This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z
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 10.3924 2461231.8924 12.86 23:20:04.82 +12:48:09.4
90.98602 -44.32889 galactic Peg Second-epoch detections are separated by 2.2" and 8.5 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 | 23:20:04.82 +12:48:09.4 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.377+/-0.032 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:20:04.82 +12:48:09.4: 13.78 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:20:04.82 +12:48:09.4: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.86CV 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 10.3924 2461231.8924 12.82 23:00:42.37 +14:44:07.7
86.86466 -40.25644 galactic Peg Second-epoch detections are separated by 0.7" and 8.4 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 | 23:00:42.37 +14:44:07.7 (user input) | T | P | (position from user input) J-Ks=0.389+/-0.028 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:42.37 +14:44:07.7: 13.76 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:42.37 +14:44:07.7: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 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,2461231.8924,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.88 22:58:54.06 +16:08:49.6
87.37895 -38.83352 galactic Peg Second-epoch detections are separated by 2.5" and 8.5 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 | 22:58:54.06 +16:08:49.6 (user input) | T | P | (position from user input) J-Ks=0.328+/-0.032 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:58:54.06 +16:08:49.6: 13.75 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:58:54.06 +16:08:49.6: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.93 23:17:58.72 +12:13:27.1
89.96283 -44.58240 galactic Peg Second-epoch detections are separated by 3.1" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:17:58.72 +12:13:27.1 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.033 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:58.72 +12:13:27.1: 13.89 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:58.72 +12:13:27.1: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461231.8924,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 12.71 23:07:14.39 +11:21:56.6
86.20392 -43.95053 galactic Peg Second-epoch detections are separated by 0.9" and 8.5 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 | 23:07:14.39 +11:21:56.6 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.350+/-0.034 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:14.39 +11:21:56.6: 13.63 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:14.39 +11:21:56.6: 13.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461231.8924,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.99 23:17:34.11 +12:12:01.4
89.82412 -44.55331 galactic Peg Second-epoch detections are separated by 0.8" and 8.5 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 | 23:17:34.11 +12:12:01.4 (user input) | T | P | (position from user input) J-Ks=0.479+/-0.030 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:34.11 +12:12:01.4: 13.97 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:34.11 +12:12:01.4: 14.14 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.04 +/- 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,2461231.8924,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.76 23:12:50.64 +16:03:07.6
91.05084 -40.63760 galactic Peg Second-epoch detections are separated by 1.1" and 8.4 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 | 23:12:50.64 +16:03:07.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.408+/-0.029 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:12:50.64 +16:03:07.6: 13.65 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:12:50.64 +16:03:07.6: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.12 23:09:58.58 +11:17:00.9
86.93047 -44.38077 galactic Peg Second-epoch detections are separated by 2.0" and 8.7 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 | 23:09:58.58 +11:17:00.9 (user input) | T | P | (position from user input) J-Ks=0.489+/-0.036 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:09:58.58 +11:17:00.9: 14.09 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:09:58.58 +11:17:00.9: 14.32 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.06
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,2461231.8924,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.12CV 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 10.3924 2461231.8924 13.13 23:08:00.83 +13:46:20.7
88.17477 -42.01408 galactic Peg Second-epoch detections are separated by 0.8" and 8.5 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 | 23:08:00.83 +13:46:20.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.430+/-0.031 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:08:00.83 +13:46:20.7: 13.96 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:08:00.83 +13:46:20.7: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.04 +/- 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,2461231.8924,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 12.91 23:11:12.86 +13:50:54.6
89.12582 -42.35002 galactic Peg Second-epoch detections are separated by 0.9" and 8.5 pix
The object was found in VSX 1" IX Peg
Type: RRAB
# Max. Min./Amp. JD0 Period
13.030 V 14.130 V 2451476.29000 0.601066290000 A2
The object was not found in astcheck.
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:11:12.86 +13:50:54.6: 14.01 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:11:12.86 +13:50:54.6: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.97 +/- 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
IX Peg,2461231.8924,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IX Peg 20260710.3924 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.85 22:59:44.39 +15:45:04.8
87.32324 -39.27559 galactic Peg Second-epoch detections are separated by 1.2" and 8.5 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 | 22:59:44.39 +15:45:04.8 (user input) | T | P | (position from user input) J-Ks=0.740+/-0.025 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:44.39 +15:45:04.8: 13.81 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:44.39 +15:45:04.8: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461231.8924,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.13 23:07:53.09 +12:10:55.2
86.99536 -43.34779 galactic Peg Second-epoch detections are separated by 1.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:07:53.09 +12:10:55.2 (user input) | T | P | (position from user input) J-Ks=0.758+/-0.028 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:53.09 +12:10:55.2: 14.16 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:53.09 +12:10:55.2: 14.11 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.06
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,2461231.8924,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 13.17 23:15:13.73 +13:06:20.8
89.76400 -43.48394 galactic Peg Second-epoch detections are separated by 2.8" and 8.4 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 | 23:15:13.73 +13:06:20.8 (user input) | T | P | (position from user input) J-Ks=0.570+/-0.025 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:15:13.73 +13:06:20.8: 14.07 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:15:13.73 +13:06:20.8: 14.21 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.06
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,2461231.8924,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.84 23:08:23.38 +11:28:53.8
86.62041 -44.00526 galactic Peg Second-epoch detections are separated by 0.7" and 8.6 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 | 23:08:23.38 +11:28:53.8 (user input) | T | P | (position from user input) SpType: M2 (LAMOST DR5)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:08:23.38 +11:28:53.8: 13.84 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:08:23.38 +11:28:53.8: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.86 +/- 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,2461231.8924,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.73 23:05:06.07 +11:41:50.9
85.84708 -43.38673 galactic Peg Second-epoch detections are separated by 1.4" and 8.7 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 | Large-amplitude variable Gaia DR2 2715600137844293248 | 23:05:06.07 +11:41:50.9 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.347+/-0.033 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:06.07 +11:41:50.9: 13.84 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:06.07 +11:41:50.9: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 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
Large-amplitude variable Gaia DR2 2715600137844293248,2461231.8924,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2715600137844293248 20260710.3924 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.05 23:14:50.89 +12:58:11.2
89.55936 -43.55516 galactic Peg Second-epoch detections are separated by 1.0" and 8.7 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 | 23:14:50.89 +12:58:11.2 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.031 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:14:50.89 +12:58:11.2: 13.99 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:14:50.89 +12:58:11.2: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.99 +/- 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,2461231.8924,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.88 23:00:32.47 +14:57:25.6
86.97777 -40.04849 galactic Peg Second-epoch detections are separated by 1.0" and 8.3 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 | 23:00:32.47 +14:57:25.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.345+/-0.029 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:32.47 +14:57:25.6: 13.87 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:32.47 +14:57:25.6: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 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,2461231.8924,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.09 23:01:50.55 +14:18:35.0
86.86571 -40.76328 galactic Peg Second-epoch detections are separated by 1.2" and 8.2 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 | Large-amplitude variable Gaia DR2 2816057193807096704 | 23:01:50.55 +14:18:35.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.521+/-0.030 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:50.55 +14:18:35.0: 14.02 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:50.55 +14:18:35.0: 14.04 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.03 +/- 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
Large-amplitude variable Gaia DR2 2816057193807096704,2461231.8924,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2816057193807096704 20260710.3924 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.78 23:07:45.71 +17:34:37.2
90.65514 -38.71105 galactic Peg Second-epoch detections are separated by 1.7" and 8.2 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 | 23:07:45.71 +17:34:37.2 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.030 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:45.71 +17:34:37.2: 13.86 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:45.71 +17:34:37.2: 13.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 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,2461231.8924,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.78CV 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 10.3924 2461231.8924 12.89 23:01:05.75 +14:16:47.0
86.64368 -40.69042 galactic Peg Second-epoch detections are separated by 0.8" and 8.4 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 | 23:01:05.75 +14:16:47.0 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.031 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:05.75 +14:16:47.0: 13.84 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:05.75 +14:16:47.0: 14.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461231.8924,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.15 23:18:56.83 +13:04:28.4
90.83288 -43.95726 galactic Peg Second-epoch detections are separated by 1.0" and 8.6 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 | 23:18:56.83 +13:04:28.4 (user input) | T | P | (position from user input) J-Ks=0.363+/-0.036 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:18:56.83 +13:04:28.4: 14.32 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:18:56.83 +13:04:28.4: 14.48 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.07
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,2461231.8924,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.15CV 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 10.3924 2461231.8924 12.80 23:06:42.34 +11:09:09.0
85.88976 -44.05801 galactic Peg Second-epoch detections are separated by 1.4" and 8.3 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 | 23:06:42.34 +11:09:09.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.341+/-0.034 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:42.34 +11:09:09.0: 13.71 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:42.34 +11:09:09.0: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.93 23:06:55.61 +12:52:43.6
87.23327 -42.63374 galactic Peg Second-epoch detections are separated by 1.0" and 8.5 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 | 23:06:55.61 +12:52:43.6 (user input) | T | P | (position from user input) J-Ks=0.376+/-0.031 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:55.61 +12:52:43.6: 13.89 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:55.61 +12:52:43.6: 13.98 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461231.8924,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 13.02 23:09:04.36 +17:36:19.2
91.02109 -38.84140 galactic Peg Second-epoch detections are separated by 0.8" and 8.3 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 | 23:09:04.36 +17:36:19.2 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.329+/-0.032 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:09:04.36 +17:36:19.2: 13.89 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:09:04.36 +17:36:19.2: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.91 +/- 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,2461231.8924,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.12 23:01:14.21 +15:24:44.7
87.48158 -39.75507 galactic Peg Second-epoch detections are separated by 0.9" and 8.4 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 | 23:01:14.21 +15:24:44.7 (user input) | T | P | (position from user input) J-Ks=0.279+/-0.032 (F)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:14.21 +15:24:44.7: 14.10 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:14.21 +15:24:44.7: 14.11 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 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,2461231.8924,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.12CV 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 10.3924 2461231.8924 13.07 23:01:52.26 +10:53:55.8
84.32725 -43.60918 galactic Peg Second-epoch detections are separated by 2.0" and 8.7 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 | 23:01:52.26 +10:53:55.8 (user input) | T | P | (position from user input) J-Ks=0.683+/-0.033 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:52.26 +10:53:55.8: 14.12 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:52.26 +10:53:55.8: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.04 +/- 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,2461231.8924,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.07CV 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 10.3924 2461231.8924 13.13 23:17:52.45 +11:56:52.0
89.73846 -44.80961 galactic Peg Second-epoch detections are separated by 1.4" and 8.3 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 | 23:17:52.45 +11:56:52.0 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.608+/-0.035 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:52.45 +11:56:52.0: 14.19 +/- 0.09 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:52.45 +11:56:52.0: 14.22 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.07
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,2461231.8924,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 12.97 23:08:58.10 +17:34:08.0
90.97022 -38.86081 galactic Peg Second-epoch detections are separated by 0.9" and 8.2 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 | 23:08:58.10 +17:34:08.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.401+/-0.030 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:08:58.10 +17:34:08.0: 13.75 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:08:58.10 +17:34:08.0: 13.86 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.80 +/- 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,2461231.8924,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.97CV 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 10.3924 2461231.8924 13.11 23:05:46.29 +11:01:32.2
85.52632 -44.03837 galactic Peg Second-epoch detections are separated by 1.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J346.4431+11.0254 | 23:05:46.29 +11:01:32.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.474+/-0.042 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:46.29 +11:01:32.2: 14.32 +/- 0.09 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:46.29 +11:01:32.2: 14.39 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J346.4431+11.0254,2461231.8924,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J346.4431+11.0254 20260710.3924 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 10.3924 2461231.8924 12.82 23:18:45.66 +12:25:24.8
90.33401 -44.50323 galactic Peg Second-epoch detections are separated by 2.3" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:18:45.66 +12:25:24.8 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.032 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:18:45.66 +12:25:24.8: 13.76 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:18:45.66 +12:25:24.8: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.84 +/- 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,2461231.8924,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.71 23:00:19.84 +14:43:35.5
86.75839 -40.21470 galactic Peg Second-epoch detections are separated by 1.3" and 8.4 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 | 23:00:19.84 +14:43:35.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:19.84 +14:43:35.5: 13.63 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:19.84 +14:43:35.5: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 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,2461231.8924,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.81 23:03:16.87 +14:56:31.1
87.69890 -40.41611 galactic Peg Second-epoch detections are separated by 1.0" and 8.3 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 | 23:03:16.87 +14:56:31.1 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.030 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:16.87 +14:56:31.1: 13.77 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:16.87 +14:56:31.1: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461231.8924,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.09 23:06:47.97 +11:00:11.3
85.80282 -44.19565 galactic Peg Second-epoch detections are separated by 1.3" and 8.4 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 | 23:06:47.97 +11:00:11.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.576+/-0.033 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:47.97 +11:00:11.3: 14.19 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:47.97 +11:00:11.3: 14.42 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.07
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,2461231.8924,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.21 23:04:24.10 +14:33:40.5
87.73521 -40.88256 galactic Peg Second-epoch detections are separated by 2.9" and 8.7 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 | 23:04:24.10 +14:33:40.5 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.395+/-0.035 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:24.10 +14:33:40.5: 14.20 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:24.10 +14:33:40.5: 14.09 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.14 +/- 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,2461231.8924,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 13.27 23:04:24.47 +13:57:43.4
87.31360 -41.39070 galactic Peg Second-epoch detections are separated by 1.5" and 8.2 pix
The object was found in VSX 1" ASASSN-V J230424.43+135744.0
Type: ROT
# Max. Min./Amp. JD0 Period
14.880 g Y 0.190 g 2459470.42100 1.581000000000
The object was not found in astcheck.
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:24.47 +13:57:43.4: 14.44 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:24.47 +13:57:43.4: 14.61 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.08
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
ASASSN-V J230424.43+135744.0,2461231.8924,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J230424.43+135744.0 20260710.3924 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.22 23:07:22.02 +13:38:01.7
87.89683 -42.04979 galactic Peg Second-epoch detections are separated by 1.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:07:22.02 +13:38:01.7 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.029 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:22.02 +13:38:01.7: 14.45 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:22.02 +13:38:01.7: 14.39 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.07
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,2461231.8924,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 12.66 23:02:01.46 +12:17:11.4
85.43314 -42.48050 galactic Peg Second-epoch detections are separated by 0.8" and 8.4 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 | 23:02:01.46 +12:17:11.4 (user input) | T | P | (position from user input) J-Ks=0.676+/-0.028 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:01.46 +12:17:11.4: 13.73 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:01.46 +12:17:11.4: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461231.8924,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.66CV 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 10.3924 2461231.8924 12.79 23:02:13.34 +14:59:20.1
87.44793 -40.24006 galactic Peg Second-epoch detections are separated by 1.6" and 8.1 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 | 23:02:13.34 +14:59:20.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.487+/-0.029 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:13.34 +14:59:20.1: 13.72 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:13.34 +14:59:20.1: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 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,2461231.8924,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 12.60 23:03:09.91 +14:13:42.2
87.16487 -41.00444 galactic Peg Second-epoch detections are separated by 0.5" and 8.3 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 | 23:03:09.91 +14:13:42.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:09.91 +14:13:42.2: 13.61 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:09.91 +14:13:42.2: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 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,2461231.8924,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.60CV 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 10.3924 2461231.8924 12.91 23:00:54.28 +14:43:08.2
86.90581 -40.29632 galactic Peg Second-epoch detections are separated by 1.4" and 8.3 pix
The object was found in VSX 1" Gaia DR3 2816130208251096192
Type: ROT
# Max. Min./Amp. JD0 Period
13.680 G 13.710 G K
The object was not found in astcheck.
