2 (user input) | T | P | (position from user input) J-Ks=0.769+/-0.028 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:59.63 +22:08:32.2: 13.87 +/- 0.04 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:59.63 +22:08:32.2: 13.89 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.88 +/- 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,2461231.8417,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.14 23:02:43.21 +20:37:55.3
91.27132 -35.46916 galactic Peg Second-epoch detections are separated by 0.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:02:43.21 +20:37:55.3 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.499+/-0.030 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:43.21 +20:37:55.3: 14.06 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:43.21 +20:37:55.3: 14.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.07 +/- 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,2461231.8417,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.04 23:05:14.17 +22:05:38.2
92.77000 -34.48304 galactic Peg Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:05:14.17 +22:05:38.2 (user input) | T | P | (position from user input) J-Ks=0.616+/-0.028 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:05:14.17 +22:05:38.2: 14.01 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:05:14.17 +22:05:38.2: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 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,2461231.8417,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 12.79 23:04:47.02 +22:02:51.6
92.63154 -34.47286 galactic Peg Second-epoch detections are separated by 0.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:04:47.02 +22:02:51.6 (user input) | T | P | (position from user input) J-Ks=0.598+/-0.028 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:04:47.02 +22:02:51.6: 13.66 +/- 0.03 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:04:47.02 +22:02:51.6: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8417,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.24 23:03:34.13 +22:14:27.1
92.44760 -34.16728 galactic Peg Second-epoch detections are separated by 0.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:03:34.13 +22:14:27.1 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.736+/-0.030 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:34.13 +22:14:27.1: 14.16 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:34.13 +22:14:27.1: 14.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.18 +/- 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,2461231.8417,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.24CV 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 10.3417 2461231.8417 13.44 23:02:58.44 +22:11:17.4
92.27134 -34.14593 galactic Peg Second-epoch detections are separated by 1.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:02:58.44 +22:11:17.4 (user input) | T | P | (position from user input) J-Ks=0.513+/-0.030 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:58.44 +22:11:17.4: 14.61 +/- 0.08 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:58.44 +22:11:17.4: 14.46 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8417,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.22 23:06:16.77 +21:41:08.9
92.78880 -34.95730 galactic Peg Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:06:16.77 +21:41:08.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.431+/-0.029 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:06:16.77 +21:41:08.9: 14.17 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:06:16.77 +21:41:08.9: 14.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 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,2461231.8417,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.14 23:03:55.41 +19:52:00.6
91.10182 -36.27310 galactic Peg Second-epoch detections are separated by 0.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:03:55.41 +19:52:00.6 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.426+/-0.030 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:55.41 +19:52:00.6: 14.14 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:55.41 +19:52:00.6: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 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,2461231.8417,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 12.96 23:05:19.22 +21:56:37.3
92.70266 -34.62404 galactic Peg Second-epoch detections are separated by 0.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:05:19.22 +21:56:37.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.498+/-0.032 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:05:19.22 +21:56:37.3: 13.97 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:05:19.22 +21:56:37.3: 13.89 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461231.8417,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.11 23:04:24.35 +23:44:47.2
93.52196 -32.94158 galactic Peg Second-epoch detections are separated by 0.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:04:24.35 +23:44:47.2 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.033 (G)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:04:24.35 +23:44:47.2: 14.15 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:04:24.35 +23:44:47.2: 14.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.13 +/- 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,2461231.8417,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3417 2461231.8417 13.24 23:02:44.31 +23:25:20.8
92.93682 -33.04179 galactic Peg Second-epoch detections are separated by 1.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:02:44.31 +23:25:20.8 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.494+/-0.028 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:44.31 +23:25:20.8: 14.29 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:44.31 +23:25:20.8: 14.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.18 +/- 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,2461231.8417,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.24CV 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 10.3417 2461231.8417 13.30 23:00:53.54 +20:36:05.1
90.79894 -35.28074 galactic Peg Second-epoch detections are separated by 1.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:00:53.54 +20:36:05.1 (user input) | T | P | (position from user input) J-Ks=0.691+/-0.031 (K)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:00:53.54 +20:36:05.1: 14.27 +/- 0.07 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:00:53.54 +20:36:05.1: 14.24 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8417,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3417 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.61327655 23.12.2025 02:42:57.094 /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
First image: 2461032.61327655 23.12.2025 02:42:57.094 /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
Last image: 2461231.84201559 10.07.2026 08:12:20.147 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
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: 4 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): 8090
Objects passed selection criteria: 8050
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 5346.5
Average stars matched: 5020 (93.8932 %)
Memory usage VmPeak: 114284 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 07:24:31 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.61327655 23.12.2025 02:42:57.094 /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
First image: 2461032.61327655 23.12.2025 02:42:57.094 /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
Last image: 2461231.84201559 10.07.2026 08:12:20.147 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 61
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 14 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): 51629
Objects passed selection criteria: 51498
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 36719.8
Average stars matched: 34063.2 (92.7655 %)
Memory usage VmPeak: 153556 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 07:26:23 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
SExtractor catalog cache: saved Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.cat to cache
SExtractor catalog cache: saved Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.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: 2461231.84145509
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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits exists and is non-empty
Saving wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits to local_wcs_cache/
'wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits' -> 'local_wcs_cache/wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits'
wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits exists and is non-empty
Saving wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits to local_wcs_cache/
'wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits' -> 'local_wcs_cache/wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits'
wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits exists and is non-empty
Saving wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits to local_wcs_cache/
'wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits' -> 'local_wcs_cache/wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits'
wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits exists and is non-empty
Saving wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits to local_wcs_cache/
'wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits' -> 'local_wcs_cache/wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits (1st reference image)
verification OK: wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
Image size: 941.5'x626.9' 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: 23:04:37.578 +22:00:09.14 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits (1st new image)
verification OK: wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.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: 23:04:17.204 +22:01:02.87 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:04:37.578 +22:00:09.14
Second-epoch image center 23:04:17.204 +22:01:02.87
Angular distance between the image centers 0.0801 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits (2nd new image)
verification OK: wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.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: 23:04:15.053 +22:00:39.66 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:04:37.578 +22:00:09.14
Second-epoch image center 23:04:15.053 +22:00:39.66
Angular distance between the image centers 0.0874 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:04:17.204 +22:01:02.87
Second-epoch second image center 23:04:15.053 +22:00:39.66
Angular distance between the image centers 0.01052 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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits &> /tmp/tmp.C4R2X7aKZ8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits &> /tmp/tmp.J2uVNDI9eq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits &> /tmp/tmp.Lkb0fntMVd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits &> /tmp/tmp.RNdsIRdU1o
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat
Found non-empty wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat
The reference image (wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits) and catalog (wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat) found
'wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat' -> 'wcsmag.cat'
Read 11180 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 337.4433 to 355.0144 deg, Dec +16.4804 to +27.2996 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 337.4433 to 355.0144 deg, Dec 16.4804 to 27.2996 deg
Loaded 7944 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): 6126 out of 6477 total matches.
Matched with Tycho-2 6477 out of 11180 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.921600
a=0.000000 b=1.000000 c=22.921600
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 11180 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 337.4433 to 355.0144 deg, Dec +16.4804 to +27.2996 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 337.4433 to 355.0144 deg, Dec 16.4804 to 27.2996 deg
Loaded 7944 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): 6126 out of 6477 total matches.
Matched with Tycho-2 6477 out of 11180 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits:
Forced-photometry filter: calibrated wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits -> calib.txt_param_ref_wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits (aperture=6.2)
Read 11099 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 337.4397 to 355.0144 deg, Dec +16.4823 to +27.2996 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 337.4397 to 355.0144 deg, Dec 16.4823 to 27.2996 deg
Loaded 7946 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): 6122 out of 6472 total matches.
Matched with Tycho-2 6472 out of 11099 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits:
Forced-photometry filter: calibrated wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits -> calib.txt_param_ref_wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
2.2 pix Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
2.2 pix fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
2.3 pix fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
2.2 pix wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
2.2 pix wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
Limiting magnitude estimates:
15.3 mag. Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
15.3 mag. Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
13.5 mag. fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
13.4 mag. fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 11.0 (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.C4R2X7aKZ8 (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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits' -> 'wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
Checking if the catalog wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat corresponding to the image wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat corresponding to the image wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
WCS catalog name: wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=789, bad_region=3238, passed=11180
Got 11180 stars (including 7346 good ones) from the SExtractor catalog wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat
util/solve_plate_with_UCAC5 got 11180 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 8270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 8270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 8270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits N_match=980 sigma_overall_arcsec=0.320 sigma_q1_arcsec=0.381 sigma_q2_arcsec=0.316 sigma_q3_arcsec=0.312 sigma_q4_arcsec=0.204 n_q1=291 n_q2=216 n_q3=264 n_q4=209 worst_quadrant_to_overall_ratio=1.191
The image catalog is written to wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits -region wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.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.J2uVNDI9eq (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-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.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-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.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-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits' -> 'wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
Checking if the catalog wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat corresponding to the image wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat corresponding to the image wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
WCS catalog name: wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=786, bad_region=3189, passed=11099
Got 11099 stars (including 7305 good ones) from the SExtractor catalog wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat
util/solve_plate_with_UCAC5 got 11099 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 8227 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 8228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 8228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits N_match=980 sigma_overall_arcsec=0.344 sigma_q1_arcsec=0.406 sigma_q2_arcsec=0.365 sigma_q3_arcsec=0.325 sigma_q4_arcsec=0.267 n_q1=289 n_q2=216 n_q3=266 n_q4=209 worst_quadrant_to_overall_ratio=1.180
The image catalog is written to wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits -region wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.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.Lkb0fntMVd (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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
WCS_IMAGE_NAME=wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
WCS-calibrated image found: wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
Checking if the catalog wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat corresponding to the image wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat corresponding to the image wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
WCS catalog name: wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=165, bad_region=823, passed=3660
Got 3660 stars (including 2703 good ones) from the SExtractor catalog wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat
util/solve_plate_with_UCAC5 got 3660 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 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 2933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 2932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 2932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits N_match=975 sigma_overall_arcsec=0.424 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.468 sigma_q3_arcsec=0.512 sigma_q4_arcsec=0.425 n_q1=328 n_q2=180 n_q3=270 n_q4=197 worst_quadrant_to_overall_ratio=1.206
The image catalog is written to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits -region wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.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.RNdsIRdU1o (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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
WCS_IMAGE_NAME=wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
WCS-calibrated image found: wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
Checking if the catalog wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat corresponding to the image wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat corresponding to the image wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
WCS catalog name: wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=164, bad_region=821, passed=3653
Got 3653 stars (including 2699 good ones) from the SExtractor catalog wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat
util/solve_plate_with_UCAC5 got 3653 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 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 2907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 2907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 2907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits N_match=973 sigma_overall_arcsec=0.414 sigma_q1_arcsec=0.361 sigma_q2_arcsec=0.397 sigma_q3_arcsec=0.432 sigma_q4_arcsec=0.427 n_q1=292 n_q2=176 n_q3=307 n_q4=198 worst_quadrant_to_overall_ratio=1.042
The image catalog is written to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits -region wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits sigma_overall=0.320 worst_q_ratio=1.191
ref2=Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits sigma_overall=0.344 worst_q_ratio=1.180
new1=fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits sigma_overall=0.424 worst_q_ratio=1.206
new2=fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits sigma_overall=0.414 worst_q_ratio=1.042
reference average sigma_overall=0.332 worst_q_ratio=1.1855
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065_astrometric_residuals.png (980 matched stars from wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066_astrometric_residuals.png (980 matched stars from wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336_astrometric_residuals.png (975 matched stars from wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337_astrometric_residuals.png (973 matched stars from wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits'
Saving fully-calibrated image wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits'
Preparing the HTML report for the field Peg-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Peg-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
SExtractor catalog cache: saved Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.cat to cache
SExtractor catalog cache: saved Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
Creating symlink local_wcs_cache/wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits exists and is non-empty
wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits exists and is non-empty
wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits exists and is non-empty
wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits (1st reference image)
verification OK: wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
Image size: 941.5'x626.9' 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: 23:04:37.578 +22:00:09.14 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits (1st new image)
verification OK: wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.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: 23:04:17.204 +22:01:02.87 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:04:37.578 +22:00:09.14
Second-epoch image center 23:04:17.204 +22:01:02.87
Angular distance between the image centers 0.0801 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits (2nd new image)
verification OK: wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.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: 23:04:15.053 +22:00:39.66 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:04:37.578 +22:00:09.14
Second-epoch image center 23:04:15.053 +22:00:39.66
Angular distance between the image centers 0.0874 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:04:17.204 +22:01:02.87
Second-epoch second image center 23:04:15.053 +22:00:39.66
Angular distance between the image centers 0.01052 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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits &> /tmp/tmp.KAFB4aFif4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits &> /tmp/tmp.7yLXYRHBe5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits &> /tmp/tmp.xiJpnXSRRw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits &> /tmp/tmp.MlT1dyNqgm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat
Found non-empty wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat
The reference image (wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits) and catalog (wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat) found
'wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat' -> 'wcsmag.cat'
Read 66918 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 337.4316 to 355.0267 deg, Dec +16.4729 to +27.3027 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 337.4316 to 355.0267 deg, Dec 16.4729 to 27.3027 deg
Loaded 7961 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): 5640 out of 6577 total matches.