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:54.28 +14:43:08.2: 13.87 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:54.28 +14:43:08.2: 13.80 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2816130208251096192,2461231.8924,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2816130208251096192 20260710.3924 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.01 23:18:41.78 +12:38:04.4
90.45958 -44.31160 galactic Peg Second-epoch detections are separated by 0.7" and 8.6 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 | 23:18:41.78 +12:38:04.4 (user input) | T | P | (position from user input) J-Ks=0.396+/-0.033 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:18:41.78 +12:38:04.4: 13.91 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:18:41.78 +12:38:04.4: 13.97 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.94 +/- 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,2461231.8924,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.76 23:05:08.49 +11:26:23.2
85.66345 -43.60754 galactic Peg Second-epoch detections are separated by 2.0" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:05:08.49 +11:26:23.2 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.034 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:08.49 +11:26:23.2: 13.76 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:08.49 +11:26:23.2: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.73 +/- 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,2461231.8924,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.98 23:08:40.25 +11:21:43.8
86.61187 -44.14302 galactic Peg Second-epoch detections are separated by 2.9" and 8.7 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 | 23:08:40.25 +11:21:43.8 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.036 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:08:40.25 +11:21:43.8: 14.12 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:08:40.25 +11:21:43.8: 14.23 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
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,2461231.8924,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.09 23:00:40.74 +15:43:53.0
87.55593 -39.41374 galactic Peg Second-epoch detections are separated by 1.9" and 8.3 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 | 23:00:40.74 +15:43:53.0 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.037 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:40.74 +15:43:53.0: 14.10 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:40.74 +15:43:53.0: 14.08 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461231.8924,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.81 23:05:19.41 +13:23:49.9
87.16109 -41.98700 galactic Peg Second-epoch detections are separated by 2.1" and 8.7 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 | 23:05:19.41 +13:23:49.9 (user input) | T | P | (position from user input) J-Ks=0.790+/-0.028 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:19.41 +13:23:49.9: 13.70 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:19.41 +13:23:49.9: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 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,2461231.8924,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.90 22:59:48.90 +15:27:59.9
87.14430 -39.52511 galactic Peg Second-epoch detections are separated by 0.9" and 8.5 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 | 22:59:48.90 +15:27:59.9 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.033 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:48.90 +15:27:59.9: 13.87 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:48.90 +15:27:59.9: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 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,2461231.8924,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.85 23:06:46.87 +11:22:52.7
86.08471 -43.87634 galactic Peg Second-epoch detections are separated by 0.5" and 8.5 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 | 23:06:46.87 +11:22:52.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.425+/-0.038 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:46.87 +11:22:52.7: 13.74 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:46.87 +11:22:52.7: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.90 23:01:01.74 +15:35:43.0
87.55377 -39.57381 galactic Peg Second-epoch detections are separated by 0.2" and 8.3 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 | 23:01:01.74 +15:35:43.0 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.031 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:01.74 +15:35:43.0: 13.87 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:01.74 +15:35:43.0: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.92 23:18:17.97 +12:22:47.2
90.16629 -44.48590 galactic Peg Second-epoch detections are separated by 1.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:18:17.97 +12:22:47.2 (user input) | T | P | (position from user input) J-Ks=0.518+/-0.030 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:18:17.97 +12:22:47.2: 13.89 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:18:17.97 +12:22:47.2: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 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,2461231.8924,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.95 23:07:18.32 +17:51:38.8
90.71554 -38.41085 galactic Peg Second-epoch detections are separated by 1.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2830663999624444288 | 23:07:19.27 +17:52:23.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.549+/-0.030 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:18.32 +17:51:38.8: 14.00 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:18.32 +17:51:38.8: 13.86 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.92 +/- 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
Gaia DR3 2830663999624444288,2461231.8924,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2830663999624444288 20260710.3924 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.04 23:17:45.91 +12:45:36.3
90.26962 -44.09073 galactic Peg Second-epoch detections are separated by 1.8" and 8.5 pix
The object was found in VSX 0" Gaia DR3 2812077786348121728
Type: ROT
# Max. Min./Amp. JD0 Period
13.840 G 13.870 G K
The object was not found in astcheck.
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:45.91 +12:45:36.3: 14.02 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:45.91 +12:45:36.3: 14.23 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.06
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 2812077786348121728,2461231.8924,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2812077786348121728 20260710.3924 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 10.3924 2461231.8924 13.05 23:15:15.26 +12:49:55.7
89.58215 -43.72389 galactic Peg Second-epoch detections are separated by 1.7" and 8.7 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 | 23:15:15.26 +12:49:55.7 (user input) | T | P | (position from user input) J-Ks=0.474+/-0.031 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:15:15.26 +12:49:55.7: 14.27 +/- 0.09 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:15:15.26 +12:49:55.7: 14.23 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.06
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,2461231.8924,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.07 23:03:45.31 +14:33:39.5
87.55982 -40.79970 galactic Peg Second-epoch detections are separated by 2.1" and 8.7 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 | 23:03:45.31 +14:33:39.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.893+/-0.027 (M)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:45.31 +14:33:39.5: 14.09 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:45.31 +14:33:39.5: 14.21 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.06
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,2461231.8924,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.07CV 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 10.3924 2461231.8924 12.42 23:00:30.00 +16:08:12.8
87.78868 -39.04798 galactic Peg Second-epoch detections are separated by 0.5" and 8.4 pix
The object was found in VSX 0" ASASSN-V J230029.98+160813.1
Type: YSO
# Max. Min./Amp. JD0 Period
13.180 V 13.300 V
The object was not found in astcheck.
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:30.00 +16:08:12.8: 13.39 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:30.00 +16:08:12.8: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J230029.98+160813.1,2461231.8924,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J230029.98+160813.1 20260710.3924 12.42CV 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 10.3924 2461231.8924 12.89 22:59:52.53 +16:10:21.8
87.65021 -38.93757 galactic Peg Second-epoch detections are separated by 0.9" and 8.3 pix
The object was found in VSX 0" Gaia DR3 2828861419029237632
Type: ROT
# Max. Min./Amp. JD0 Period
13.490 G 13.520 G K
The object was not found in astcheck.
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:52.53 +16:10:21.8: 13.85 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:52.53 +16:10:21.8: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2828861419029237632,2461231.8924,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2828861419029237632 20260710.3924 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.69 23:03:02.91 +14:12:59.7
87.12487 -40.99922 galactic Peg Second-epoch detections are separated by 0.6" and 8.3 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 | 23:03:02.91 +14:12:59.7 (user input) | T | P | (position from user input) J-Ks=0.317+/-0.029 (F)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:02.91 +14:12:59.7: 13.60 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:02.91 +14:12:59.7: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461231.8924,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.79 23:07:17.18 +18:02:21.2
90.82383 -38.25386 galactic Peg Second-epoch detections are separated by 0.6" and 8.4 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 | 23:07:17.18 +18:02:21.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.394+/-0.032 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:17.18 +18:02:21.2: 13.86 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:17.18 +18:02:21.2: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 12.72 23:02:11.79 +14:28:14.6
87.07555 -40.67398 galactic Peg Second-epoch detections are separated by 0.8" and 8.5 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 | 23:02:11.79 +14:28:14.6 (user input) | T | P | (position from user input) J-Ks=0.614+/-0.027 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:11.79 +14:28:14.6: 13.69 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:11.79 +14:28:14.6: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461231.8924,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.12 23:18:44.12 +13:00:25.8
90.72471 -43.99107 galactic Peg Second-epoch detections are separated by 2.0" and 8.5 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 | 23:18:44.12 +13:00:25.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.468+/-0.035 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:18:44.12 +13:00:25.8: 14.04 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:18:44.12 +13:00:25.8: 14.15 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.06
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,2461231.8924,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.12CV 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 10.3924 2461231.8924 13.07 23:03:19.21 +14:08:11.8
87.14159 -41.10204 galactic Peg Second-epoch detections are separated by 1.6" and 8.4 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 | 23:03:19.21 +14:08:11.8 (user input) | T | P | (position from user input) J-Ks=0.848+/-0.030 (M)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:19.21 +14:08:11.8: 14.02 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:19.21 +14:08:11.8: 14.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461231.8924,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.07CV 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 10.3924 2461231.8924 13.02 23:00:58.49 +14:45:06.4
86.94780 -40.27788 galactic Peg Second-epoch detections are separated by 1.1" and 8.3 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 | 23:00:58.49 +14:45:06.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.393+/-0.032 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:58.49 +14:45:06.4: 13.98 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:58.49 +14:45:06.4: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 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,2461231.8924,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.04 23:02:30.80 +11:58:02.0
85.32750 -42.81244 galactic Peg Second-epoch detections are separated by 0.7" and 8.4 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 | 23:02:30.80 +11:58:02.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.419+/-0.038 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:30.80 +11:58:02.0: 14.05 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:30.80 +11:58:02.0: 14.05 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.05 +/- 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,2461231.8924,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 12.96 23:04:10.77 +13:48:44.9
87.14439 -41.48743 galactic Peg Second-epoch detections are separated by 1.8" and 8.5 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 | 23:04:10.77 +13:48:44.9 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:10.77 +13:48:44.9: 14.00 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:10.77 +13:48:44.9: 14.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461231.8924,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 13.14 23:00:12.69 +15:13:32.4
87.07975 -39.77954 galactic Peg Second-epoch detections are separated by 1.3" and 8.3 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 | 23:00:12.69 +15:13:32.4 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.029 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:12.69 +15:13:32.4: 13.99 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:12.69 +15:13:32.4: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461231.8924,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 12.60 22:59:15.94 +16:05:03.1
87.43026 -38.93369 galactic Peg Second-epoch detections are separated by 0.4" and 8.4 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 | 22:59:15.94 +16:05:03.1 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.044 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:15.94 +16:05:03.1: 13.56 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:15.94 +16:05:03.1: 13.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.60CV 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 10.3924 2461231.8924 12.53 22:59:55.24 +15:48:04.2
87.40523 -39.25698 galactic Peg Second-epoch detections are separated by 1.0" and 8.6 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 | 22:59:55.24 +15:48:04.2 (user input) | T | P | (position from user input) J-Ks=0.484+/-0.028 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:55.24 +15:48:04.2: 13.57 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:55.24 +15:48:04.2: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.72 23:00:04.59 +15:03:00.7
86.92041 -39.90949 galactic Peg Second-epoch detections are separated by 0.9" and 8.4 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 | 23:00:04.59 +15:03:00.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.581+/-0.026 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:04.59 +15:03:00.7: 13.56 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:04.59 +15:03:00.7: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461231.8924,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.74 23:04:10.25 +13:39:06.9
87.02691 -41.62179 galactic Peg Second-epoch detections are separated by 2.2" and 8.7 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 | 23:04:10.25 +13:39:06.9 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.324+/-0.030 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:10.25 +13:39:06.9: 13.70 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:10.25 +13:39:06.9: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.74CV 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 10.3924 2461231.8924 12.82 23:00:48.21 +16:14:59.9
87.94556 -38.99105 galactic Peg Second-epoch detections are separated by 2.1" and 8.7 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 | 23:00:48.21 +16:14:59.9 (user input) | T | P | (position from user input) J-Ks=0.586+/-0.030 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:48.21 +16:14:59.9: 13.83 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:48.21 +16:14:59.9: 13.73 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461231.8924,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.87 23:01:21.26 +14:36:49.4
86.95120 -40.44364 galactic Peg Second-epoch detections are separated by 0.4" and 8.4 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 | 23:01:21.26 +14:36:49.4 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.626+/-0.028 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:21.26 +14:36:49.4: 13.82 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:21.26 +14:36:49.4: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.93 23:02:10.99 +14:14:21.7
86.90724 -40.86708 galactic Peg Second-epoch detections are separated by 0.7" and 8.3 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 | 23:02:10.99 +14:14:21.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.334+/-0.030 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:10.99 +14:14:21.7: 13.83 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:10.99 +14:14:21.7: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 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,2461231.8924,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 12.80 23:07:35.22 +10:57:19.2
85.99248 -44.34123 galactic Peg Second-epoch detections are separated by 2.0" and 8.7 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 | 23:07:35.22 +10:57:19.2 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.037 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:35.22 +10:57:19.2: 13.66 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:35.22 +10:57:19.2: 13.97 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.35 22:59:26.53 +15:59:30.1
87.41224 -39.03448 galactic Peg Second-epoch detections are separated by 1.3" and 8.4 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 | 22:59:26.53 +15:59:30.1 (user input) | T | P | (position from user input) J-Ks=0.360+/-0.035 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:26.53 +15:59:30.1: 13.35 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:26.53 +15:59:30.1: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.12 23:04:05.84 +14:04:41.9
87.31152 -41.25219 galactic Peg Second-epoch detections are separated by 1.5" and 8.2 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 | 23:04:05.84 +14:04:41.9 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.033 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:05.84 +14:04:41.9: 14.04 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:05.84 +14:04:41.9: 14.17 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 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,2461231.8924,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.12CV 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 10.3924 2461231.8924 12.92 23:05:18.91 +18:32:16.3
90.62581 -37.58815 galactic Peg Second-epoch detections are separated by 2.6" and 8.2 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 | 23:05:18.91 +18:32:16.3 (user input) | T | P | (position from user input) J-Ks=0.454+/-0.028 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:18.91 +18:32:16.3: 13.83 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:18.91 +18:32:16.3: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461231.8924,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.05 23:01:55.72 +15:00:15.3
87.38023 -40.18915 galactic Peg Second-epoch detections are separated by 1.0" and 8.2 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 | 23:01:55.72 +15:00:15.3 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.564+/-0.030 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:55.72 +15:00:15.3: 14.06 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:55.72 +15:00:15.3: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 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,2461231.8924,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.01 23:06:42.15 +17:42:30.1
90.45956 -38.47108 galactic Peg Second-epoch detections are separated by 1.8" and 8.6 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 | 23:06:42.15 +17:42:30.1 (user input) | T | P | (position from user input) J-Ks=0.440+/-0.031 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:42.15 +17:42:30.1: 13.97 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:42.15 +17:42:30.1: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.99 +/- 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,2461231.8924,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.86 23:05:54.16 +18:42:43.7
90.88776 -37.50684 galactic Peg Second-epoch detections are separated by 1.2" and 8.2 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 | 23:05:54.16 +18:42:43.7 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.654+/-0.027 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:54.16 +18:42:43.7: 13.79 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:54.16 +18:42:43.7: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 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,2461231.8924,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.86CV 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 10.3924 2461231.8924 12.97 23:06:10.42 +11:31:12.2
86.01658 -43.67888 galactic Peg Second-epoch detections are separated by 1.3" and 8.7 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 | 23:06:10.42 +11:31:12.2 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.722+/-0.030 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:10.42 +11:31:12.2: 14.02 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:10.42 +11:31:12.2: 14.07 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.04 +/- 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,2461231.8924,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.97CV 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 10.3924 2461231.8924 12.63 23:02:48.53 +12:03:14.7
85.47508 -42.78020 galactic Peg Second-epoch detections are separated by 1.5" and 8.7 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 | 23:02:48.53 +12:03:14.7 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.035 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:48.53 +12:03:14.7: 13.53 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:48.53 +12:03:14.7: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 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,2461231.8924,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.04 23:21:06.79 +13:09:57.9
91.53740 -44.13058 galactic Peg Second-epoch detections are separated by 2.3" and 8.3 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 | 23:21:06.79 +13:09:57.9 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.600+/-0.030 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:21:06.79 +13:09:57.9: 14.05 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:21:06.79 +13:09:57.9: 14.11 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.06
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,2461231.8924,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 13.10 23:05:21.15 +11:40:30.1
85.90103 -43.43920 galactic Peg Second-epoch detections are separated by 0.7" and 8.4 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 | 23:05:21.15 +11:40:30.1 (user input) | T | P | (position from user input) J-Ks=0.686+/-0.030 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:21.15 +11:40:30.1: 14.05 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:21.15 +11:40:30.1: 14.14 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461231.8924,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.10CV 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 10.3924 2461231.8924 12.91 23:01:27.37 +14:57:37.5
87.22343 -40.16489 galactic Peg Second-epoch detections are separated by 1.7" and 8.5 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 | 23:01:27.37 +14:57:37.5 (user input) | T | P | (position from user input) J-Ks=0.295+/-0.033 (F)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:27.37 +14:57:37.5: 13.96 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:27.37 +14:57:37.5: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.89 23:17:57.23 +12:59:28.5
90.48317 -43.91197 galactic Peg Second-epoch detections are separated by 1.1" and 8.6 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 | 23:17:57.23 +12:59:28.5 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.031 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:57.23 +12:59:28.5: 14.05 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:57.23 +12:59:28.5: 13.98 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 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,2461231.8924,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.07 23:07:33.87 +17:59:32.8
90.86731 -38.32732 galactic Peg Second-epoch detections are separated by 1.0" and 8.5 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 | 23:07:33.87 +17:59:32.8 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.341+/-0.032 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:33.87 +17:59:32.8: 14.06 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:33.87 +17:59:32.8: 14.13 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.06
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,2461231.8924,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.07CV 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 10.3924 2461231.8924 13.01 23:00:30.96 +15:39:09.4
87.45839 -39.45923 galactic Peg Second-epoch detections are separated by 1.2" and 8.5 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 | 23:00:30.96 +15:39:09.4 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.032 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:30.96 +15:39:09.4: 14.03 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:30.96 +15:39:09.4: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 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,2461231.8924,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.44 23:01:21.09 +14:34:02.4
86.91748 -40.48230 galactic Peg Second-epoch detections are separated by 0.7" and 8.4 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 | 23:01:21.09 +14:34:02.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.388+/-0.029 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:21.09 +14:34:02.4: 13.32 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:21.09 +14:34:02.4: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 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,2461231.8924,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.02 22:59:31.40 +15:22:01.3
86.99776 -39.57088 galactic Peg Second-epoch detections are separated by 2.3" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J344.8793+15.3649 | 22:59:31.40 +15:22:01.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:31.40 +15:22:01.3: 13.95 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:31.40 +15:22:01.3: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J344.8793+15.3649,2461231.8924,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J344.8793+15.3649 20260710.3924 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.98 23:01:11.53 +14:35:01.6
86.88655 -40.44761 galactic Peg Second-epoch detections are separated by 2.0" and 8.4 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 | 23:01:11.53 +14:35:01.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:11.53 +14:35:01.6: 13.96 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:11.53 +14:35:01.6: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.94 +/- 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,2461231.8924,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.02 23:03:11.92 +14:15:35.5
87.19632 -40.98223 galactic Peg Second-epoch detections are separated by 1.4" and 8.3 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 | 23:03:11.92 +14:15:35.5 (user input) | T | P | (position from user input) J-Ks=0.390+/-0.030 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:11.92 +14:15:35.5: 13.96 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:11.92 +14:15:35.5: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461231.8924,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.02 23:03:10.79 +09:25:40.7
83.52765 -45.00195 galactic Peg Second-epoch detections are separated by 0.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.690 Wratislavia 3 -2 3 12.9 0 0
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:10.79 +09:25:40.7: 13.37 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:10.79 +09:25:40.7: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461231.8924,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3924 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.76 23:19:12.77 +12:55:41.0
90.81264 -44.11675 galactic Peg Second-epoch detections are separated by 0.5" and 8.6 pix
The object was found in VSX 1" Gaia DR3 2811336852950062208
Type: ROT
# Max. Min./Amp. JD0 Period
13.520 G 13.540 G K
The object was not found in astcheck.