Matched with Tycho-2 6577 out of 66918 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.796300
a=0.000000 b=1.000000 c=22.796300
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 66918 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 337.4316 to 355.0267 deg, Dec +16.4729 to +27.3027 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 337.4316 to 355.0267 deg, Dec 16.4729 to 27.3027 deg
Loaded 7961 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): 5640 out of 6577 total matches.
Matched with Tycho-2 6577 out of 66918 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits:
Forced-photometry filter: calibrated wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits -> calib.txt_param_ref_wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits (aperture=4.8)
Read 67805 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 337.4316 to 355.0266 deg, Dec +16.4730 to +27.3052 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 337.4316 to 355.0266 deg, Dec 16.4730 to 27.3052 deg
Loaded 7963 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): 5624 out of 6580 total matches.
Matched with Tycho-2 6580 out of 67805 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits:
Forced-photometry filter: calibrated wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits -> calib.txt_param_ref_wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
2.1 pix Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
2.1 pix fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
2.1 pix fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
2.1 pix wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
2.1 pix wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
Limiting magnitude estimates:
15.5 mag. Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
15.5 mag. Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
13.8 mag. fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
13.7 mag. fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.KAFB4aFif4 (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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.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-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits' -> 'wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
Checking if the catalog wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat corresponding to the image wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat corresponding to the image wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits
WCS catalog name: wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=4068, bad_region=15852, passed=66904
Got 66904 stars (including 48004 good ones) from the SExtractor catalog wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat
util/solve_plate_with_UCAC5 got 66904 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 52823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 52824 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 52824 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits N_match=980 sigma_overall_arcsec=0.335 sigma_q1_arcsec=0.394 sigma_q2_arcsec=0.338 sigma_q3_arcsec=0.325 sigma_q4_arcsec=0.243 n_q1=291 n_q2=209 n_q3=275 n_q4=205 worst_quadrant_to_overall_ratio=1.175
The image catalog is written to wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits -region wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.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.7yLXYRHBe5 (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-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.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-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.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-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits' -> 'wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
Checking if the catalog wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat corresponding to the image wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat corresponding to the image wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits
WCS catalog name: wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=4112, bad_region=16057, passed=67795
Got 67795 stars (including 48617 good ones) from the SExtractor catalog wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat
util/solve_plate_with_UCAC5 got 67795 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 53431 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 53430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 53430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits N_match=979 sigma_overall_arcsec=0.365 sigma_q1_arcsec=0.415 sigma_q2_arcsec=0.355 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.275 n_q1=292 n_q2=208 n_q3=277 n_q4=202 worst_quadrant_to_overall_ratio=1.138
The image catalog is written to wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits -region wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.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.xiJpnXSRRw (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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
WCS_IMAGE_NAME=wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
WCS-calibrated image found: wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
Checking if the catalog wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat corresponding to the image wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat corresponding to the image wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
WCS catalog name: wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=774, bad_region=4662, passed=27430
Got 27430 stars (including 22117 good ones) from the SExtractor catalog wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat
util/solve_plate_with_UCAC5 got 27430 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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 23318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 23319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 23319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits N_match=976 sigma_overall_arcsec=0.430 sigma_q1_arcsec=0.344 sigma_q2_arcsec=0.488 sigma_q3_arcsec=0.523 sigma_q4_arcsec=0.416 n_q1=331 n_q2=187 n_q3=256 n_q4=202 worst_quadrant_to_overall_ratio=1.217
The image catalog is written to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits -region wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.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.MlT1dyNqgm (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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
WCS_IMAGE_NAME=wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
WCS-calibrated image found: wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
Checking if the catalog wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat corresponding to the image wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat corresponding to the image wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
WCS catalog name: wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=745, bad_region=4656, passed=26913
Got 26913 stars (including 21618 good ones) from the SExtractor catalog wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat
util/solve_plate_with_UCAC5 got 26913 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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 22733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 22733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 22733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits N_match=974 sigma_overall_arcsec=0.419 sigma_q1_arcsec=0.380 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.434 sigma_q4_arcsec=0.442 n_q1=299 n_q2=180 n_q3=294 n_q4=201 worst_quadrant_to_overall_ratio=1.055
The image catalog is written to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits -region wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.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-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-11-31_20.00sec_4.90C_LIGHT_0336.fits
Saving fully-calibrated image wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.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-06-Q2b1x1_035859_TTUQ2b1x1_2641946_gI3P2cMT/wcs_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337.fits
Preparing the HTML report for the field Peg-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:16:27.88 +26:15:29.1: 13.43 +/- 0.03 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:11.43 +20:54:19.4: 13.74 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 22:47:58.54 +18:33:51.4: 13.31 +/- 0.03 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:05:30.74 +20:13:52.3: 13.32 +/- 0.04 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 22:59:46.10 +20:36:40.7: 14.03 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:10:55.61 +21:40:12.8: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:22:30.03 +21:25:28.0: 13.65 +/- 0.04 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:16:27.88 +26:15:29.1: 13.42 +/- 0.03 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 22:47:58.54 +18:33:51.4: 13.27 +/- 0.03 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:05:30.74 +20:13:52.3: 13.34 +/- 0.03 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:11.43 +20:54:19.4: 13.75 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter REJECTED candidate at 23:16:27.88 +26:15:29.1: ref_mag=13.43 +/- 0.02 new_mean_mag=13.2306 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry reference-image weighted average: 13.75 +/- 0.05
Forced photometry filter REJECTED candidate at 22:47:58.54 +18:33:51.4: ref_mag=13.29 +/- 0.02 new_mean_mag=13.0654 delta=0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:05:30.74 +20:13:52.3: ref_mag=13.33 +/- 0.02 new_mean_mag=12.7390 delta=0.59 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:03:11.43 +20:54:19.4: ref_mag=13.75 +/- 0.05 new_mean_mag=12.9360 delta=0.81 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:01:26.85 +21:13:24.1: 14.13 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:34.54 +21:47:11.4: 14.46 +/- 0.07 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:10:55.61 +21:40:12.8: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 22:59:46.10 +20:36:40.7: 14.03 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:22:30.03 +21:25:28.0: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.04
Forced photometry filter REJECTED candidate at 22:59:46.10 +20:36:40.7: ref_mag=14.03 +/- 0.04 new_mean_mag=13.3329 delta=0.70 (need > 0.90)
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter REJECTED candidate at 23:22:30.03 +21:25:28.0: ref_mag=13.68 +/- 0.03 new_mean_mag=13.3349 delta=0.35 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:06:12.24 +21:32:16.1: 13.98 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:01:26.85 +21:13:24.1: 14.08 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:34.54 +21:47:11.4: 14.35 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Forced photometry filter KEPT candidate at 23:01:26.85 +21:13:24.1: ref_mag=14.10 +/- 0.04 new_mean_mag=13.1671 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 14.40 +/- 0.05
Forced photometry filter KEPT candidate at 23:02:34.54 +21:47:11.4: ref_mag=14.40 +/- 0.05 new_mean_mag=13.3537 delta=1.05 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:06:12.24 +21:32:16.1: 14.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.03
Forced photometry filter KEPT candidate at 23:06:12.24 +21:32:16.1: ref_mag=14.02 +/- 0.03 new_mean_mag=13.1075 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:06:59.27 +22:06:38.1: 14.00 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:27.64 +25:03:03.4: 14.06 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:55.48 +23:47:03.9: 13.86 +/- 0.04 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:01:04.25 +23:58:52.6: 13.88 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:04:43.53 +21:50:41.0: 14.33 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:06:59.27 +22:06:38.1: 14.12 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:55.48 +23:47:03.9: 13.94 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:27.64 +25:03:03.4: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.04
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Forced photometry filter KEPT candidate at 23:06:59.27 +22:06:38.1: ref_mag=14.05 +/- 0.04 new_mean_mag=13.0876 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 23:03:55.48 +23:47:03.9: ref_mag=13.89 +/- 0.03 new_mean_mag=12.9692 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Forced photometry filter KEPT candidate at 23:03:27.64 +25:03:03.4: ref_mag=14.10 +/- 0.04 new_mean_mag=13.1892 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:01:04.25 +23:58:52.6: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Forced photometry filter REJECTED candidate at 23:01:04.25 +23:58:52.6: ref_mag=13.95 +/- 0.04 new_mean_mag=13.1773 delta=0.77 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:04:43.53 +21:50:41.0: 14.38 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.05
Forced photometry filter KEPT candidate at 23:04:43.53 +21:50:41.0: ref_mag=14.35 +/- 0.05 new_mean_mag=13.3639 delta=0.99 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:05:15.26 +19:57:04.7: 14.24 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:05:15.26 +19:57:04.7: 14.28 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.04
Forced photometry filter KEPT candidate at 23:05:15.26 +19:57:04.7: ref_mag=14.26 +/- 0.04 new_mean_mag=13.2788 delta=0.98 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:04:25.10 +21:33:07.2: 14.39 +/- 0.07 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:04:25.10 +21:33:07.2: 14.29 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.05
Forced photometry filter KEPT candidate at 23:04:25.10 +21:33:07.2: ref_mag=14.34 +/- 0.05 new_mean_mag=13.2156 delta=1.12 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:13.89 +23:23:48.0: 14.38 +/- 0.07 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:13.89 +23:23:48.0: 14.44 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.05
Forced photometry filter KEPT candidate at 23:03:13.89 +23:23:48.0: ref_mag=14.41 +/- 0.05 new_mean_mag=13.4136 delta=0.99 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:09.96 +22:10:44.5: 14.22 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:00:47.14 +23:52:46.0: 14.09 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:09.96 +22:10:44.5: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.04
Forced photometry filter KEPT candidate at 23:03:09.96 +22:10:44.5: ref_mag=14.20 +/- 0.04 new_mean_mag=13.2713 delta=0.93 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:00:47.14 +23:52:46.0: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.04