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:19:12.77 +12:55:41.0: 13.81 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:19:12.77 +12:55:41.0: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 2811336852950062208,2461231.8924,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2811336852950062208 20260710.3924 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.89 23:16:06.00 +12:54:53.4
89.88644 -43.75529 galactic Peg Second-epoch detections are separated by 0.6" and 8.5 pix
The object was found in VSX 1" Gaia DR3 2812052016544472576
Type: ROT
# Max. Min./Amp. JD0 Period
13.720 G 13.750 G G
The object was not found in astcheck.
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:16:06.00 +12:54:53.4: 13.96 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:16:06.00 +12:54:53.4: 14.04 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 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
Gaia DR3 2812052016544472576,2461231.8924,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2812052016544472576 20260710.3924 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.98 23:17:14.34 +12:17:48.8
89.79356 -44.42955 galactic Peg Second-epoch detections are separated by 0.7" and 8.5 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 | 23:17:14.34 +12:17:48.8 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.512+/-0.030 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:14.34 +12:17:48.8: 13.98 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:14.34 +12:17:48.8: 13.97 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.97 +/- 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,2461231.8924,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.56 23:05:07.99 +11:32:59.8
85.74463 -43.51437 galactic Peg Second-epoch detections are separated by 0.8" and 8.6 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 | 23:05:07.99 +11:32:59.8 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.033 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:07.99 +11:32:59.8: 13.48 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:07.99 +11:32:59.8: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.97 23:03:12.99 +12:05:43.4
85.61937 -42.80085 galactic Peg Second-epoch detections are separated by 3.5" and 8.6 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 | 23:03:12.99 +12:05:43.4 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.030 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:12.99 +12:05:43.4: 13.94 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:12.99 +12:05:43.4: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 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,2461231.8924,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.97CV 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 10.3924 2461231.8924 12.57 23:08:37.51 +18:53:35.1
91.70770 -37.66713 galactic Peg Second-epoch detections are separated by 1.1" and 8.3 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 | 23:08:37.51 +18:53:35.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.423+/-0.030 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:08:37.51 +18:53:35.1: 13.44 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:08:37.51 +18:53:35.1: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 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,2461231.8924,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.57CV 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 10.3924 2461231.8924 13.04 23:04:53.36 +11:30:55.2
85.64960 -43.51046 galactic Peg Second-epoch detections are separated by 2.5" and 8.7 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 | Large-amplitude variable Gaia DR2 2715595950248508032 | 23:04:53.36 +11:30:55.2 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.535+/-0.033 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:53.36 +11:30:55.2: 13.96 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:53.36 +11:30:55.2: 14.28 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.06
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
Large-amplitude variable Gaia DR2 2715595950248508032,2461231.8924,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2715595950248508032 20260710.3924 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 10.3924 2461231.8924 13.01 23:07:42.26 +12:03:28.9
86.85278 -43.42891 galactic Peg Second-epoch detections are separated by 1.4" and 8.7 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 | 23:07:42.26 +12:03:28.9 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.411+/-0.037 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:42.26 +12:03:28.9: 13.98 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:42.26 +12:03:28.9: 14.29 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.08 +/- 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,2461231.8924,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.69 23:00:45.47 +16:08:38.5
87.86106 -39.07493 galactic Peg Second-epoch detections are separated by 0.2" and 8.4 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 | 23:00:45.47 +16:08:38.5 (user input) | T | P | (position from user input) J-Ks=0.622+/-0.030 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:45.47 +16:08:38.5: 13.65 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:45.47 +16:08:38.5: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 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,2461231.8924,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.81 23:02:50.91 +14:49:04.3
87.49580 -40.46548 galactic Peg Second-epoch detections are separated by 2.0" and 8.4 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 | 23:02:50.91 +14:49:04.3 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.760+/-0.030 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:50.91 +14:49:04.3: 13.94 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:50.91 +14:49:04.3: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 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,2461231.8924,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.16 23:00:04.55 +15:49:54.1
87.46706 -39.25128 galactic Peg Second-epoch detections are separated by 1.5" and 8.3 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 | 23:00:04.55 +15:49:54.1 (user input) | T | P | (position from user input) J-Ks=0.461+/-0.032 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:04.55 +15:49:54.1: 14.14 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:04.55 +15:49:54.1: 14.21 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
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,2461231.8924,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.21 23:01:50.62 +14:20:21.2
86.88708 -40.73861 galactic Peg Second-epoch detections are separated by 0.4" and 8.4 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 | 23:01:50.62 +14:20:21.2 (user input) | T | P | (position from user input) J-Ks=0.504+/-0.032 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:50.62 +14:20:21.2: 14.17 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:50.62 +14:20:21.2: 14.21 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.06
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,2461231.8924,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 12.97 23:02:31.57 +14:16:39.7
87.02713 -40.87962 galactic Peg Second-epoch detections are separated by 0.8" and 8.5 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 | 23:02:31.57 +14:16:39.7 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.522+/-0.028 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:31.57 +14:16:39.7: 13.92 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:31.57 +14:16:39.7: 13.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461231.8924,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.97CV 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 10.3924 2461231.8924 12.65 23:03:02.20 +11:55:36.9
85.44236 -42.91695 galactic Peg Second-epoch detections are separated by 0.8" and 8.5 pix
The object was found in VSX 1" CSS_J230302.2+115538
Type: EW
# Max. Min./Amp. JD0 Period
13.360 CV Y 0.530 CV 0.423090000000 G3
The object was not found in astcheck.
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:02.20 +11:55:36.9: 13.65 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:02.20 +11:55:36.9: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 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
CSS_J230302.2+115538,2461231.8924,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CSS_J230302.2+115538 20260710.3924 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.84 23:05:39.30 +18:18:17.0
90.56608 -37.83026 galactic Peg Second-epoch detections are separated by 1.1" and 8.4 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 | 23:05:39.30 +18:18:17.0 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.605+/-0.029 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:39.30 +18:18:17.0: 13.77 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:39.30 +18:18:17.0: 13.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461231.8924,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.61 23:01:09.51 +14:39:25.9
86.92972 -40.38146 galactic Peg Second-epoch detections are separated by 1.4" and 8.6 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 | 23:01:09.51 +14:39:25.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.258+/-0.032 (F)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:09.51 +14:39:25.9: 13.44 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:09.51 +14:39:25.9: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 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,2461231.8924,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.99 22:59:52.75 +15:33:52.0
87.22955 -39.45111 galactic Peg Second-epoch detections are separated by 0.3" and 8.3 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 | 22:59:52.75 +15:33:52.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:52.75 +15:33:52.0: 13.90 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:52.75 +15:33:52.0: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.12 23:04:29.81 +14:05:08.5
87.42578 -41.29764 galactic Peg Second-epoch detections are separated by 0.4" and 8.3 pix
The object was found in VSX 2" ASASSN-V J230429.71+140510.1
Type: ROT
# Max. Min./Amp. JD0 Period
14.250 V 14.370 V 2458366.00500 1.228940000000
The object was not found in astcheck.
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:29.81 +14:05:08.5: 14.02 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:29.81 +14:05:08.5: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.08 +/- 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
ASASSN-V J230429.71+140510.1,2461231.8924,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J230429.71+140510.1 20260710.3924 13.12CV 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 10.3924 2461231.8924 12.80 23:00:43.35 +14:53:37.0
86.98104 -40.12560 galactic Peg Second-epoch detections are separated by 1.2" and 8.5 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 | 23:00:43.35 +14:53:37.0 (user input) | T | P | (position from user input) J-Ks=0.449+/-0.029 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:43.35 +14:53:37.0: 13.77 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:43.35 +14:53:37.0: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461231.8924,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.77 23:00:36.23 +16:00:51.6
87.73160 -39.16494 galactic Peg Second-epoch detections are separated by 1.1" and 8.4 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 | 23:00:36.23 +16:00:51.6 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.030 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:36.23 +16:00:51.6: 13.79 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:36.23 +16:00:51.6: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 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,2461231.8924,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.87 23:03:02.14 +14:56:31.7
87.63308 -40.38443 galactic Peg Second-epoch detections are separated by 1.2" and 8.6 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 | 23:03:02.14 +14:56:31.7 (user input) | T | P | (position from user input) J-Ks=0.387+/-0.031 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:02.14 +14:56:31.7: 13.76 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:02.14 +14:56:31.7: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.88 23:16:33.75 +12:43:46.2
89.89414 -43.97215 galactic Peg Second-epoch detections are separated by 0.9" and 8.5 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 | 23:16:33.75 +12:43:46.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.658+/-0.027 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:16:33.75 +12:43:46.2: 13.78 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:16:33.75 +12:43:46.2: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.85 +/- 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,2461231.8924,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.86 23:05:43.34 +13:13:46.8
87.15088 -42.18045 galactic Peg Second-epoch detections are separated by 0.4" and 8.5 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 | 23:05:43.34 +13:13:46.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.370+/-0.030 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:43.34 +13:13:46.8: 13.76 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:43.34 +13:13:46.8: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461231.8924,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.86CV 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 10.3924 2461231.8924 13.18 23:05:52.43 +18:18:10.0
90.62175 -37.85799 galactic Peg Second-epoch detections are separated by 3.9" and 8.2 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 | 23:05:52.43 +18:18:10.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.383+/-0.032 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:52.43 +18:18:10.0: 14.22 +/- 0.09 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:52.43 +18:18:10.0: 14.32 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.07
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,2461231.8924,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 13.03 22:59:04.99 +16:00:19.9
87.32828 -38.97637 galactic Peg Second-epoch detections are separated by 2.2" and 8.7 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 | 22:59:04.99 +16:00:19.9 (user input) | T | P | (position from user input) J-Ks=0.490+/-0.033 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:04.99 +16:00:19.9: 14.01 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:04.99 +16:00:19.9: 14.07 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.04 +/- 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,2461231.8924,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 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 10.3924 2461231.8924 12.72 23:00:55.83 +15:00:03.1
87.11202 -40.06245 galactic Peg Second-epoch detections are separated by 0.2" and 8.4 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 | 23:00:55.83 +15:00:03.1 (user input) | T | P | (position from user input) J-Ks=0.491+/-0.028 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:55.83 +15:00:03.1: 13.59 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:55.83 +15:00:03.1: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 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,2461231.8924,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 13.07 23:04:23.51 +13:44:31.0
87.15206 -41.57460 galactic Peg Second-epoch detections are separated by 1.1" and 8.5 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 | 23:04:23.51 +13:44:31.0 (user input) | T | P | (position from user input) J-Ks=0.461+/-0.030 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:23.51 +13:44:31.0: 14.01 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:23.51 +13:44:31.0: 14.09 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.05 +/- 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,2461231.8924,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 13.07CV 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 10.3924 2461231.8924 12.55 23:06:59.17 +11:22:44.1
86.14140 -43.90568 galactic Peg Second-epoch detections are separated by 0.5" and 8.5 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 | 23:06:59.17 +11:22:44.1 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.285+/-0.039 (F)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:59.17 +11:22:44.1: 13.45 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:59.17 +11:22:44.1: 13.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.50 +/- 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,2461231.8924,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.81 23:17:11.62 +12:49:26.8
90.14500 -43.96629 galactic Peg Second-epoch detections are separated by 1.5" and 8.7 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 | 23:17:11.62 +12:49:26.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.261+/-0.032 (F)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:11.62 +12:49:26.8: 13.78 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:11.62 +12:49:26.8: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461231.8924,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.70 22:59:17.80 +16:08:08.4
87.47390 -38.89430 galactic Peg Second-epoch detections are separated by 0.7" and 8.4 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 | 22:59:17.80 +16:08:08.4 (user input) | T | P | (position from user input) J-Ks=0.483+/-0.031 (K)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:17.80 +16:08:08.4: 13.61 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:17.80 +16:08:08.4: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461231.8924,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.70 23:00:20.36 +16:01:11.7
87.66617 -39.12627 galactic Peg Second-epoch detections are separated by 0.7" and 8.4 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 | 23:00:20.36 +16:01:11.7 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.030 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:20.36 +16:01:11.7: 13.59 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:20.36 +16:01:11.7: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 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,2461231.8924,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3924 2461231.8924 12.55 22:59:54.31 +16:08:20.0
87.63466 -38.96996 galactic Peg Second-epoch detections are separated by 1.1" and 8.4 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 | 22:59:54.31 +16:08:20.0 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.027 (G)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:54.31 +16:08:20.0: 13.42 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:54.31 +16:08:20.0: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8924,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3924 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461203.92142735 12.06.2026 10:06:41.323 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
First image: 2461203.92142735 12.06.2026 10:06:41.323 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Last image: 2461231.89266069 10.07.2026 09:25:15.884 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.66
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: 5 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): 6916
Objects passed selection criteria: 6913
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 5197.75
Average stars matched: 4989.75 (95.9983 %)
Memory usage VmPeak: 113216 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 07:06:00 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: 2461203.92142735 12.06.2026 10:06:41.323 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
First image: 2461203.92142735 12.06.2026 10:06:41.323 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Last image: 2461231.89266069 10.07.2026 09:25:15.884 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 133
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 21 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): 39003
Objects passed selection criteria: 38929
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 31164.8
Average stars matched: 30232 (97.007 %)
Memory usage VmPeak: 142828 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 07:08:01 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
SExtractor catalog cache: saved Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.cat to cache
SExtractor catalog cache: saved Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.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: 2461231.89207887
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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits exists and is non-empty
Saving wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits to local_wcs_cache/
'wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits' -> 'local_wcs_cache/wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits'
wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits exists and is non-empty
Saving wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits to local_wcs_cache/
'wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits' -> 'local_wcs_cache/wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits'
wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits exists and is non-empty
Saving wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits to local_wcs_cache/
'wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits' -> 'local_wcs_cache/wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits'
wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits exists and is non-empty
Saving wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits to local_wcs_cache/
'wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits' -> 'local_wcs_cache/wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits (1st reference image)
verification OK: wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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: 23:06:38.452 +14:00:51.18 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits (1st new image)
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:06:39.804 +14:00:12.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:38.452 +14:00:51.18
Second-epoch image center 23:06:39.804 +14:00:12.31
Angular distance between the image centers 0.0121 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits (2nd new image)
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:06:42.620 +14:00:42.25 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:38.452 +14:00:51.18
Second-epoch image center 23:06:42.620 +14:00:42.25
Angular distance between the image centers 0.0170 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 23:06:39.804 +14:00:12.31
Second-epoch second image center 23:06:42.620 +14:00:42.25
Angular distance between the image centers 0.01410 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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits &> /tmp/tmp.gZe7tvFWRe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits &> /tmp/tmp.JbzB4uAD6V
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits &> /tmp/tmp.GMi3QEcqbG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits &> /tmp/tmp.UIy3hd6hZd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits and wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits and wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
Found non-empty wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits and wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
The reference image (wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits) and catalog (wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat) found
'wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat' -> 'wcsmag.cat'
Read 7458 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3587 to 354.8627 deg, Dec +8.6419 to +19.2809 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 338.3587 to 354.8627 deg, Dec 8.6419 to 19.2809 deg
Loaded 5970 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): 4723 out of 4851 total matches.
Matched with Tycho-2 4851 out of 7458 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.619800
a=0.000000 b=1.000000 c=22.619800
From vast_summary.log: estimated ref. image limiting mag.: -7.66
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.96
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.96
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7458 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3587 to 354.8627 deg, Dec +8.6419 to +19.2809 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 338.3587 to 354.8627 deg, Dec 8.6419 to 19.2809 deg
Loaded 5970 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): 4723 out of 4851 total matches.
Matched with Tycho-2 4851 out of 7458 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits:
Forced-photometry filter: calibrated wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits -> calib.txt_param_ref_wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits (aperture=6.4)
Read 7660 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4285 to 355.2030 deg, Dec +8.2117 to +19.5193 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 338.4285 to 355.2030 deg, Dec 8.2117 to 19.5193 deg
Loaded 6456 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): 4837 out of 4961 total matches.