Forced photometry filter KEPT candidate at 23:00:47.14 +23:52:46.0: ref_mag=14.13 +/- 0.04 new_mean_mag=13.1183 delta=1.01 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:25.74 +22:27:31.5: 14.49 +/- 0.08 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:25.74 +22:27:31.5: 14.45 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.05
Forced photometry filter KEPT candidate at 23:02:25.74 +22:27:31.5: ref_mag=14.47 +/- 0.05 new_mean_mag=13.3915 delta=1.08 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:06:18.67 +22:10:44.1: 14.36 +/- 0.07 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:27.28 +23:29:46.0: 14.10 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:07:16.96 +21:43:02.1: 14.06 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:22.17 +23:20:04.8: 14.18 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:06:18.67 +22:10:44.1: 14.31 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:27.28 +23:29:46.0: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.05
Forced photometry filter KEPT candidate at 23:06:18.67 +22:10:44.1: ref_mag=14.33 +/- 0.05 new_mean_mag=13.3800 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 14.12 +/- 0.04
Forced photometry filter KEPT candidate at 23:02:27.28 +23:29:46.0: ref_mag=14.12 +/- 0.04 new_mean_mag=13.1650 delta=0.95 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:22.17 +23:20:04.8: 14.03 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:07:16.96 +21:43:02.1: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.04
Forced photometry reference-image weighted average: 14.04 +/- 0.04
Forced photometry filter KEPT candidate at 23:03:22.17 +23:20:04.8: ref_mag=14.09 +/- 0.04 new_mean_mag=13.1207 delta=0.97 (need > 0.90)
Forced photometry filter KEPT candidate at 23:07:16.96 +21:43:02.1: ref_mag=14.04 +/- 0.04 new_mean_mag=13.1377 delta=0.90 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:56.89 +20:25:02.9: 14.20 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:56.89 +20:25:02.9: 14.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.04
Forced photometry filter KEPT candidate at 23:02:56.89 +20:25:02.9: ref_mag=14.19 +/- 0.04 new_mean_mag=13.2133 delta=0.98 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:04:58.44 +21:44:38.7: 14.31 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:04:58.44 +21:44:38.7: 14.30 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.04
Forced photometry filter KEPT candidate at 23:04:58.44 +21:44:38.7: ref_mag=14.30 +/- 0.04 new_mean_mag=13.3662 delta=0.94 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:05:43.11 +21:50:29.8: 13.72 +/- 0.04 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:05:43.11 +21:50:29.8: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Forced photometry filter KEPT candidate at 23:05:43.11 +21:50:29.8: ref_mag=13.74 +/- 0.03 new_mean_mag=12.7780 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:59.63 +22:08:32.2: 13.87 +/- 0.04 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:43.21 +20:37:55.3: 14.06 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:59.63 +22:08:32.2: 13.89 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.03
Forced photometry filter KEPT candidate at 23:02:59.63 +22:08:32.2: ref_mag=13.88 +/- 0.03 new_mean_mag=12.9265 delta=0.95 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:43.21 +20:37:55.3: 14.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.04
Forced photometry filter KEPT candidate at 23:02:43.21 +20:37:55.3: ref_mag=14.07 +/- 0.04 new_mean_mag=13.1370 delta=0.94 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:05:14.17 +22:05:38.2: 14.01 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:05:14.17 +22:05:38.2: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.03
Forced photometry filter KEPT candidate at 23:05:14.17 +22:05:38.2: ref_mag=14.01 +/- 0.03 new_mean_mag=13.0380 delta=0.98 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:04:47.02 +22:02:51.6: 13.66 +/- 0.03 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:04:47.02 +22:02:51.6: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.02
Forced photometry filter KEPT candidate at 23:04:47.02 +22:02:51.6: ref_mag=13.70 +/- 0.02 new_mean_mag=12.7879 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:34.13 +22:14:27.1: 14.16 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:58.44 +22:11:17.4: 14.61 +/- 0.08 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:34.13 +22:14:27.1: 14.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.04
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:58.44 +22:11:17.4: 14.46 +/- 0.07 detection
Forced photometry filter KEPT candidate at 23:03:34.13 +22:14:27.1: ref_mag=14.18 +/- 0.04 new_mean_mag=13.2325 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 14.53 +/- 0.05
Forced photometry filter KEPT candidate at 23:02:58.44 +22:11:17.4: ref_mag=14.53 +/- 0.05 new_mean_mag=13.4061 delta=1.13 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:06:16.77 +21:41:08.9: 14.17 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:03:55.41 +19:52:00.6: 14.14 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:06:16.77 +21:41:08.9: 14.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.04
Forced photometry filter KEPT candidate at 23:06:16.77 +21:41:08.9: ref_mag=14.18 +/- 0.04 new_mean_mag=13.2027 delta=0.98 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:01:43.63 +23:55:03.6: 14.12 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:03:55.41 +19:52:00.6: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.04
Forced photometry filter KEPT candidate at 23:03:55.41 +19:52:00.6: ref_mag=14.06 +/- 0.04 new_mean_mag=13.0872 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:01:43.63 +23:55:03.6: 14.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.04
Forced photometry filter REJECTED candidate at 23:01:43.63 +23:55:03.6: ref_mag=14.09 +/- 0.04 new_mean_mag=13.2042 delta=0.89 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:05:19.22 +21:56:37.3: 13.97 +/- 0.05 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:04:24.35 +23:44:47.2: 14.15 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:05:19.22 +21:56:37.3: 13.89 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.03
Forced photometry filter KEPT candidate at 23:05:19.22 +21:56:37.3: ref_mag=13.92 +/- 0.03 new_mean_mag=12.9652 delta=0.96 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:04:24.35 +23:44:47.2: 14.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.04
Forced photometry filter KEPT candidate at 23:04:24.35 +23:44:47.2: ref_mag=14.13 +/- 0.04 new_mean_mag=13.0972 delta=1.03 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:02:44.31 +23:25:20.8: 14.29 +/- 0.06 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:00:21.34 +24:09:40.6: 13.43 +/- 0.03 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:02:44.31 +23:25:20.8: 14.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.04
Forced photometry filter KEPT candidate at 23:02:44.31 +23:25:20.8: ref_mag=14.18 +/- 0.04 new_mean_mag=13.2374 delta=0.95 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:00:21.34 +24:09:40.6: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter REJECTED candidate at 23:00:21.34 +24:09:40.6: ref_mag=13.42 +/- 0.02 new_mean_mag=12.8753 delta=0.54 (need > 0.90)
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-42-57_20.00sec_-15.00C_LIGHT_0065.fits at 23:00:53.54 +20:36:05.1: 14.27 +/- 0.07 detection