Matched with Tycho-2 4961 out of 7660 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits:
Forced-photometry filter: calibrated wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits -> calib.txt_param_ref_wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits (aperture=6.3)
____ 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:
2.3 pix Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
2.5 pix Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
2.7 pix fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
2.7 pix fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
2.3 pix wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
2.5 pix wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Limiting magnitude estimates:
15.0 mag. Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
14.9 mag. Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
12.9 mag. fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
13.1 mag. fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gZe7tvFWRe (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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits' -> 'wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WCS-calibrated image found: wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Checking if the catalog wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WCS catalog name: wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=405, bad_region=0, passed=7458
Got 7458 stars (including 7045 good ones) from the SExtractor catalog wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
util/solve_plate_with_UCAC5 got 7458 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits N_match=969 sigma_overall_arcsec=0.513 sigma_q1_arcsec=0.414 sigma_q2_arcsec=0.533 sigma_q3_arcsec=0.568 sigma_q4_arcsec=0.586 n_q1=240 n_q2=249 n_q3=257 n_q4=223 worst_quadrant_to_overall_ratio=1.142
The image catalog is written to wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits -region wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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.JbzB4uAD6V (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.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-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits' -> 'wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WCS-calibrated image found: wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Checking if the catalog wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WCS catalog name: wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=367, bad_region=0, passed=7660
Got 7660 stars (including 7285 good ones) from the SExtractor catalog wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat
util/solve_plate_with_UCAC5 got 7660 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 7536 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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 7536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 7536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits N_match=968 sigma_overall_arcsec=0.313 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.323 sigma_q3_arcsec=0.301 sigma_q4_arcsec=0.272 n_q1=257 n_q2=230 n_q3=276 n_q4=205 worst_quadrant_to_overall_ratio=1.076
The image catalog is written to wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits -region wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.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.GMi3QEcqbG (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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
Checking if the catalog wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
WCS catalog name: wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=95, bad_region=0, passed=2855
Got 2855 stars (including 2756 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat
util/solve_plate_with_UCAC5 got 2855 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 2752 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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 2749 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 2749 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 965 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits N_match=965 sigma_overall_arcsec=0.344 sigma_q1_arcsec=0.384 sigma_q2_arcsec=0.401 sigma_q3_arcsec=0.281 sigma_q4_arcsec=0.316 n_q1=249 n_q2=240 n_q3=286 n_q4=190 worst_quadrant_to_overall_ratio=1.164
The image catalog is written to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits -region wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.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.UIy3hd6hZd (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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
Checking if the catalog wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
WCS catalog name: wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=99, bad_region=0, passed=2928
Got 2928 stars (including 2827 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat
util/solve_plate_with_UCAC5 got 2928 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 2762 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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 2760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 2760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits N_match=966 sigma_overall_arcsec=0.364 sigma_q1_arcsec=0.442 sigma_q2_arcsec=0.395 sigma_q3_arcsec=0.336 sigma_q4_arcsec=0.324 n_q1=214 n_q2=273 n_q3=271 n_q4=208 worst_quadrant_to_overall_ratio=1.212
The image catalog is written to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits -region wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits sigma_overall=0.513 worst_q_ratio=1.142
ref2=Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits sigma_overall=0.313 worst_q_ratio=1.076
new1=fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits sigma_overall=0.344 worst_q_ratio=1.164
new2=fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits sigma_overall=0.364 worst_q_ratio=1.212
reference average sigma_overall=0.413 worst_q_ratio=1.109
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287_astrometric_residuals.png (969 matched stars from wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366_astrometric_residuals.png (968 matched stars from wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366_astrometric_residuals.png (965 matched stars from wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367_astrometric_residuals.png (966 matched stars from wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits'
Saving fully-calibrated image wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits'
Preparing the HTML report for the field Peg-10-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Peg-10-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
SExtractor catalog cache: saved Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.cat to cache
SExtractor catalog cache: saved Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Creating symlink local_wcs_cache/wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits exists and is non-empty
wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits exists and is non-empty
wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits exists and is non-empty
wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits (1st reference image)
verification OK: wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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: 23:06:38.452 +14:00:51.18 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits (1st new image)
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:06:39.804 +14:00:12.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:38.452 +14:00:51.18
Second-epoch image center 23:06:39.804 +14:00:12.31
Angular distance between the image centers 0.0121 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits (2nd new image)
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:06:42.620 +14:00:42.25 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:38.452 +14:00:51.18
Second-epoch image center 23:06:42.620 +14:00:42.25
Angular distance between the image centers 0.0170 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 23:06:39.804 +14:00:12.31
Second-epoch second image center 23:06:42.620 +14:00:42.25
Angular distance between the image centers 0.01410 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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits &> /tmp/tmp.qStuaTsLV9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits &> /tmp/tmp.GZ1I2jaVjL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits &> /tmp/tmp.fGxTYDQ7bw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits &> /tmp/tmp.teilbkUmup
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits and wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits and wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
Found non-empty wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits and wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
The reference image (wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits) and catalog (wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat) found
'wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat' -> 'wcsmag.cat'
Read 44707 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3587 to 354.8627 deg, Dec +8.6411 to +19.2831 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 338.3587 to 354.8627 deg, Dec 8.6411 to 19.2831 deg
Loaded 5972 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): 4687 out of 5110 total matches.
Matched with Tycho-2 5110 out of 44707 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.488600
a=0.000000 b=1.000000 c=22.488600
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.13
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.13
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 44707 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3587 to 354.8627 deg, Dec +8.6411 to +19.2831 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 338.3587 to 354.8627 deg, Dec 8.6411 to 19.2831 deg
Loaded 5972 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): 4687 out of 5110 total matches.
Matched with Tycho-2 5110 out of 44707 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits:
Forced-photometry filter: calibrated wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits -> calib.txt_param_ref_wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits (aperture=4.9)
Read 42031 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4279 to 355.2152 deg, Dec +8.2029 to +19.5229 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 338.4279 to 355.2152 deg, Dec 8.2029 to 19.5229 deg
Loaded 6473 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): 4800 out of 5169 total matches.
Matched with Tycho-2 5169 out of 42031 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits:
Forced-photometry filter: calibrated wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits -> calib.txt_param_ref_wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits (aperture=5.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 127 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
2.4 pix Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
2.5 pix fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
2.5 pix fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
2.1 pix wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
2.4 pix wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Limiting magnitude estimates:
15.1 mag. Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
15.0 mag. Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
13.5 mag. fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
13.7 mag. fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 13.3 (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.qStuaTsLV9 (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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits' -> 'wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WCS-calibrated image found: wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Checking if the catalog wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WCS catalog name: wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2139, bad_region=0, passed=44695
Got 44695 stars (including 42494 good ones) from the SExtractor catalog wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
util/solve_plate_with_UCAC5 got 44695 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 44346 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 44345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 44345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits N_match=971 sigma_overall_arcsec=0.518 sigma_q1_arcsec=0.412 sigma_q2_arcsec=0.545 sigma_q3_arcsec=0.553 sigma_q4_arcsec=0.588 n_q1=236 n_q2=247 n_q3=257 n_q4=231 worst_quadrant_to_overall_ratio=1.135
The image catalog is written to wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits -region wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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.GZ1I2jaVjL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.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-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits' -> 'wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WCS-calibrated image found: wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Checking if the catalog wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WCS catalog name: wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1612, bad_region=2, passed=42025
Got 42025 stars (including 40353 good ones) from the SExtractor catalog wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat
util/solve_plate_with_UCAC5 got 42025 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 41532 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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 41532 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 41532 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 968 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits N_match=968 sigma_overall_arcsec=0.313 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.343 sigma_q3_arcsec=0.297 sigma_q4_arcsec=0.280 n_q1=250 n_q2=226 n_q3=281 n_q4=211 worst_quadrant_to_overall_ratio=1.095
The image catalog is written to wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits -region wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.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.fGxTYDQ7bw (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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
Checking if the catalog wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
WCS catalog name: wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=468, bad_region=5, passed=19232
Got 19232 stars (including 18735 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat
util/solve_plate_with_UCAC5 got 19232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 18554 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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 18555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 18556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits N_match=965 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.363 sigma_q2_arcsec=0.414 sigma_q3_arcsec=0.294 sigma_q4_arcsec=0.338 n_q1=241 n_q2=241 n_q3=290 n_q4=193 worst_quadrant_to_overall_ratio=1.181
The image catalog is written to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits -region wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.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.teilbkUmup (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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
Checking if the catalog wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
WCS catalog name: wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=450, bad_region=7, passed=19506
Got 19506 stars (including 19022 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat
util/solve_plate_with_UCAC5 got 19506 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 18594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 18595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 18595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 963 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits N_match=963 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.435 sigma_q2_arcsec=0.355 sigma_q3_arcsec=0.318 sigma_q4_arcsec=0.288 n_q1=206 n_q2=270 n_q3=275 n_q4=212 worst_quadrant_to_overall_ratio=1.236
The image catalog is written to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Peg-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits -region wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.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-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-24-25_20.00sec_-0.00C_LIGHTs_0366.fits
Saving fully-calibrated image wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.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-10-Q1b1x1_042549_TTUQ1b1x1_538146_CluV6N9Z/wcs_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367.fits
Preparing the HTML report for the field Peg-10-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:12:50.64 +16:03:07.6: 13.65 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:58.72 +12:13:27.1: 13.89 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:34.11 +12:12:01.4: 13.97 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:08:00.83 +13:46:20.7: 13.96 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:58:54.06 +16:08:49.6: 13.75 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:09:58.58 +11:17:00.9: 14.09 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:20:04.82 +12:48:09.4: 13.78 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:42.37 +14:44:07.7: 13.76 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:14.39 +11:21:56.6: 13.63 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:58:35.01 +11:21:44.7: 14.02 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:42.37 +14:44:07.7: 13.71 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:58:54.06 +16:08:49.6: 13.89 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:20:04.82 +12:48:09.4: 13.86 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:12:50.64 +16:03:07.6: 13.63 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:09:58.58 +11:17:00.9: 14.32 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:58.72 +12:13:27.1: 13.95 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:58:35.01 +11:21:44.7: 13.86 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:34.11 +12:12:01.4: 14.14 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:08:00.83 +13:46:20.7: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:14.39 +11:21:56.6: 13.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Forced photometry filter KEPT candidate at 23:00:42.37 +14:44:07.7: ref_mag=13.73 +/- 0.04 new_mean_mag=12.8092 delta=0.92 (need > 0.90)
Forced photometry filter KEPT candidate at 23:20:04.82 +12:48:09.4: ref_mag=13.81 +/- 0.04 new_mean_mag=12.8460 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 14.19 +/- 0.06
Forced photometry filter KEPT candidate at 22:58:54.06 +16:08:49.6: ref_mag=13.81 +/- 0.04 new_mean_mag=12.8298 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 23:12:50.64 +16:03:07.6: ref_mag=13.64 +/- 0.04 new_mean_mag=12.7269 delta=0.91 (need > 0.90)
Forced photometry reference-image weighted average: 14.04 +/- 0.05
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Forced photometry filter KEPT candidate at 23:17:58.72 +12:13:27.1: ref_mag=13.92 +/- 0.05 new_mean_mag=12.9183 delta=1.00 (need > 0.90)
Forced photometry filter KEPT candidate at 23:09:58.58 +11:17:00.9: ref_mag=14.19 +/- 0.06 new_mean_mag=13.1285 delta=1.06 (need > 0.90)
Forced photometry filter KEPT candidate at 23:17:34.11 +12:12:01.4: ref_mag=14.04 +/- 0.05 new_mean_mag=12.9958 delta=1.05 (need > 0.90)
Forced photometry reference-image weighted average: 14.04 +/- 0.05
Forced photometry filter REJECTED candidate at 22:58:35.01 +11:21:44.7: ref_mag=13.93 +/- 0.05 new_mean_mag=13.0351 delta=0.89 (need > 0.90)
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter KEPT candidate at 23:08:00.83 +13:46:20.7: ref_mag=14.04 +/- 0.05 new_mean_mag=13.0786 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 23:07:14.39 +11:21:56.6: ref_mag=13.74 +/- 0.04 new_mean_mag=12.7130 delta=1.02 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:11:12.86 +13:50:54.6: 14.01 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:11:12.86 +13:50:54.6: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.05
Forced photometry filter KEPT candidate at 23:11:12.86 +13:50:54.6: ref_mag=13.97 +/- 0.05 new_mean_mag=12.9108 delta=1.06 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:44.39 +15:45:04.8: 13.81 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:44.39 +15:45:04.8: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry filter KEPT candidate at 22:59:44.39 +15:45:04.8: ref_mag=13.78 +/- 0.04 new_mean_mag=12.8110 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:53.09 +12:10:55.2: 14.16 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:15:13.73 +13:06:20.8: 14.07 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:53.09 +12:10:55.2: 14.11 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.06
Forced photometry filter KEPT candidate at 23:07:53.09 +12:10:55.2: ref_mag=14.14 +/- 0.06 new_mean_mag=13.1307 delta=1.01 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:29.92 +13:59:59.0: 13.58 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:08:23.38 +11:28:53.8: 13.84 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:15:13.73 +13:06:20.8: 14.21 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.06
Forced photometry filter KEPT candidate at 23:15:13.73 +13:06:20.8: ref_mag=14.13 +/- 0.06 new_mean_mag=13.1379 delta=0.99 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:29.92 +13:59:59.0: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter REJECTED candidate at 23:01:29.92 +13:59:59.0: ref_mag=13.50 +/- 0.03 new_mean_mag=12.8278 delta=0.67 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:08:23.38 +11:28:53.8: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Forced photometry filter KEPT candidate at 23:08:23.38 +11:28:53.8: ref_mag=13.86 +/- 0.05 new_mean_mag=12.8360 delta=1.03 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:06.07 +11:41:50.9: 13.84 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:06.07 +11:41:50.9: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter KEPT candidate at 23:05:06.07 +11:41:50.9: ref_mag=13.79 +/- 0.04 new_mean_mag=12.7342 delta=1.06 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:14:50.89 +12:58:11.2: 13.99 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:32.47 +14:57:25.6: 13.87 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:50.55 +14:18:35.0: 14.02 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:45.71 +17:34:37.2: 13.86 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:14:50.89 +12:58:11.2: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.05
Forced photometry filter KEPT candidate at 23:14:50.89 +12:58:11.2: ref_mag=13.99 +/- 0.05 new_mean_mag=13.0412 delta=0.95 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:05.75 +14:16:47.0: 13.84 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:32.47 +14:57:25.6: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Forced photometry filter KEPT candidate at 23:00:32.47 +14:57:25.6: ref_mag=13.82 +/- 0.04 new_mean_mag=12.8323 delta=0.99 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:50.55 +14:18:35.0: 14.04 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.05
Forced photometry filter KEPT candidate at 23:01:50.55 +14:18:35.0: ref_mag=14.03 +/- 0.05 new_mean_mag=13.0894 delta=0.94 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:45.71 +17:34:37.2: 13.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.05
Forced photometry filter KEPT candidate at 23:07:45.71 +17:34:37.2: ref_mag=13.88 +/- 0.05 new_mean_mag=12.7769 delta=1.10 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:05.75 +14:16:47.0: 14.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Forced photometry filter KEPT candidate at 23:01:05.75 +14:16:47.0: ref_mag=13.92 +/- 0.05 new_mean_mag=12.8641 delta=1.05 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:18:56.83 +13:04:28.4: 14.32 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:18:56.83 +13:04:28.4: 14.48 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.07
Forced photometry filter KEPT candidate at 23:18:56.83 +13:04:28.4: ref_mag=14.38 +/- 0.07 new_mean_mag=13.1235 delta=1.26 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:42.34 +11:09:09.0: 13.71 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:55.61 +12:52:43.6: 13.89 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:42.34 +11:09:09.0: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter KEPT candidate at 23:06:42.34 +11:09:09.0: ref_mag=13.76 +/- 0.04 new_mean_mag=12.7861 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:55.61 +12:52:43.6: 13.98 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Forced photometry filter KEPT candidate at 23:06:55.61 +12:52:43.6: ref_mag=13.93 +/- 0.05 new_mean_mag=12.9203 delta=1.01 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:09:04.36 +17:36:19.2: 13.89 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:09:04.36 +17:36:19.2: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Forced photometry filter KEPT candidate at 23:09:04.36 +17:36:19.2: ref_mag=13.91 +/- 0.05 new_mean_mag=12.9210 delta=0.99 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:14.21 +15:24:44.7: 14.10 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:52.26 +10:53:55.8: 14.12 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:14.21 +15:24:44.7: 14.11 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Forced photometry filter KEPT candidate at 23:01:14.21 +15:24:44.7: ref_mag=14.10 +/- 0.05 new_mean_mag=13.0892 delta=1.01 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:52.26 +10:53:55.8: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.05
Forced photometry filter KEPT candidate at 23:01:52.26 +10:53:55.8: ref_mag=14.04 +/- 0.05 new_mean_mag=13.0541 delta=0.98 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:52.45 +11:56:52.0: 14.19 +/- 0.09 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:08:58.10 +17:34:08.0: 13.75 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:52.45 +11:56:52.0: 14.22 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.07
Forced photometry filter KEPT candidate at 23:17:52.45 +11:56:52.0: ref_mag=14.21 +/- 0.07 new_mean_mag=13.1229 delta=1.08 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:46.29 +11:01:32.2: 14.32 +/- 0.09 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:18:45.66 +12:25:24.8: 13.76 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:08:58.10 +17:34:08.0: 13.86 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Forced photometry filter KEPT candidate at 23:08:58.10 +17:34:08.0: ref_mag=13.80 +/- 0.04 new_mean_mag=12.8863 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:46.29 +11:01:32.2: 14.39 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.07
Forced photometry filter KEPT candidate at 23:05:46.29 +11:01:32.2: ref_mag=14.35 +/- 0.07 new_mean_mag=13.0776 delta=1.27 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:18:45.66 +12:25:24.8: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Forced photometry filter KEPT candidate at 23:18:45.66 +12:25:24.8: ref_mag=13.84 +/- 0.05 new_mean_mag=12.8226 delta=1.02 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:19.84 +14:43:35.5: 13.63 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:19.84 +14:43:35.5: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter KEPT candidate at 23:00:19.84 +14:43:35.5: ref_mag=13.60 +/- 0.03 new_mean_mag=12.6961 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:16.87 +14:56:31.1: 13.77 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:16.87 +14:56:31.1: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter KEPT candidate at 23:03:16.87 +14:56:31.1: ref_mag=13.79 +/- 0.04 new_mean_mag=12.7787 delta=1.01 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:47.97 +11:00:11.3: 14.19 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:47.97 +11:00:11.3: 14.42 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.07
Forced photometry filter KEPT candidate at 23:06:47.97 +11:00:11.3: ref_mag=14.28 +/- 0.07 new_mean_mag=13.0894 delta=1.19 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:24.10 +14:33:40.5: 14.20 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:24.47 +13:57:43.4: 14.44 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:22.02 +13:38:01.7: 14.45 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:24.10 +14:33:40.5: 14.09 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.05
Forced photometry filter KEPT candidate at 23:04:24.10 +14:33:40.5: ref_mag=14.14 +/- 0.05 new_mean_mag=13.2042 delta=0.93 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:24.47 +13:57:43.4: 14.61 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.08
Forced photometry filter KEPT candidate at 23:04:24.47 +13:57:43.4: ref_mag=14.51 +/- 0.08 new_mean_mag=13.2691 delta=1.24 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:22.02 +13:38:01.7: 14.39 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.07
Forced photometry filter KEPT candidate at 23:07:22.02 +13:38:01.7: ref_mag=14.42 +/- 0.07 new_mean_mag=13.2237 delta=1.19 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:01.46 +12:17:11.4: 13.73 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:01.46 +12:17:11.4: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter KEPT candidate at 23:02:01.46 +12:17:11.4: ref_mag=13.69 +/- 0.04 new_mean_mag=12.6616 delta=1.03 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:13.34 +14:59:20.1: 13.72 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:09.91 +14:13:42.2: 13.61 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:13.34 +14:59:20.1: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Forced photometry filter KEPT candidate at 23:02:13.34 +14:59:20.1: ref_mag=13.71 +/- 0.04 new_mean_mag=12.7494 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:54.28 +14:43:08.2: 13.87 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:09.91 +14:13:42.2: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter KEPT candidate at 23:03:09.91 +14:13:42.2: ref_mag=13.55 +/- 0.03 new_mean_mag=12.6026 delta=0.95 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:54.28 +14:43:08.2: 13.80 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Forced photometry filter KEPT candidate at 23:00:54.28 +14:43:08.2: ref_mag=13.83 +/- 0.04 new_mean_mag=12.8881 delta=0.94 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:18:41.78 +12:38:04.4: 13.91 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:08.49 +11:26:23.2: 13.76 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:18:41.78 +12:38:04.4: 13.97 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Forced photometry filter KEPT candidate at 23:18:41.78 +12:38:04.4: ref_mag=13.94 +/- 0.05 new_mean_mag=12.9638 delta=0.98 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:08.49 +11:26:23.2: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry filter KEPT candidate at 23:05:08.49 +11:26:23.2: ref_mag=13.73 +/- 0.04 new_mean_mag=12.7332 delta=1.00 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:08:40.25 +11:21:43.8: 14.12 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:08:40.25 +11:21:43.8: 14.23 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Forced photometry filter KEPT candidate at 23:08:40.25 +11:21:43.8: ref_mag=14.17 +/- 0.06 new_mean_mag=12.9928 delta=1.18 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:40.74 +15:43:53.0: 14.10 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:19.41 +13:23:49.9: 13.70 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:40.74 +15:43:53.0: 14.08 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.05
Forced photometry filter KEPT candidate at 23:00:40.74 +15:43:53.0: ref_mag=14.09 +/- 0.05 new_mean_mag=13.0843 delta=1.01 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:19.41 +13:23:49.9: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Forced photometry filter KEPT candidate at 23:05:19.41 +13:23:49.9: ref_mag=13.77 +/- 0.04 new_mean_mag=12.8072 delta=0.96 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:48.90 +15:27:59.9: 13.87 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:48.90 +15:27:59.9: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.04
Forced photometry filter KEPT candidate at 22:59:48.90 +15:27:59.9: ref_mag=13.88 +/- 0.04 new_mean_mag=12.8708 delta=1.01 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:46.87 +11:22:52.7: 13.74 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:46.87 +11:22:52.7: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry filter KEPT candidate at 23:06:46.87 +11:22:52.7: ref_mag=13.81 +/- 0.04 new_mean_mag=12.8468 delta=0.96 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:01.74 +15:35:43.0: 13.87 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:01.74 +15:35:43.0: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry filter KEPT candidate at 23:01:01.74 +15:35:43.0: ref_mag=13.81 +/- 0.04 new_mean_mag=12.9060 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:18.73 +15:53:05.8: 13.02 +/- 0.03 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:18.73 +15:53:05.8: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter REJECTED candidate at 22:59:18.73 +15:53:05.8: ref_mag=13.01 +/- 0.02 new_mean_mag=12.2220 delta=0.79 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:18:17.97 +12:22:47.2: 13.89 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:18:17.97 +12:22:47.2: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
Forced photometry filter KEPT candidate at 23:18:17.97 +12:22:47.2: ref_mag=13.86 +/- 0.04 new_mean_mag=12.8968 delta=0.96 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:18.32 +17:51:38.8: 14.00 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:45.91 +12:45:36.3: 14.02 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:18.32 +17:51:38.8: 13.86 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Forced photometry filter KEPT candidate at 23:07:18.32 +17:51:38.8: ref_mag=13.92 +/- 0.05 new_mean_mag=12.9491 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:15:15.26 +12:49:55.7: 14.27 +/- 0.09 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:45.91 +12:45:36.3: 14.23 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.06
Forced photometry filter KEPT candidate at 23:17:45.91 +12:45:36.3: ref_mag=14.10 +/- 0.06 new_mean_mag=13.0071 delta=1.10 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:15:15.26 +12:49:55.7: 14.23 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.06
Forced photometry filter KEPT candidate at 23:15:15.26 +12:49:55.7: ref_mag=14.25 +/- 0.06 new_mean_mag=13.0824 delta=1.17 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:45.31 +14:33:39.5: 14.09 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:45.31 +14:33:39.5: 14.21 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.06
Forced photometry filter KEPT candidate at 23:03:45.31 +14:33:39.5: ref_mag=14.15 +/- 0.06 new_mean_mag=13.0738 delta=1.07 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:30.00 +16:08:12.8: 13.39 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:30.00 +16:08:12.8: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter KEPT candidate at 23:00:30.00 +16:08:12.8: ref_mag=13.33 +/- 0.03 new_mean_mag=12.3836 delta=0.95 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:52.53 +16:10:21.8: 13.85 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:52.53 +16:10:21.8: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.04
Forced photometry filter KEPT candidate at 22:59:52.53 +16:10:21.8: ref_mag=13.84 +/- 0.04 new_mean_mag=12.8942 delta=0.95 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:02.91 +14:12:59.7: 13.60 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:02.91 +14:12:59.7: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 23:03:02.91 +14:12:59.7: ref_mag=13.62 +/- 0.03 new_mean_mag=12.6870 delta=0.93 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:17.18 +18:02:21.2: 13.86 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:11.79 +14:28:14.6: 13.69 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:17.18 +18:02:21.2: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry filter KEPT candidate at 23:07:17.18 +18:02:21.2: ref_mag=13.81 +/- 0.04 new_mean_mag=12.7769 delta=1.03 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:11.79 +14:28:14.6: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Forced photometry filter KEPT candidate at 23:02:11.79 +14:28:14.6: ref_mag=13.72 +/- 0.04 new_mean_mag=12.6904 delta=1.03 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:18:44.12 +13:00:25.8: 14.04 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:18:44.12 +13:00:25.8: 14.15 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:19.21 +14:08:11.8: 14.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.06
Forced photometry filter KEPT candidate at 23:18:44.12 +13:00:25.8: ref_mag=14.09 +/- 0.06 new_mean_mag=13.1023 delta=0.99 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:19.21 +14:08:11.8: 14.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Forced photometry filter KEPT candidate at 23:03:19.21 +14:08:11.8: ref_mag=14.02 +/- 0.05 new_mean_mag=13.0745 delta=0.95 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:58.49 +14:45:06.4: 13.98 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:58.49 +14:45:06.4: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Forced photometry filter KEPT candidate at 23:00:58.49 +14:45:06.4: ref_mag=14.00 +/- 0.05 new_mean_mag=13.0071 delta=0.99 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:30.80 +11:58:02.0: 14.05 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:30.80 +11:58:02.0: 14.05 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.05
Forced photometry filter KEPT candidate at 23:02:30.80 +11:58:02.0: ref_mag=14.05 +/- 0.05 new_mean_mag=13.0392 delta=1.01 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:10.77 +13:48:44.9: 14.00 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:10.77 +13:48:44.9: 14.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.05
Forced photometry filter KEPT candidate at 23:04:10.77 +13:48:44.9: ref_mag=14.03 +/- 0.05 new_mean_mag=12.9461 delta=1.09 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:12.69 +15:13:32.4: 13.99 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:12.69 +15:13:32.4: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Forced photometry filter KEPT candidate at 23:00:12.69 +15:13:32.4: ref_mag=14.02 +/- 0.05 new_mean_mag=13.1087 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:15.94 +16:05:03.1: 13.56 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:15.94 +16:05:03.1: 13.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 22:59:15.94 +16:05:03.1: ref_mag=13.57 +/- 0.03 new_mean_mag=12.5516 delta=1.02 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:55.24 +15:48:04.2: 13.57 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:55.24 +15:48:04.2: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter KEPT candidate at 22:59:55.24 +15:48:04.2: ref_mag=13.49 +/- 0.03 new_mean_mag=12.5136 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:04.59 +15:03:00.7: 13.56 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:10.25 +13:39:06.9: 13.70 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:04.59 +15:03:00.7: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 23:00:04.59 +15:03:00.7: ref_mag=13.62 +/- 0.03 new_mean_mag=12.7123 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:10.25 +13:39:06.9: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter KEPT candidate at 23:04:10.25 +13:39:06.9: ref_mag=13.76 +/- 0.04 new_mean_mag=12.7269 delta=1.03 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:48.21 +16:14:59.9: 13.83 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:21.26 +14:36:49.4: 13.82 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:48.21 +16:14:59.9: 13.73 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry filter KEPT candidate at 23:00:48.21 +16:14:59.9: ref_mag=13.78 +/- 0.04 new_mean_mag=12.8036 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:21.26 +14:36:49.4: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Forced photometry filter KEPT candidate at 23:01:21.26 +14:36:49.4: ref_mag=13.83 +/- 0.04 new_mean_mag=12.8478 delta=0.98 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:20.07 +10:23:56.1: 13.72 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:20.07 +10:23:56.1: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Forced photometry filter REJECTED candidate at 23:04:20.07 +10:23:56.1: ref_mag=13.77 +/- 0.04 new_mean_mag=13.0277 delta=0.74 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:10.99 +14:14:21.7: 13.83 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:35.22 +10:57:19.2: 13.66 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:10.99 +14:14:21.7: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Forced photometry filter KEPT candidate at 23:02:10.99 +14:14:21.7: ref_mag=13.90 +/- 0.04 new_mean_mag=12.9146 delta=0.98 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:35.22 +10:57:19.2: 13.97 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter KEPT candidate at 23:07:35.22 +10:57:19.2: ref_mag=13.76 +/- 0.04 new_mean_mag=12.8013 delta=0.96 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:26.53 +15:59:30.1: 13.35 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:05.84 +14:04:41.9: 14.04 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:26.53 +15:59:30.1: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Forced photometry filter KEPT candidate at 22:59:26.53 +15:59:30.1: ref_mag=13.29 +/- 0.03 new_mean_mag=12.3051 delta=0.99 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:05.84 +14:04:41.9: 14.17 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Forced photometry filter KEPT candidate at 23:04:05.84 +14:04:41.9: ref_mag=14.10 +/- 0.05 new_mean_mag=13.1021 delta=1.00 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:18.91 +18:32:16.3: 13.83 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:18.91 +18:32:16.3: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter KEPT candidate at 23:05:18.91 +18:32:16.3: ref_mag=13.79 +/- 0.04 new_mean_mag=12.8637 delta=0.93 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:55.72 +15:00:15.3: 14.06 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:55.72 +15:00:15.3: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.05
Forced photometry filter KEPT candidate at 23:01:55.72 +15:00:15.3: ref_mag=14.06 +/- 0.05 new_mean_mag=13.0531 delta=1.01 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:42.15 +17:42:30.1: 13.97 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:42.15 +17:42:30.1: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.05