Forced photometry on wcs_Peg-06-Q2b1x1_2025-12-22_20-43-41_20.00sec_-14.90C_LIGHT_0066.fits at 23:00:53.54 +20:36:05.1: 14.24 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.05
Forced photometry filter KEPT candidate at 23:00:53.54 +20:36:05.1: ref_mag=14.25 +/- 0.05 new_mean_mag=13.2630 delta=0.99 (need > 0.90)
Adding exclusion_list_local.txt__out15997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86122.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 56s
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 80985_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 80985_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
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Considering the candidate 80986_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 80986_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
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Considering the candidate 80987_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 80987_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
**** FOUND 23:04:25.17 +20:44:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82109_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 82109_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
**** FOUND 23:21:42.15 +20:37:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83589_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 83589_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
**** FOUND 22:50:53.73 +17:59:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83630_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 83630_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
**** FOUND 23:06:15.75 +18:29:45.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 83674_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 83674_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
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Considering the candidate 83779_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 83779_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
**** FOUND 23:03:13.13 +20:54:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84430_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 84430_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
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Considering the candidate 84536_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 84536_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
**** FOUND 22:54:03.03 +19:52:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84709_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 84709_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
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Considering the candidate 84715_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 84715_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
**** FOUND 23:16:28.88 +26:12:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85441_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 85441_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
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Considering the candidate 86122_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 86122_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 41414_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 41414_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 37961_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 37961_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 39375_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 39375_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 47553_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 47553_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
**** FOUND 22:52:09.80 +17:49:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35728_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 35728_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 24618_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 24618_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 15997_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 15997_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 37487_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 37487_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 77126_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 77126_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
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Considering the candidate 47947_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 47947_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
**** FOUND 22:50:24.94 +17:53:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62598_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 62598_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 39394_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 39394_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 27403_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 27403_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 35356_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 35356_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 24059_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 24059_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 33630_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 33630_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 35307_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 35307_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 26659_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 26659_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 38253_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 38253_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 27814_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 27814_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 65723_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 65723_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 38152_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 38152_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 37452_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 37452_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 35610_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 35610_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 59887_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 59887_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 35871_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 35871_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 36174_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 36174_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 35013_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 35013_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 35326_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 35326_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 38502_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 38502_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 61943_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 61943_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 23749_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 23749_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
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Considering the candidate 36812_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 36812_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 24924_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 24924_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 27232_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 27232_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