Forced photometry filter KEPT candidate at 23:06:42.15 +17:42:30.1: ref_mag=13.99 +/- 0.05 new_mean_mag=13.0037 delta=0.99 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:54.16 +18:42:43.7: 13.79 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:54.16 +18:42:43.7: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Forced photometry filter KEPT candidate at 23:05:54.16 +18:42:43.7: ref_mag=13.77 +/- 0.04 new_mean_mag=12.7697 delta=1.00 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:48.53 +12:03:14.7: 13.53 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:10.42 +11:31:12.2: 14.02 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:48.53 +12:03:14.7: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Forced photometry filter KEPT candidate at 23:02:48.53 +12:03:14.7: ref_mag=13.57 +/- 0.04 new_mean_mag=12.5888 delta=0.98 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:10.42 +11:31:12.2: 14.07 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.05
Forced photometry filter KEPT candidate at 23:06:10.42 +11:31:12.2: ref_mag=14.04 +/- 0.05 new_mean_mag=12.9352 delta=1.10 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:21:06.79 +13:09:57.9: 14.05 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:21.15 +11:40:30.1: 14.05 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:21:06.79 +13:09:57.9: 14.11 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.06
Forced photometry filter KEPT candidate at 23:21:06.79 +13:09:57.9: ref_mag=14.08 +/- 0.06 new_mean_mag=13.0370 delta=1.04 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:21.15 +11:40:30.1: 14.14 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.05
Forced photometry filter KEPT candidate at 23:05:21.15 +11:40:30.1: ref_mag=14.09 +/- 0.05 new_mean_mag=13.0608 delta=1.03 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:27.37 +14:57:37.5: 13.96 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:57.23 +12:59:28.5: 14.05 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:27.37 +14:57:37.5: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Forced photometry filter KEPT candidate at 23:01:27.37 +14:57:37.5: ref_mag=13.95 +/- 0.05 new_mean_mag=12.8727 delta=1.08 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:57.23 +12:59:28.5: 13.98 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.05
Forced photometry filter KEPT candidate at 23:17:57.23 +12:59:28.5: ref_mag=14.01 +/- 0.05 new_mean_mag=12.8853 delta=1.13 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:33.87 +17:59:32.8: 14.06 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:33.87 +17:59:32.8: 14.13 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.06
Forced photometry filter KEPT candidate at 23:07:33.87 +17:59:32.8: ref_mag=14.09 +/- 0.06 new_mean_mag=13.0677 delta=1.02 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:30.96 +15:39:09.4: 14.03 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:30.96 +15:39:09.4: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Forced photometry filter KEPT candidate at 23:00:30.96 +15:39:09.4: ref_mag=14.00 +/- 0.05 new_mean_mag=13.0136 delta=0.98 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:21.09 +14:34:02.4: 13.32 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:21.09 +14:34:02.4: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter KEPT candidate at 23:01:21.09 +14:34:02.4: ref_mag=13.36 +/- 0.03 new_mean_mag=12.4324 delta=0.93 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:31.40 +15:22:01.3: 13.95 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:31.40 +15:22:01.3: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Forced photometry filter KEPT candidate at 22:59:31.40 +15:22:01.3: ref_mag=13.95 +/- 0.05 new_mean_mag=13.0179 delta=0.93 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:11.53 +14:35:01.6: 13.96 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:11.92 +14:15:35.5: 13.96 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:11.53 +14:35:01.6: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 23:01:11.53 +14:35:01.6: ref_mag=13.94 +/- 0.04 new_mean_mag=12.9817 delta=0.96 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:11.92 +14:15:35.5: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Forced photometry filter KEPT candidate at 23:03:11.92 +14:15:35.5: ref_mag=13.93 +/- 0.05 new_mean_mag=13.0131 delta=0.92 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:10.79 +09:25:40.7: 13.37 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:19:12.77 +12:55:41.0: 13.81 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:10.79 +09:25:40.7: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter KEPT candidate at 23:03:10.79 +09:25:40.7: ref_mag=13.43 +/- 0.03 new_mean_mag=12.0071 delta=1.43 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:19:12.77 +12:55:41.0: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Forced photometry filter KEPT candidate at 23:19:12.77 +12:55:41.0: ref_mag=13.77 +/- 0.04 new_mean_mag=12.7216 delta=1.05 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:16:06.00 +12:54:53.4: 13.96 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:14.34 +12:17:48.8: 13.98 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:16:06.00 +12:54:53.4: 14.04 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Forced photometry filter KEPT candidate at 23:16:06.00 +12:54:53.4: ref_mag=14.00 +/- 0.05 new_mean_mag=12.8849 delta=1.11 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:14.34 +12:17:48.8: 13.97 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.05
Forced photometry filter KEPT candidate at 23:17:14.34 +12:17:48.8: ref_mag=13.97 +/- 0.05 new_mean_mag=12.9733 delta=1.00 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:07.99 +11:32:59.8: 13.48 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:12.99 +12:05:43.4: 13.94 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:07.99 +11:32:59.8: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry filter KEPT candidate at 23:05:07.99 +11:32:59.8: ref_mag=13.51 +/- 0.03 new_mean_mag=12.5528 delta=0.95 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:08:37.51 +18:53:35.1: 13.44 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:12.99 +12:05:43.4: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Forced photometry filter KEPT candidate at 23:03:12.99 +12:05:43.4: ref_mag=13.96 +/- 0.05 new_mean_mag=12.9605 delta=1.00 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:08:37.51 +18:53:35.1: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry filter KEPT candidate at 23:08:37.51 +18:53:35.1: ref_mag=13.48 +/- 0.03 new_mean_mag=12.5677 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:53.36 +11:30:55.2: 13.96 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:53.36 +11:30:55.2: 14.28 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.06
Forced photometry filter KEPT candidate at 23:04:53.36 +11:30:55.2: ref_mag=14.07 +/- 0.06 new_mean_mag=13.0412 delta=1.03 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:07:42.26 +12:03:28.9: 13.98 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:07:42.26 +12:03:28.9: 14.29 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.05
Forced photometry filter KEPT candidate at 23:07:42.26 +12:03:28.9: ref_mag=14.08 +/- 0.05 new_mean_mag=12.9744 delta=1.11 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:45.47 +16:08:38.5: 13.65 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:45.47 +16:08:38.5: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter KEPT candidate at 23:00:45.47 +16:08:38.5: ref_mag=13.65 +/- 0.04 new_mean_mag=12.6734 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:50.91 +14:49:04.3: 13.94 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:50.91 +14:49:04.3: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
Forced photometry filter KEPT candidate at 23:02:50.91 +14:49:04.3: ref_mag=13.86 +/- 0.04 new_mean_mag=12.8165 delta=1.05 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:04.55 +15:49:54.1: 14.14 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:50.62 +14:20:21.2: 14.17 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:04.55 +15:49:54.1: 14.21 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Forced photometry filter KEPT candidate at 23:00:04.55 +15:49:54.1: ref_mag=14.18 +/- 0.06 new_mean_mag=13.1572 delta=1.02 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:50.62 +14:20:21.2: 14.21 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.06
Forced photometry filter KEPT candidate at 23:01:50.62 +14:20:21.2: ref_mag=14.19 +/- 0.06 new_mean_mag=13.1791 delta=1.01 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:31.57 +14:16:39.7: 13.92 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:31.57 +14:16:39.7: 13.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter KEPT candidate at 23:02:31.57 +14:16:39.7: ref_mag=13.93 +/- 0.04 new_mean_mag=12.9770 delta=0.95 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:02.20 +11:55:36.9: 13.65 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:39.30 +18:18:17.0: 13.77 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:02.20 +11:55:36.9: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Forced photometry filter KEPT candidate at 23:03:02.20 +11:55:36.9: ref_mag=13.71 +/- 0.04 new_mean_mag=12.6228 delta=1.08 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:39.30 +18:18:17.0: 13.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Forced photometry filter KEPT candidate at 23:05:39.30 +18:18:17.0: ref_mag=13.72 +/- 0.04 new_mean_mag=12.7864 delta=0.94 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:01:09.51 +14:39:25.9: 13.44 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:01:09.51 +14:39:25.9: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry filter KEPT candidate at 23:01:09.51 +14:39:25.9: ref_mag=13.48 +/- 0.03 new_mean_mag=12.5662 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:52.75 +15:33:52.0: 13.90 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:52.75 +15:33:52.0: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.04
Forced photometry filter KEPT candidate at 22:59:52.75 +15:33:52.0: ref_mag=13.89 +/- 0.04 new_mean_mag=12.9820 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:29.81 +14:05:08.5: 14.02 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:29.81 +14:05:08.5: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.05
Forced photometry filter KEPT candidate at 23:04:29.81 +14:05:08.5: ref_mag=14.08 +/- 0.05 new_mean_mag=13.1071 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:43.35 +14:53:37.0: 13.77 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:36.23 +16:00:51.6: 13.79 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:43.35 +14:53:37.0: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter KEPT candidate at 23:00:43.35 +14:53:37.0: ref_mag=13.74 +/- 0.04 new_mean_mag=12.7825 delta=0.96 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:36.23 +16:00:51.6: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Forced photometry filter KEPT candidate at 23:00:36.23 +16:00:51.6: ref_mag=13.70 +/- 0.04 new_mean_mag=12.7439 delta=0.95 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:03:02.14 +14:56:31.7: 13.76 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:03:02.14 +14:56:31.7: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter KEPT candidate at 23:03:02.14 +14:56:31.7: ref_mag=13.76 +/- 0.04 new_mean_mag=12.8310 delta=0.93 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:16:33.75 +12:43:46.2: 13.78 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:16:33.75 +12:43:46.2: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Forced photometry filter KEPT candidate at 23:16:33.75 +12:43:46.2: ref_mag=13.85 +/- 0.04 new_mean_mag=12.8588 delta=0.99 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:43.34 +13:13:46.8: 13.76 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:05:52.43 +18:18:10.0: 14.22 +/- 0.09 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:43.34 +13:13:46.8: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter KEPT candidate at 23:05:43.34 +13:13:46.8: ref_mag=13.79 +/- 0.04 new_mean_mag=12.8618 delta=0.93 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:05:52.43 +18:18:10.0: 14.32 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.07
Forced photometry filter KEPT candidate at 23:05:52.43 +18:18:10.0: ref_mag=14.26 +/- 0.07 new_mean_mag=13.1193 delta=1.14 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:04.99 +16:00:19.9: 14.01 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:04.99 +16:00:19.9: 14.07 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.05
Forced photometry filter KEPT candidate at 22:59:04.99 +16:00:19.9: ref_mag=14.04 +/- 0.05 new_mean_mag=13.0200 delta=1.02 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:55.83 +15:00:03.1: 13.59 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:55.83 +15:00:03.1: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter KEPT candidate at 23:00:55.83 +15:00:03.1: ref_mag=13.60 +/- 0.03 new_mean_mag=12.6771 delta=0.92 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:04:23.51 +13:44:31.0: 14.01 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:04:23.51 +13:44:31.0: 14.09 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.05
Forced photometry filter KEPT candidate at 23:04:23.51 +13:44:31.0: ref_mag=14.05 +/- 0.05 new_mean_mag=13.0363 delta=1.01 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:06:59.17 +11:22:44.1: 13.45 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:06:59.17 +11:22:44.1: 13.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter KEPT candidate at 23:06:59.17 +11:22:44.1: ref_mag=13.50 +/- 0.03 new_mean_mag=12.5430 delta=0.96 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:17:11.62 +12:49:26.8: 13.78 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:17:11.62 +12:49:26.8: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry filter KEPT candidate at 23:17:11.62 +12:49:26.8: ref_mag=13.78 +/- 0.04 new_mean_mag=12.7929 delta=0.99 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:17.80 +16:08:08.4: 13.61 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:17.80 +16:08:08.4: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 22:59:17.80 +16:08:08.4: ref_mag=13.62 +/- 0.03 new_mean_mag=12.6482 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:00:20.36 +16:01:11.7: 13.59 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:00:20.36 +16:01:11.7: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter KEPT candidate at 23:00:20.36 +16:01:11.7: ref_mag=13.60 +/- 0.03 new_mean_mag=12.6905 delta=0.91 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 22:59:54.31 +16:08:20.0: 13.42 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 22:59:54.31 +16:08:20.0: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 22:59:54.31 +16:08:20.0: ref_mag=13.45 +/- 0.03 new_mean_mag=12.5249 delta=0.93 (need > 0.90)
Adding exclusion_list_local.txt__out02256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44611.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 156s
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: 61s
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Considering the candidate 15223_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 15223_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 23924_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 23924_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 42278_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 42278_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 09339_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
The candidate 09339_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367 did not pass the final checks
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Considering the candidate 12762_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 12762_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 09257_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 09257_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 12653_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 12653_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 42813_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 42813_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 08900_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 08900_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 19462_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 19462_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 19809_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 19809_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 43668_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 43668_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 12585_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 12585_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 16516_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 16516_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 20592_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
The candidate 20592_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367 did not pass the final checks
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Considering the candidate 09732_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 09732_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 10656_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 10656_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 15972_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 15972_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 24958_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 24958_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 21926_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 21926_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 37482_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 37482_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 21833_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 21833_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 16409_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 16409_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 08360_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 08360_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 15616_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 15616_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 37348_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 37348_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 32548_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 32548_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 07429_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 07429_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 11624_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 11624_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 37496_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 37496_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 07873_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 07873_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 13581_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 13581_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 23916_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 23916_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 24843_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 24843_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 07787_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 07787_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 23091_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 23091_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 20379_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 20379_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 18848_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 18848_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 13094_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 13094_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 25051_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 25051_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 21535_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 21535_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 23870_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 23870_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 14471_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 14471_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 09568_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 09568_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 09229_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 09229_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 43755_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 43755_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 17824_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 17824_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 44611_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 44611_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 09302_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 09302_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 44197_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 44197_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 43248_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
The candidate 43248_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367 did not pass the final checks