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Considering the candidate 22117_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 22117_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
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Considering the candidate 33658_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
The candidate 33658_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337 did not pass the final checks
**** FOUND 23:00:03.49 +22:27:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66570_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
Preparing report for the candidate 66570_fd_Peg-06-Q2b1x1_2026-07-10_03-12-20_20.00sec_5.00C_LIGHT_0337
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 74s
Prepared the HTML report for the field Peg-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:03:27.64 +25:03:03.4
23:00:47.14 +23:52:46.0
23:03:55.48 +23:47:03.9
23:04:24.35 +23:44:47.2
23:02:27.28 +23:29:46.0
23:02:44.31 +23:25:20.8
23:03:13.89 +23:23:48.0
23:03:22.17 +23:20:04.8
23:02:25.74 +22:27:31.5
23:03:34.13 +22:14:27.1
23:06:18.67 +22:10:44.1
23:02:58.44 +22:11:17.4
23:03:09.96 +22:10:44.5
23:02:59.63 +22:08:32.2
23:06:59.27 +22:06:38.1
23:05:14.17 +22:05:38.2
23:04:47.02 +22:02:51.6
23:05:19.22 +21:56:37.3
23:05:43.11 +21:50:29.8
23:04:43.53 +21:50:41.0
23:02:34.54 +21:47:11.4
23:04:58.44 +21:44:38.7
23:07:16.96 +21:43:02.1
23:06:16.77 +21:41:08.9
23:06:12.24 +21:32:16.1
23:04:25.10 +21:33:07.2
23:01:26.85 +21:13:24.1
23:02:43.21 +20:37:55.3
23:03:55.41 +19:52:00.6
23:05:15.26 +19:57:04.7
23:02:56.89 +20:25:02.9
23:00:53.54 +20:36:05.1
23:10:55.61 +21:40:12.8
########### Completed Peg-06-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
23:10:55.61 +21:40:12.8
23:01:26.85 +21:13:24.1
23:02:34.54 +21:47:11.4
23:06:12.24 +21:32:16.1
23:06:59.27 +22:06:38.1
23:03:55.48 +23:47:03.9
23:03:27.64 +25:03:03.4
23:04:43.53 +21:50:41.0
23:05:15.26 +19:57:04.7
23:04:25.10 +21:33:07.2
23:03:13.89 +23:23:48.0
23:03:09.96 +22:10:44.5
23:00:47.14 +23:52:46.0
23:02:25.74 +22:27:31.5
23:06:18.67 +22:10:44.1
23:02:27.28 +23:29:46.0
23:07:16.96 +21:43:02.1
23:03:22.17 +23:20:04.8
23:02:56.89 +20:25:02.9
23:04:58.44 +21:44:38.7
23:05:43.11 +21:50:29.8
23:02:59.63 +22:08:32.2
23:02:43.21 +20:37:55.3
23:05:14.17 +22:05:38.2
23:04:47.02 +22:02:51.6
23:03:34.13 +22:14:27.1
23:02:58.44 +22:11:17.4
23:06:16.77 +21:41:08.9
23:03:55.41 +19:52:00.6
23:05:19.22 +21:56:37.3
23:04:24.35 +23:44:47.2
23:02:44.31 +23:25:20.8
23:00:53.54 +20:36:05.1
###################################################################################
23:10:55.61 +21:40:12.8 -- asteroid (will NOT add it to exclusion list)
23:01:26.85 +21:13:24.1 -- not an asteroid (will add it to exclusion list)
23:02:34.54 +21:47:11.4 -- not an asteroid (will add it to exclusion list)
23:06:12.24 +21:32:16.1 -- not an asteroid (will add it to exclusion list)
23:06:59.27 +22:06:38.1 -- not an asteroid (will add it to exclusion list)
23:03:55.48 +23:47:03.9 -- not an asteroid (will add it to exclusion list)
23:03:27.64 +25:03:03.4 -- not an asteroid (will add it to exclusion list)
23:04:43.53 +21:50:41.0 -- not an asteroid (will add it to exclusion list)
23:05:15.26 +19:57:04.7 -- not an asteroid (will add it to exclusion list)
23:04:25.10 +21:33:07.2 -- not an asteroid (will add it to exclusion list)
23:03:13.89 +23:23:48.0 -- not an asteroid (will add it to exclusion list)
23:03:09.96 +22:10:44.5 -- not an asteroid (will add it to exclusion list)
23:00:47.14 +23:52:46.0 -- not an asteroid (will add it to exclusion list)
23:02:25.74 +22:27:31.5 -- not an asteroid (will add it to exclusion list)
23:06:18.67 +22:10:44.1 -- not an asteroid (will add it to exclusion list)
23:02:27.28 +23:29:46.0 -- not an asteroid (will add it to exclusion list)
23:07:16.96 +21:43:02.1 -- not an asteroid (will add it to exclusion list)
23:03:22.17 +23:20:04.8 -- not an asteroid (will add it to exclusion list)
23:02:56.89 +20:25:02.9 -- not an asteroid (will add it to exclusion list)
23:04:58.44 +21:44:38.7 -- not an asteroid (will add it to exclusion list)
23:05:43.11 +21:50:29.8 -- not an asteroid (will add it to exclusion list)
23:02:59.63 +22:08:32.2 -- not an asteroid (will add it to exclusion list)
23:02:43.21 +20:37:55.3 -- not an asteroid (will add it to exclusion list)
23:05:14.17 +22:05:38.2 -- not an asteroid (will add it to exclusion list)
23:04:47.02 +22:02:51.6 -- not an asteroid (will add it to exclusion list)
23:03:34.13 +22:14:27.1 -- not an asteroid (will add it to exclusion list)
23:02:58.44 +22:11:17.4 -- not an asteroid (will add it to exclusion list)
23:06:16.77 +21:41:08.9 -- not an asteroid (will add it to exclusion list)
23:03:55.41 +19:52:00.6 -- not an asteroid (will add it to exclusion list)
23:05:19.22 +21:56:37.3 -- not an asteroid (will add it to exclusion list)
23:04:24.35 +23:44:47.2 -- not an asteroid (will add it to exclusion list)
23:02:44.31 +23:25:20.8 -- not an asteroid (will add it to exclusion list)
23:00:53.54 +20:36:05.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
23:00:47.14 +23:52:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:53.54 +20:36:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:26.85 +21:13:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:25.74 +22:27:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:27.28 +23:29:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:34.54 +21:47:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:43.21 +20:37:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:44.31 +23:25:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:56.89 +20:25:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:58.44 +22:11:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:59.63 +22:08:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:09.96 +22:10:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:13.89 +23:23:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:22.17 +23:20:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:27.64 +25:03:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:34.13 +22:14:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:55.41 +19:52:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:55.48 +23:47:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:24.35 +23:44:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:25.10 +21:33:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:43.53 +21:50:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:47.02 +22:02:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:58.44 +21:44:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:14.17 +22:05:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:15.26 +19:57:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:19.22 +21:56:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:43.11 +21:50:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:12.24 +21:32:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:16.77 +21:41:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:18.67 +22:10:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:59.27 +22:06:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:16.96 +21:43:02.1 -- 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)