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Considering the candidate 13406_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 13406_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 36086_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 36086_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 15050_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 15050_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 15373_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 15373_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 23094_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 23094_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 42446_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 42446_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 42311_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 42311_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 21476_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 21476_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 35639_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 35639_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 22687_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 22687_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 16138_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 16138_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 21161_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 21161_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 23990_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 23990_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 11769_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 11769_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 19694_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 19694_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 33366_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 33366_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 42539_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 42539_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 29722_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 29722_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 34069_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 34069_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 18956_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 18956_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 42085_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 42085_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 23368_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 23368_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 05546_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
The candidate 05546_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367 did not pass the final checks
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Considering the candidate 21594_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 21594_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 07596_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 07596_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 42878_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 42878_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 20878_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 20878_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 28663_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 28663_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 25124_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 25124_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 36939_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 36939_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 27849_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 27849_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 09898_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 09898_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 12114_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 12114_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 16823_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 16823_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 10545_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 10545_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 24939_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 24939_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 16059_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 16059_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 35657_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 35657_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 43993_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 43993_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 23119_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 23119_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 29880_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 29880_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 23239_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 23239_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 21713_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 21713_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 02256_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 02256_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 15701_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 15701_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 15723_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 15723_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 13051_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 13051_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 10005_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 10005_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 12261_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 12261_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 27019_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 27019_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 09891_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 09891_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 12101_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 12101_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 42379_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 42379_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 24288_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 24288_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 43458_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 43458_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 22080_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 22080_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 21807_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 21807_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 11618_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 11618_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 34449_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 34449_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 23547_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 23547_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 44370_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 44370_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 20910_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 20910_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 24646_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 24646_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 42147_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 42147_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 24846_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 24846_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 14896_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 14896_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 17083_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 17083_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 34581_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 34581_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 42860_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 42860_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 25125_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 25125_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 19364_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 19364_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 09296_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 09296_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 15295_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 15295_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 42371_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 42371_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 42821_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 42821_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
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Considering the candidate 31775_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
Preparing report for the candidate 31775_fd_Peg-10-Q1b1x1_2026-07-10_04-25-15_20.00sec_0.00C_LIGHTs_0367
make_report_in_HTML.sh Phase 2 (HTML assembly): 9s
make_report_in_HTML.sh TOTAL: 226s
Prepared the HTML report for the field Peg-10-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:03:10.79 +09:25:40.7
23:01:52.26 +10:53:55.8
23:07:35.22 +10:57:19.2
23:06:47.97 +11:00:11.3
23:05:46.29 +11:01:32.2
23:06:42.34 +11:09:09.0
23:09:58.58 +11:17:00.9
23:08:40.25 +11:21:43.8
23:07:14.39 +11:21:56.6
23:06:59.17 +11:22:44.1
23:06:46.87 +11:22:52.7
23:05:08.49 +11:26:23.2
23:08:23.38 +11:28:53.8
23:04:53.36 +11:30:55.2
23:06:10.42 +11:31:12.2
23:05:07.99 +11:32:59.8
23:05:21.15 +11:40:30.1
23:05:06.07 +11:41:50.9
23:03:02.20 +11:55:36.9
23:17:52.45 +11:56:52.0
23:02:30.80 +11:58:02.0
23:07:42.26 +12:03:28.9
23:02:48.53 +12:03:14.7
23:03:12.99 +12:05:43.4
23:07:53.09 +12:10:55.2
23:17:34.11 +12:12:01.4
23:17:58.72 +12:13:27.1
23:17:14.34 +12:17:48.8
23:02:01.46 +12:17:11.4
23:18:17.97 +12:22:47.2
23:18:45.66 +12:25:24.8
23:18:41.78 +12:38:04.4
23:16:33.75 +12:43:46.2
23:17:45.91 +12:45:36.3
23:20:04.82 +12:48:09.4
23:17:11.62 +12:49:26.8
23:15:15.26 +12:49:55.7
23:06:55.61 +12:52:43.6
23:19:12.77 +12:55:41.0
23:16:06.00 +12:54:53.4
23:14:50.89 +12:58:11.2
23:17:57.23 +12:59:28.5
23:18:44.12 +13:00:25.8
23:18:56.83 +13:04:28.4
23:15:13.73 +13:06:20.8
23:21:06.79 +13:09:57.9
23:05:43.34 +13:13:46.8
23:05:19.41 +13:23:49.9
23:07:22.02 +13:38:01.7
23:04:10.25 +13:39:06.9
23:04:23.51 +13:44:31.0
23:08:00.83 +13:46:20.7
23:04:10.77 +13:48:44.9
23:11:12.86 +13:50:54.6
23:04:24.47 +13:57:43.4
23:04:05.84 +14:04:41.9
23:04:29.81 +14:05:08.5
23:03:19.21 +14:08:11.8
23:03:02.91 +14:12:59.7
23:03:09.91 +14:13:42.2
23:02:10.99 +14:14:21.7
23:03:11.92 +14:15:35.5
23:02:31.57 +14:16:39.7
23:01:05.75 +14:16:47.0
23:01:50.55 +14:18:35.0
23:01:50.62 +14:20:21.2
23:02:11.79 +14:28:14.6
23:04:24.10 +14:33:40.5
23:03:45.31 +14:33:39.5
23:01:21.09 +14:34:02.4
23:01:11.53 +14:35:01.6
23:01:21.26 +14:36:49.4
23:01:09.51 +14:39:25.9
23:00:54.28 +14:43:08.2
23:00:19.84 +14:43:35.5
23:00:42.37 +14:44:07.7
23:00:58.49 +14:45:06.4
23:02:50.91 +14:49:04.3
23:00:43.35 +14:53:37.0
23:03:16.87 +14:56:31.1
23:03:02.14 +14:56:31.7
23:01:27.37 +14:57:37.5
23:00:32.47 +14:57:25.6
23:02:13.34 +14:59:20.1
23:01:55.72 +15:00:15.3
23:00:55.83 +15:00:03.1
23:08:37.51 +18:53:35.1
23:05:54.16 +18:42:43.7
23:05:18.91 +18:32:16.3
22:59:55.24 +15:48:04.2
22:59:31.40 +15:22:01.3
22:59:54.31 +16:08:20.0
23:01:14.21 +15:24:44.7
23:00:12.69 +15:13:32.4
23:00:04.59 +15:03:00.7
23:05:39.30 +18:18:17.0
23:05:52.43 +18:18:10.0
23:07:17.18 +18:02:21.2
23:07:33.87 +17:59:32.8
23:07:18.32 +17:51:38.8
23:06:42.15 +17:42:30.1
23:09:04.36 +17:36:19.2
23:07:45.71 +17:34:37.2
23:08:58.10 +17:34:08.0
23:00:48.21 +16:14:59.9
23:00:36.23 +16:00:51.6
22:58:54.06 +16:08:49.6
22:59:52.53 +16:10:21.8
22:59:17.80 +16:08:08.4
23:00:45.47 +16:08:38.5
23:00:30.00 +16:08:12.8
22:59:15.94 +16:05:03.1
23:12:50.64 +16:03:07.6
23:00:20.36 +16:01:11.7
22:59:04.99 +16:00:19.9
22:59:26.53 +15:59:30.1
23:00:04.55 +15:49:54.1
22:59:44.39 +15:45:04.8
23:00:40.74 +15:43:53.0
23:00:30.96 +15:39:09.4
23:01:01.74 +15:35:43.0
22:59:52.75 +15:33:52.0
22:59:48.90 +15:27:59.9
########### Completed Peg-10-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
23:20:04.82 +12:48:09.4
23:00:42.37 +14:44:07.7
22:58:54.06 +16:08:49.6
23:17:58.72 +12:13:27.1
23:07:14.39 +11:21:56.6
23:17:34.11 +12:12:01.4
23:12:50.64 +16:03:07.6
23:09:58.58 +11:17:00.9
23:08:00.83 +13:46:20.7
23:11:12.86 +13:50:54.6
22:59:44.39 +15:45:04.8
23:07:53.09 +12:10:55.2
23:15:13.73 +13:06:20.8
23:08:23.38 +11:28:53.8
23:05:06.07 +11:41:50.9
23:14:50.89 +12:58:11.2
23:00:32.47 +14:57:25.6
23:01:50.55 +14:18:35.0
23:07:45.71 +17:34:37.2
23:01:05.75 +14:16:47.0
23:18:56.83 +13:04:28.4
23:06:42.34 +11:09:09.0
23:06:55.61 +12:52:43.6
23:09:04.36 +17:36:19.2
23:01:14.21 +15:24:44.7
23:01:52.26 +10:53:55.8
23:17:52.45 +11:56:52.0
23:08:58.10 +17:34:08.0
23:05:46.29 +11:01:32.2
23:18:45.66 +12:25:24.8
23:00:19.84 +14:43:35.5
23:03:16.87 +14:56:31.1
23:06:47.97 +11:00:11.3
23:04:24.10 +14:33:40.5
23:04:24.47 +13:57:43.4
23:07:22.02 +13:38:01.7
23:02:01.46 +12:17:11.4
23:02:13.34 +14:59:20.1
23:03:09.91 +14:13:42.2
23:00:54.28 +14:43:08.2
23:18:41.78 +12:38:04.4
23:05:08.49 +11:26:23.2
23:08:40.25 +11:21:43.8
23:00:40.74 +15:43:53.0
23:05:19.41 +13:23:49.9
22:59:48.90 +15:27:59.9
23:06:46.87 +11:22:52.7
23:01:01.74 +15:35:43.0
23:18:17.97 +12:22:47.2
23:07:18.32 +17:51:38.8
23:17:45.91 +12:45:36.3
23:15:15.26 +12:49:55.7
23:03:45.31 +14:33:39.5
23:00:30.00 +16:08:12.8
22:59:52.53 +16:10:21.8
23:03:02.91 +14:12:59.7
23:07:17.18 +18:02:21.2
23:02:11.79 +14:28:14.6
23:18:44.12 +13:00:25.8
23:03:19.21 +14:08:11.8
23:00:58.49 +14:45:06.4
23:02:30.80 +11:58:02.0
23:04:10.77 +13:48:44.9
23:00:12.69 +15:13:32.4
22:59:15.94 +16:05:03.1
22:59:55.24 +15:48:04.2
23:00:04.59 +15:03:00.7
23:04:10.25 +13:39:06.9
23:00:48.21 +16:14:59.9
23:01:21.26 +14:36:49.4
23:02:10.99 +14:14:21.7
23:07:35.22 +10:57:19.2
22:59:26.53 +15:59:30.1
23:04:05.84 +14:04:41.9
23:05:18.91 +18:32:16.3
23:01:55.72 +15:00:15.3
23:06:42.15 +17:42:30.1
23:05:54.16 +18:42:43.7
23:06:10.42 +11:31:12.2
23:02:48.53 +12:03:14.7
23:21:06.79 +13:09:57.9
23:05:21.15 +11:40:30.1
23:01:27.37 +14:57:37.5
23:17:57.23 +12:59:28.5
23:07:33.87 +17:59:32.8
23:00:30.96 +15:39:09.4
23:01:21.09 +14:34:02.4
22:59:31.40 +15:22:01.3
23:01:11.53 +14:35:01.6
23:03:11.92 +14:15:35.5
23:03:10.79 +09:25:40.7
23:19:12.77 +12:55:41.0
23:16:06.00 +12:54:53.4
23:17:14.34 +12:17:48.8
23:05:07.99 +11:32:59.8
23:03:12.99 +12:05:43.4
23:08:37.51 +18:53:35.1
23:04:53.36 +11:30:55.2
23:07:42.26 +12:03:28.9
23:00:45.47 +16:08:38.5
23:02:50.91 +14:49:04.3
23:00:04.55 +15:49:54.1
23:01:50.62 +14:20:21.2
23:02:31.57 +14:16:39.7
23:03:02.20 +11:55:36.9
23:05:39.30 +18:18:17.0
23:01:09.51 +14:39:25.9
22:59:52.75 +15:33:52.0
23:04:29.81 +14:05:08.5
23:00:43.35 +14:53:37.0
23:00:36.23 +16:00:51.6
23:03:02.14 +14:56:31.7
23:16:33.75 +12:43:46.2
23:05:43.34 +13:13:46.8
23:05:52.43 +18:18:10.0
22:59:04.99 +16:00:19.9
23:00:55.83 +15:00:03.1
23:04:23.51 +13:44:31.0
23:06:59.17 +11:22:44.1
23:17:11.62 +12:49:26.8
22:59:17.80 +16:08:08.4
23:00:20.36 +16:01:11.7
22:59:54.31 +16:08:20.0
###################################################################################
23:20:04.82 +12:48:09.4 -- not an asteroid (will add it to exclusion list)
23:00:42.37 +14:44:07.7 -- not an asteroid (will add it to exclusion list)
22:58:54.06 +16:08:49.6 -- not an asteroid (will add it to exclusion list)
23:17:58.72 +12:13:27.1 -- not an asteroid (will add it to exclusion list)
23:07:14.39 +11:21:56.6 -- not an asteroid (will add it to exclusion list)
23:17:34.11 +12:12:01.4 -- not an asteroid (will add it to exclusion list)
23:12:50.64 +16:03:07.6 -- not an asteroid (will add it to exclusion list)
23:09:58.58 +11:17:00.9 -- not an asteroid (will add it to exclusion list)
23:08:00.83 +13:46:20.7 -- not an asteroid (will add it to exclusion list)
23:11:12.86 +13:50:54.6 -- not an asteroid (will add it to exclusion list)
22:59:44.39 +15:45:04.8 -- not an asteroid (will add it to exclusion list)
23:07:53.09 +12:10:55.2 -- not an asteroid (will add it to exclusion list)
23:15:13.73 +13:06:20.8 -- not an asteroid (will add it to exclusion list)
23:08:23.38 +11:28:53.8 -- not an asteroid (will add it to exclusion list)
23:05:06.07 +11:41:50.9 -- not an asteroid (will add it to exclusion list)
23:14:50.89 +12:58:11.2 -- not an asteroid (will add it to exclusion list)
23:00:32.47 +14:57:25.6 -- not an asteroid (will add it to exclusion list)
23:01:50.55 +14:18:35.0 -- not an asteroid (will add it to exclusion list)
23:07:45.71 +17:34:37.2 -- not an asteroid (will add it to exclusion list)
23:01:05.75 +14:16:47.0 -- not an asteroid (will add it to exclusion list)
23:18:56.83 +13:04:28.4 -- not an asteroid (will add it to exclusion list)
23:06:42.34 +11:09:09.0 -- not an asteroid (will add it to exclusion list)
23:06:55.61 +12:52:43.6 -- not an asteroid (will add it to exclusion list)
23:09:04.36 +17:36:19.2 -- not an asteroid (will add it to exclusion list)
23:01:14.21 +15:24:44.7 -- not an asteroid (will add it to exclusion list)
23:01:52.26 +10:53:55.8 -- not an asteroid (will add it to exclusion list)
23:17:52.45 +11:56:52.0 -- not an asteroid (will add it to exclusion list)
23:08:58.10 +17:34:08.0 -- not an asteroid (will add it to exclusion list)
23:05:46.29 +11:01:32.2 -- not an asteroid (will add it to exclusion list)
23:18:45.66 +12:25:24.8 -- not an asteroid (will add it to exclusion list)
23:00:19.84 +14:43:35.5 -- not an asteroid (will add it to exclusion list)
23:03:16.87 +14:56:31.1 -- not an asteroid (will add it to exclusion list)
23:06:47.97 +11:00:11.3 -- not an asteroid (will add it to exclusion list)
23:04:24.10 +14:33:40.5 -- not an asteroid (will add it to exclusion list)
23:04:24.47 +13:57:43.4 -- not an asteroid (will add it to exclusion list)
23:07:22.02 +13:38:01.7 -- not an asteroid (will add it to exclusion list)
23:02:01.46 +12:17:11.4 -- not an asteroid (will add it to exclusion list)
23:02:13.34 +14:59:20.1 -- not an asteroid (will add it to exclusion list)
23:03:09.91 +14:13:42.2 -- not an asteroid (will add it to exclusion list)
23:00:54.28 +14:43:08.2 -- not an asteroid (will add it to exclusion list)
23:18:41.78 +12:38:04.4 -- not an asteroid (will add it to exclusion list)
23:05:08.49 +11:26:23.2 -- not an asteroid (will add it to exclusion list)
23:08:40.25 +11:21:43.8 -- not an asteroid (will add it to exclusion list)
23:00:40.74 +15:43:53.0 -- not an asteroid (will add it to exclusion list)
23:05:19.41 +13:23:49.9 -- not an asteroid (will add it to exclusion list)
22:59:48.90 +15:27:59.9 -- not an asteroid (will add it to exclusion list)
23:06:46.87 +11:22:52.7 -- not an asteroid (will add it to exclusion list)
23:01:01.74 +15:35:43.0 -- not an asteroid (will add it to exclusion list)
23:18:17.97 +12:22:47.2 -- not an asteroid (will add it to exclusion list)
23:07:18.32 +17:51:38.8 -- not an asteroid (will add it to exclusion list)
23:17:45.91 +12:45:36.3 -- not an asteroid (will add it to exclusion list)
23:15:15.26 +12:49:55.7 -- not an asteroid (will add it to exclusion list)
23:03:45.31 +14:33:39.5 -- not an asteroid (will add it to exclusion list)
23:00:30.00 +16:08:12.8 -- not an asteroid (will add it to exclusion list)
22:59:52.53 +16:10:21.8 -- not an asteroid (will add it to exclusion list)
23:03:02.91 +14:12:59.7 -- not an asteroid (will add it to exclusion list)
23:07:17.18 +18:02:21.2 -- not an asteroid (will add it to exclusion list)
23:02:11.79 +14:28:14.6 -- not an asteroid (will add it to exclusion list)
23:18:44.12 +13:00:25.8 -- not an asteroid (will add it to exclusion list)
23:03:19.21 +14:08:11.8 -- not an asteroid (will add it to exclusion list)
23:00:58.49 +14:45:06.4 -- not an asteroid (will add it to exclusion list)
23:02:30.80 +11:58:02.0 -- not an asteroid (will add it to exclusion list)
23:04:10.77 +13:48:44.9 -- not an asteroid (will add it to exclusion list)
23:00:12.69 +15:13:32.4 -- not an asteroid (will add it to exclusion list)
22:59:15.94 +16:05:03.1 -- not an asteroid (will add it to exclusion list)
22:59:55.24 +15:48:04.2 -- not an asteroid (will add it to exclusion list)
23:00:04.59 +15:03:00.7 -- not an asteroid (will add it to exclusion list)
23:04:10.25 +13:39:06.9 -- not an asteroid (will add it to exclusion list)
23:00:48.21 +16:14:59.9 -- not an asteroid (will add it to exclusion list)
23:01:21.26 +14:36:49.4 -- not an asteroid (will add it to exclusion list)
23:02:10.99 +14:14:21.7 -- not an asteroid (will add it to exclusion list)
23:07:35.22 +10:57:19.2 -- not an asteroid (will add it to exclusion list)
22:59:26.53 +15:59:30.1 -- not an asteroid (will add it to exclusion list)
23:04:05.84 +14:04:41.9 -- not an asteroid (will add it to exclusion list)
23:05:18.91 +18:32:16.3 -- not an asteroid (will add it to exclusion list)
23:01:55.72 +15:00:15.3 -- not an asteroid (will add it to exclusion list)
23:06:42.15 +17:42:30.1 -- not an asteroid (will add it to exclusion list)
23:05:54.16 +18:42:43.7 -- not an asteroid (will add it to exclusion list)
23:06:10.42 +11:31:12.2 -- not an asteroid (will add it to exclusion list)
23:02:48.53 +12:03:14.7 -- not an asteroid (will add it to exclusion list)
23:21:06.79 +13:09:57.9 -- not an asteroid (will add it to exclusion list)
23:05:21.15 +11:40:30.1 -- not an asteroid (will add it to exclusion list)
23:01:27.37 +14:57:37.5 -- not an asteroid (will add it to exclusion list)
23:17:57.23 +12:59:28.5 -- not an asteroid (will add it to exclusion list)
23:07:33.87 +17:59:32.8 -- not an asteroid (will add it to exclusion list)