23:00:47.14 +23:52:46.0 -- not a known variable star
23:00:53.54 +20:36:05.1 -- not a known variable star
23:01:26.85 +21:13:24.1 -- not a known variable star
23:02:25.74 +22:27:31.5 -- not a known variable star
23:02:27.28 +23:29:46.0 -- not a known variable star
23:02:34.54 +21:47:11.4 -- not a known variable star
23:02:43.21 +20:37:55.3 -- not a known variable star
23:02:44.31 +23:25:20.8 -- not a known variable star
23:02:56.89 +20:25:02.9 -- not a known variable star
23:02:58.44 +22:11:17.4 -- not a known variable star
23:02:59.63 +22:08:32.2 -- not a known variable star
23:03:09.96 +22:10:44.5 -- not a known variable star
23:03:13.89 +23:23:48.0 -- not a known variable star
23:03:22.17 +23:20:04.8 -- not a known variable star
23:03:27.64 +25:03:03.4 -- not a known variable star
23:03:34.13 +22:14:27.1 -- not a known variable star
23:03:55.41 +19:52:00.6 -- not a known variable star
23:03:55.48 +23:47:03.9 -- not a known variable star
23:04:24.35 +23:44:47.2 -- not a known variable star
23:04:25.10 +21:33:07.2 -- not a known variable star
23:04:43.53 +21:50:41.0 -- not a known variable star
23:04:47.02 +22:02:51.6 -- not a known variable star
23:04:58.44 +21:44:38.7 -- not a known variable star
23:05:14.17 +22:05:38.2 -- not a known variable star
23:05:15.26 +19:57:04.7 -- not a known variable star
23:05:19.22 +21:56:37.3 -- not a known variable star
23:05:43.11 +21:50:29.8 -- not a known variable star
23:06:12.24 +21:32:16.1 -- not a known variable star
23:06:16.77 +21:41:08.9 -- not a known variable star
23:06:18.67 +22:10:44.1 -- not a known variable star
23:06:59.27 +22:06:38.1 -- not a known variable star
23:07:16.96 +21:43:02.1 -- not a known variable star
Found 32 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
32 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
23:00:47.14 +23:52:46.0
23:00:53.54 +20:36:05.1
23:01:26.85 +21:13:24.1
23:02:25.74 +22:27:31.5
23:02:27.28 +23:29:46.0
23:02:34.54 +21:47:11.4
23:02:43.21 +20:37:55.3
23:02:44.31 +23:25:20.8
23:02:56.89 +20:25:02.9
23:02:58.44 +22:11:17.4
23:02:59.63 +22:08:32.2
23:03:09.96 +22:10:44.5
23:03:13.89 +23:23:48.0
23:03:22.17 +23:20:04.8
23:03:27.64 +25:03:03.4
23:03:34.13 +22:14:27.1
23:03:55.41 +19:52:00.6
23:03:55.48 +23:47:03.9
23:04:24.35 +23:44:47.2
23:04:25.10 +21:33:07.2
23:04:43.53 +21:50:41.0
23:04:47.02 +22:02:51.6
23:04:58.44 +21:44:38.7
23:05:14.17 +22:05:38.2
23:05:15.26 +19:57:04.7
23:05:19.22 +21:56:37.3
23:05:43.11 +21:50:29.8
23:06:12.24 +21:32:16.1
23:06:16.77 +21:41:08.9
23:06:18.67 +22:10:44.1
23:06:59.27 +22:06:38.1
23:07:16.96 +21:43:02.1
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461231.84145509 -observatory V36
07:32:18.15 +17:08:02.6 Mercury (5.1mag)
10:11:36.45 +12:41:14.2 Venus (-4.1mag)
04:24:08.70 +21:25:08.1 Mars (1.3mag)
08:16:40.06 +20:11:30.6 Jupiter (-1.8mag)
00:55:50.85 +03:20:28.6 Saturn (0.7mag)
04:07:13.93 +20:45:03.1 Uranus (5.8mag)
00:17:01.50 +00:20:41.2 Neptune (7.8mag)
20:30:54.99 -23:18:00.4 Pluto (14.4mag)
03:11:10.42 +22:17:33.0 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 361 Jul 10 07:24 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461231.84145509:
08:16:46.67 +20:11:07.7 Io (6.1mag)
08:16:42.76 +20:11:22.3 Europa (6.3mag)
08:16:57.11 +20:10:29.0 Ganymede (5.6mag)
08:17:08.07 +20:09:47.1 Callisto (6.8mag)
08:15:11.58 +19:55:39.9 Himalia (15.7mag)
08:16:39.09 +20:11:35.1 Thebe (16.6mag)
08:14:32.92 +20:00:09.6 Elara (17.6mag)
08:20:12.27 +20:05:41.0 Pasiphae (17.8mag)
08:21:37.94 +20:16:35.5 Carme (19.0mag)
00:55:40.69 +03:20:19.6 Titan (8.5mag)
00:55:45.61 +03:20:31.8 Rhea (9.8mag)
00:55:20.15 +03:19:37.6 Iapetus (11.2mag)
00:56:00.12 +03:20:47.6 Hyperion (14.5mag)
00:55:51.59 +03:17:42.5 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 07:24 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.84145509:
17:46:08.71 -32:59:36.4 JWST
16:13:31.53 +48:54:15.6 Chandra
02:43:24.73 +62:15:28.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 07:24 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.84145509 -observatory V36
02:36:15.31 +14:25:37.4 17.9mag P/1996 R2 (Lagerkvist)
18:17:56.85 -34:21:44.4 13.7mag P/2010 H2 (Vales)
06:25:39.87 -68:08:22.4 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:48.16 +32:26:48.4 17.6mag C/2017 K2 (PANSTARRS)
17:03:07.13 +16:02:54.7 18.0mag C/2021 G2 (ATLAS)
01:47:44.87 +08:12:01.7 15.4mag P/2021 N1 (ZTF)
22:59:32.25 +32:17:08.0 17.3mag C/2022 E2 (ATLAS)
06:12:23.27 +26:55:35.0 16.7mag C/2022 N2 (PANSTARRS)
09:55:30.37 +29:46:52.9 16.8mag C/2022 QE78 (ATLAS)
09:09:43.72 +04:59:56.5 17.8mag C/2022 R6 (PANSTARRS)
18:07:13.46 +21:17:39.3 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:35.29 -11:23:15.2 17.7mag P/2023 B1 (PANSTARRS)
21:49:14.83 +67:37:16.9 17.8mag C/2023 H5 (Lemmon)
16:30:54.35 -10:04:37.7 13.9mag C/2023 R1 (PANSTARRS)
08:00:37.96 +65:42:28.4 17.9mag C/2024 A1 (ATLAS)
07:32:48.06 +30:00:10.1 14.6mag C/2024 E1 (Wierzchos)
15:16:19.87 +15:19:41.1 17.5mag C/2024 G6 (ATLAS)
19:41:19.37 +39:23:27.7 13.8mag C/2024 J3 (ATLAS)
21:47:35.60 +46:00:06.1 17.8mag C/2024 R4 (PANSTARRS)
04:49:37.77 -13:47:46.9 15.7mag C/2024 T5 (ATLAS)
06:34:33.87 +29:04:17.7 18.0mag C/2025 J1 (Borisov)
07:14:19.91 -12:53:19.5 16.5mag C/2025 R3 (PANSTARRS)
09:56:04.78 +22:26:14.3 17.6mag C/2025 V2 (Rankin)
12:44:36.81 +03:56:17.7 17.1mag C/2025 Y1 (ATLAS)
16:51:59.00 +79:07:12.4 17.4mag C/2026 A2 (Bok)
02:46:15.88 +45:14:21.7 16.7mag C/2026 B2 (Sun-Gao)
11:25:30.27 +04:32:32.1 16.9mag A/2026 E1
21:19:01.26 -15:04:21.8 7.3mag 10P/Tempel
11:13:27.00 -01:53:12.3 16.1mag 29P/Schwassmann-Wachmann
04:00:09.41 +29:33:07.2 17.8mag 47P/Ashbrook-Jackson
10:08:03.24 +14:00:53.4 17.0mag 63P/Wild
00:48:21.46 -05:05:35.7 15.5mag 65P/Gunn
08:26:55.17 +34:13:09.6 17.9mag 76P/West-Kohoutek-Ikemura
04:27:22.33 +20:10:41.5 13.7mag 78P/Gehrels
02:22:19.01 +10:36:28.8 16.2mag 88P/Howell
06:35:29.89 +30:32:07.4 15.7mag 93P/Lovas
04:20:57.86 +31:07:21.1 16.9mag 114P/Wiseman-Skiff
08:08:40.07 +30:42:16.9 15.3mag 123P/West-Hartley
10:48:06.66 +01:11:28.7 16.8mag 124P/Mrkos
04:51:42.64 +20:48:45.5 16.2mag 128P/Shoemaker-Holt
05:36:14.10 +19:42:50.8 17.8mag 131P/Mueller
00:01:32.55 +02:56:05.3 17.9mag 139P/Vaisala-Oterma
07:13:31.30 +17:01:22.9 15.5mag 141P-D/Machholz
03:16:50.66 -21:06:24.5 15.5mag 161P/Hartley-IRAS
05:33:01.46 +33:56:46.5 15.3mag 162P/SidingSpring
19:04:30.05 +15:04:33.6 14.7mag 169P/NEAT
01:41:00.26 +07:35:50.7 17.7mag 220P/McNaught
16:35:58.23 -08:23:05.9 17.0mag 235P/LINEAR
08:45:15.75 +33:18:01.6 17.9mag 240P/NEAT
20:42:10.79 -49:34:05.6 17.8mag 259P/Garradd
01:59:16.57 +12:05:22.9 15.7mag 260P/McNaught
05:37:11.59 +36:50:31.3 17.4mag 295P/LINEAR
15:06:36.83 +06:03:28.3 17.6mag 391P/Kowalski
08:34:35.63 +19:40:38.0 17.9mag 450P/LONEOS
07:51:44.96 +39:13:01.4 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 07:24 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
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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 07:24 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:28:30.644 -11:03:16.17 AT 2026sql 2026-07-07.04 18.753
11:03:23.326 +12:49:15.53 AT 2026sqk 2026-07-06.95 17.816
02:23:45.306 -56:30:54.13 AT 2026sqj 2026-07-07.14 18.706
20:05:32.749 -40:04:20.18 AT 2026sqi 2026-07-07.00 19.025
13:27:09.068 +62:50:19.22 AT 2026sqh 2026-07-06.32 19.347
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
-rw-r--r-- 1 apache apache 30K Jul 10 07:24 tns_transients_list.txt