23:00:30.96 +15:39:09.4 -- not an asteroid (will add it to exclusion list)
23:01:21.09 +14:34:02.4 -- not an asteroid (will add it to exclusion list)
22:59:31.40 +15:22:01.3 -- not an asteroid (will add it to exclusion list)
23:01:11.53 +14:35:01.6 -- not an asteroid (will add it to exclusion list)
23:03:11.92 +14:15:35.5 -- not an asteroid (will add it to exclusion list)
23:03:10.79 +09:25:40.7 -- asteroid (will NOT add it to exclusion list)
23:19:12.77 +12:55:41.0 -- not an asteroid (will add it to exclusion list)
23:16:06.00 +12:54:53.4 -- not an asteroid (will add it to exclusion list)
23:17:14.34 +12:17:48.8 -- not an asteroid (will add it to exclusion list)
23:05:07.99 +11:32:59.8 -- not an asteroid (will add it to exclusion list)
23:03:12.99 +12:05:43.4 -- not an asteroid (will add it to exclusion list)
23:08:37.51 +18:53:35.1 -- not an asteroid (will add it to exclusion list)
23:04:53.36 +11:30:55.2 -- not an asteroid (will add it to exclusion list)
23:07:42.26 +12:03:28.9 -- not an asteroid (will add it to exclusion list)
23:00:45.47 +16:08:38.5 -- not an asteroid (will add it to exclusion list)
23:02:50.91 +14:49:04.3 -- not an asteroid (will add it to exclusion list)
23:00:04.55 +15:49:54.1 -- not an asteroid (will add it to exclusion list)
23:01:50.62 +14:20:21.2 -- not an asteroid (will add it to exclusion list)
23:02:31.57 +14:16:39.7 -- not an asteroid (will add it to exclusion list)
23:03:02.20 +11:55:36.9 -- not an asteroid (will add it to exclusion list)
23:05:39.30 +18:18:17.0 -- not an asteroid (will add it to exclusion list)
23:01:09.51 +14:39:25.9 -- not an asteroid (will add it to exclusion list)
22:59:52.75 +15:33:52.0 -- not an asteroid (will add it to exclusion list)
23:04:29.81 +14:05:08.5 -- not an asteroid (will add it to exclusion list)
23:00:43.35 +14:53:37.0 -- not an asteroid (will add it to exclusion list)
23:00:36.23 +16:00:51.6 -- not an asteroid (will add it to exclusion list)
23:03:02.14 +14:56:31.7 -- not an asteroid (will add it to exclusion list)
23:16:33.75 +12:43:46.2 -- not an asteroid (will add it to exclusion list)
23:05:43.34 +13:13:46.8 -- not an asteroid (will add it to exclusion list)
23:05:52.43 +18:18:10.0 -- not an asteroid (will add it to exclusion list)
22:59:04.99 +16:00:19.9 -- not an asteroid (will add it to exclusion list)
23:00:55.83 +15:00:03.1 -- not an asteroid (will add it to exclusion list)
23:04:23.51 +13:44:31.0 -- not an asteroid (will add it to exclusion list)
23:06:59.17 +11:22:44.1 -- not an asteroid (will add it to exclusion list)
23:17:11.62 +12:49:26.8 -- not an asteroid (will add it to exclusion list)
22:59:17.80 +16:08:08.4 -- not an asteroid (will add it to exclusion list)
23:00:20.36 +16:01:11.7 -- not an asteroid (will add it to exclusion list)
22:59:54.31 +16:08:20.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
22:58:54.06 +16:08:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:04.99 +16:00:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:15.94 +16:05:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:17.80 +16:08:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:26.53 +15:59:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:31.40 +15:22:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:44.39 +15:45:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:48.90 +15:27:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:52.53 +16:10:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:52.75 +15:33:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:54.31 +16:08:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:55.24 +15:48:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:04.55 +15:49:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:04.59 +15:03:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:12.69 +15:13:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:19.84 +14:43:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:20.36 +16:01:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:30.00 +16:08:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:30.96 +15:39:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:32.47 +14:57:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:36.23 +16:00:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:40.74 +15:43:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:42.37 +14:44:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:43.35 +14:53:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:45.47 +16:08:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:48.21 +16:14:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:54.28 +14:43:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:55.83 +15:00:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:58.49 +14:45:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:01.74 +15:35:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:05.75 +14:16:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:09.51 +14:39:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:11.53 +14:35:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:14.21 +15:24:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:21.09 +14:34:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:21.26 +14:36:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:27.37 +14:57:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:50.55 +14:18:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:50.62 +14:20:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:52.26 +10:53:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:55.72 +15:00:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:01.46 +12:17:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:10.99 +14:14:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:11.79 +14:28:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:13.34 +14:59:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:30.80 +11:58:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:31.57 +14:16:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:48.53 +12:03:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:50.91 +14:49:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:02.14 +14:56:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:02.20 +11:55:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:02.91 +14:12:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:09.91 +14:13:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:11.92 +14:15:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:12.99 +12:05:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:16.87 +14:56:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:19.21 +14:08:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:45.31 +14:33:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:05.84 +14:04:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:10.25 +13:39:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:10.77 +13:48:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:23.51 +13:44:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:24.10 +14:33:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:24.47 +13:57:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:29.81 +14:05:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:53.36 +11:30:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:06.07 +11:41:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:07.99 +11:32:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:08.49 +11:26:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:18.91 +18:32:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:19.41 +13:23:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:21.15 +11:40:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:39.30 +18:18:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:43.34 +13:13:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:46.29 +11:01:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:52.43 +18:18:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:54.16 +18:42:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:10.42 +11:31:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:42.15 +17:42:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:42.34 +11:09:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:46.87 +11:22:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:47.97 +11:00:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:55.61 +12:52:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:59.17 +11:22:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:14.39 +11:21:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:17.18 +18:02:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:18.32 +17:51:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:22.02 +13:38:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:33.87 +17:59:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:35.22 +10:57:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:42.26 +12:03:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:45.71 +17:34:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:53.09 +12:10:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:00.83 +13:46:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:23.38 +11:28:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:37.51 +18:53:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:40.25 +11:21:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:58.10 +17:34:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:04.36 +17:36:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:58.58 +11:17:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:12.86 +13:50:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:50.64 +16:03:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:50.89 +12:58:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:13.73 +13:06:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:15.26 +12:49:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:06.00 +12:54:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:33.75 +12:43:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:11.62 +12:49:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:14.34 +12:17:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:34.11 +12:12:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:45.91 +12:45:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:52.45 +11:56:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:57.23 +12:59:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:58.72 +12:13:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:17.97 +12:22:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:41.78 +12:38:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:44.12 +13:00:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:45.66 +12:25:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:56.83 +13:04:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:12.77 +12:55:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:04.82 +12:48:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:06.79 +13:09:57.9 -- 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)
22:58:54.06 +16:08:49.6 -- not a known variable star
22:59:04.99 +16:00:19.9 -- not a known variable star
22:59:15.94 +16:05:03.1 -- not a known variable star
22:59:17.80 +16:08:08.4 -- not a known variable star
22:59:26.53 +15:59:30.1 -- not a known variable star
22:59:31.40 +15:22:01.3 -- not a known variable star
22:59:44.39 +15:45:04.8 -- not a known variable star
22:59:48.90 +15:27:59.9 -- not a known variable star
22:59:52.53 +16:10:21.8 -- a known variable star
22:59:52.75 +15:33:52.0 -- not a known variable star
22:59:54.31 +16:08:20.0 -- not a known variable star
22:59:55.24 +15:48:04.2 -- not a known variable star
23:00:04.55 +15:49:54.1 -- not a known variable star
23:00:04.59 +15:03:00.7 -- not a known variable star
23:00:12.69 +15:13:32.4 -- not a known variable star
23:00:19.84 +14:43:35.5 -- not a known variable star
23:00:20.36 +16:01:11.7 -- not a known variable star
23:00:30.00 +16:08:12.8 -- a known variable star
23:00:30.96 +15:39:09.4 -- not a known variable star
23:00:32.47 +14:57:25.6 -- not a known variable star
23:00:36.23 +16:00:51.6 -- not a known variable star
23:00:40.74 +15:43:53.0 -- not a known variable star
23:00:42.37 +14:44:07.7 -- not a known variable star
23:00:43.35 +14:53:37.0 -- not a known variable star
23:00:45.47 +16:08:38.5 -- not a known variable star
23:00:48.21 +16:14:59.9 -- not a known variable star
23:00:54.28 +14:43:08.2 -- a known variable star
23:00:55.83 +15:00:03.1 -- not a known variable star
23:00:58.49 +14:45:06.4 -- not a known variable star
23:01:01.74 +15:35:43.0 -- not a known variable star
23:01:05.75 +14:16:47.0 -- not a known variable star
23:01:09.51 +14:39:25.9 -- not a known variable star
23:01:11.53 +14:35:01.6 -- not a known variable star
23:01:14.21 +15:24:44.7 -- not a known variable star
23:01:21.09 +14:34:02.4 -- not a known variable star
23:01:21.26 +14:36:49.4 -- not a known variable star
23:01:27.37 +14:57:37.5 -- not a known variable star
23:01:50.55 +14:18:35.0 -- not a known variable star
23:01:50.62 +14:20:21.2 -- not a known variable star
23:01:52.26 +10:53:55.8 -- not a known variable star
23:01:55.72 +15:00:15.3 -- not a known variable star
23:02:01.46 +12:17:11.4 -- not a known variable star
23:02:10.99 +14:14:21.7 -- not a known variable star
23:02:11.79 +14:28:14.6 -- not a known variable star
23:02:13.34 +14:59:20.1 -- not a known variable star
23:02:30.80 +11:58:02.0 -- not a known variable star
23:02:31.57 +14:16:39.7 -- not a known variable star
23:02:48.53 +12:03:14.7 -- not a known variable star
23:02:50.91 +14:49:04.3 -- not a known variable star
23:03:02.14 +14:56:31.7 -- not a known variable star
23:03:02.20 +11:55:36.9 -- a known variable star
23:03:02.91 +14:12:59.7 -- not a known variable star
23:03:09.91 +14:13:42.2 -- not a known variable star
23:03:11.92 +14:15:35.5 -- not a known variable star
23:03:12.99 +12:05:43.4 -- not a known variable star
23:03:16.87 +14:56:31.1 -- not a known variable star
23:03:19.21 +14:08:11.8 -- not a known variable star
23:03:45.31 +14:33:39.5 -- not a known variable star
23:04:05.84 +14:04:41.9 -- not a known variable star
23:04:10.25 +13:39:06.9 -- not a known variable star
23:04:10.77 +13:48:44.9 -- not a known variable star
23:04:23.51 +13:44:31.0 -- not a known variable star
23:04:24.10 +14:33:40.5 -- not a known variable star
23:04:24.47 +13:57:43.4 -- a known variable star
23:04:29.81 +14:05:08.5 -- a known variable star
23:04:53.36 +11:30:55.2 -- not a known variable star
23:05:06.07 +11:41:50.9 -- not a known variable star
23:05:07.99 +11:32:59.8 -- not a known variable star
23:05:08.49 +11:26:23.2 -- not a known variable star
23:05:18.91 +18:32:16.3 -- not a known variable star
23:05:19.41 +13:23:49.9 -- not a known variable star
23:05:21.15 +11:40:30.1 -- not a known variable star
23:05:39.30 +18:18:17.0 -- not a known variable star
23:05:43.34 +13:13:46.8 -- not a known variable star
23:05:46.29 +11:01:32.2 -- not a known variable star
23:05:52.43 +18:18:10.0 -- not a known variable star
23:05:54.16 +18:42:43.7 -- not a known variable star
23:06:10.42 +11:31:12.2 -- not a known variable star
23:06:42.15 +17:42:30.1 -- not a known variable star
23:06:42.34 +11:09:09.0 -- not a known variable star
23:06:46.87 +11:22:52.7 -- not a known variable star
23:06:47.97 +11:00:11.3 -- not a known variable star
23:06:55.61 +12:52:43.6 -- not a known variable star
23:06:59.17 +11:22:44.1 -- not a known variable star
23:07:14.39 +11:21:56.6 -- not a known variable star
23:07:17.18 +18:02:21.2 -- not a known variable star
23:07:18.32 +17:51:38.8 -- not a known variable star
23:07:22.02 +13:38:01.7 -- not a known variable star
23:07:33.87 +17:59:32.8 -- not a known variable star
23:07:35.22 +10:57:19.2 -- not a known variable star
23:07:42.26 +12:03:28.9 -- not a known variable star
23:07:45.71 +17:34:37.2 -- not a known variable star
23:07:53.09 +12:10:55.2 -- not a known variable star
23:08:00.83 +13:46:20.7 -- not a known variable star
23:08:23.38 +11:28:53.8 -- not a known variable star
23:08:37.51 +18:53:35.1 -- not a known variable star
23:08:40.25 +11:21:43.8 -- not a known variable star
23:08:58.10 +17:34:08.0 -- not a known variable star
23:09:04.36 +17:36:19.2 -- not a known variable star
23:09:58.58 +11:17:00.9 -- not a known variable star
23:11:12.86 +13:50:54.6 -- a known variable star
23:12:50.64 +16:03:07.6 -- not a known variable star
23:14:50.89 +12:58:11.2 -- not a known variable star
23:15:13.73 +13:06:20.8 -- not a known variable star
23:15:15.26 +12:49:55.7 -- not a known variable star
23:16:06.00 +12:54:53.4 -- a known variable star
23:16:33.75 +12:43:46.2 -- not a known variable star
23:17:11.62 +12:49:26.8 -- not a known variable star
23:17:14.34 +12:17:48.8 -- not a known variable star
23:17:34.11 +12:12:01.4 -- not a known variable star
23:17:45.91 +12:45:36.3 -- a known variable star
23:17:52.45 +11:56:52.0 -- not a known variable star
23:17:57.23 +12:59:28.5 -- not a known variable star
23:17:58.72 +12:13:27.1 -- not a known variable star
23:18:17.97 +12:22:47.2 -- not a known variable star
23:18:41.78 +12:38:04.4 -- not a known variable star
23:18:44.12 +13:00:25.8 -- not a known variable star
23:18:45.66 +12:25:24.8 -- not a known variable star
23:18:56.83 +13:04:28.4 -- not a known variable star
23:19:12.77 +12:55:41.0 -- a known variable star
23:20:04.82 +12:48:09.4 -- not a known variable star
23:21:06.79 +13:09:57.9 -- not a known variable star
Found 112 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
122 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 122 (excluding asteroids and hot pixels, 112 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461231.89207887 -observatory V36
07:32:10.34 +17:07:55.6 Mercury (5.1mag)
10:11:49.35 +12:39:54.3 Venus (-4.1mag)
04:24:17.73 +21:25:31.3 Mars (1.3mag)
08:16:42.85 +20:11:21.9 Jupiter (-1.8mag)
00:55:51.18 +03:20:29.8 Saturn (0.7mag)
04:07:14.52 +20:45:04.7 Uranus (5.8mag)
00:17:01.49 +00:20:41.0 Neptune (7.8mag)
20:30:54.71 -23:18:01.7 Pluto (14.4mag)
03:14:17.01 +22:35:59.6 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 361 Jul 10 07:06 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461231.89207887:
08:16:50.02 +20:10:56.7 Io (6.1mag)
08:16:46.43 +20:11:10.3 Europa (6.3mag)
08:17:00.06 +20:10:19.5 Ganymede (5.6mag)
08:17:10.65 +20:09:39.1 Callisto (6.8mag)
08:15:14.22 +19:55:32.5 Himalia (15.7mag)
08:16:43.25 +20:11:21.2 Thebe (16.6mag)
08:14:35.55 +20:00:01.5 Elara (17.6mag)
08:20:15.15 +20:05:30.7 Pasiphae (17.8mag)
08:21:40.55 +20:16:27.2 Carme (19.0mag)
00:55:41.14 +03:20:20.2 Titan (8.5mag)
00:55:45.94 +03:20:32.1 Rhea (9.8mag)
00:55:20.42 +03:19:38.2 Iapetus (11.2mag)
00:56:00.26 +03:20:49.2 Hyperion (14.5mag)
00:55:51.84 +03:17:43.2 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 07:06 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.89207887:
17:46:01.89 -32:57:33.8 JWST
16:21:02.63 +47:28:05.5 Chandra
04:59:09.97 +48:15:38.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 07:06 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.89207887 -observatory V36
02:36:19.64 +14:25:59.5 17.9mag P/1996 R2 (Lagerkvist)
18:17:54.44 -34:21:49.4 13.7mag P/2010 H2 (Vales)
06:25:42.93 -68:08:25.3 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:49.23 +32:26:51.6 17.6mag C/2017 K2 (PANSTARRS)
17:03:06.25 +16:02:53.6 18.0mag C/2021 G2 (ATLAS)
01:48:02.17 +08:18:11.0 15.4mag P/2021 N1 (ZTF)
22:59:30.42 +32:17:08.0 17.3mag C/2022 E2 (ATLAS)
06:12:26.77 +26:55:33.5 16.7mag C/2022 N2 (PANSTARRS)
09:55:33.04 +29:46:44.7 16.8mag C/2022 QE78 (ATLAS)
09:09:45.69 +05:00:00.1 17.8mag C/2022 R6 (PANSTARRS)
18:07:11.58 +21:17:32.4 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:34.97 -11:23:19.2 17.7mag P/2023 B1 (PANSTARRS)
21:49:11.14 +67:37:16.2 17.8mag C/2023 H5 (Lemmon)
16:30:48.29 -10:04:56.7 13.9mag C/2023 R1 (PANSTARRS)
08:00:43.26 +65:42:38.2 17.9mag C/2024 A1 (ATLAS)
07:32:52.09 +30:00:19.6 14.6mag C/2024 E1 (Wierzchos)
15:16:18.38 +15:19:46.0 17.5mag C/2024 G6 (ATLAS)
19:41:15.48 +39:24:03.7 13.8mag C/2024 J3 (ATLAS)
21:47:32.47 +46:00:33.9 17.8mag C/2024 R4 (PANSTARRS)
04:49:40.66 -13:47:38.6 15.7mag C/2024 T5 (ATLAS)
06:34:36.43 +29:03:47.5 18.0mag C/2025 J1 (Borisov)
07:14:22.12 -12:53:35.5 16.5mag C/2025 R3 (PANSTARRS)
09:56:08.32 +22:26:06.5 17.6mag C/2025 V2 (Rankin)
12:44:37.82 +03:56:10.0 17.1mag C/2025 Y1 (ATLAS)
16:51:50.20 +79:07:16.0 17.4mag C/2026 A2 (Bok)
02:46:19.15 +45:14:30.3 16.7mag C/2026 B2 (Sun-Gao)
11:25:32.22 +04:33:05.0 16.9mag A/2026 E1
21:19:05.72 -15:05:25.9 7.3mag 10P/Tempel
11:13:28.43 -01:53:19.9 16.1mag 29P/Schwassmann-Wachmann
04:00:13.82 +29:33:27.5 17.8mag 47P/Ashbrook-Jackson
10:08:09.65 +13:59:55.3 17.0mag 63P/Wild
00:48:22.79 -05:05:33.5 15.5mag 65P/Gunn
08:27:04.74 +34:13:01.3 17.9mag 76P/West-Kohoutek-Ikemura
04:27:29.71 +20:10:51.6 13.7mag 78P/Gehrels
02:22:23.96 +10:36:54.6 16.2mag 88P/Howell
06:35:39.03 +30:31:57.4 15.7mag 93P/Lovas
04:21:07.73 +31:07:29.8 16.9mag 114P/Wiseman-Skiff
08:08:47.56 +30:41:57.0 15.2mag 123P/West-Hartley
10:48:12.39 +01:10:14.4 16.8mag 124P/Mrkos
04:51:47.56 +20:48:51.1 16.2mag 128P/Shoemaker-Holt
05:36:19.88 +19:42:49.8 17.8mag 131P/Mueller
00:01:33.37 +02:56:12.7 17.9mag 139P/Vaisala-Oterma
07:13:42.67 +17:00:44.0 15.5mag 141P-D/Machholz
03:16:51.99 -21:06:09.5 15.5mag 161P/Hartley-IRAS
05:33:12.45 +33:57:27.0 15.3mag 162P/SidingSpring
19:04:22.20 +15:06:22.8 14.7mag 169P/NEAT
01:41:07.52 +07:36:11.9 17.7mag 220P/McNaught
16:35:57.73 -08:23:12.6 17.0mag 235P/LINEAR
08:45:22.23 +33:17:45.0 17.9mag 240P/NEAT
20:42:09.31 -49:34:46.1 17.8mag 259P/Garradd
01:59:25.03 +12:06:48.6 15.7mag 260P/McNaught
05:37:20.83 +36:50:46.8 17.4mag 295P/LINEAR
15:06:36.64 +06:03:12.2 17.6mag 391P/Kowalski
08:34:38.38 +19:40:30.6 17.9mag 450P/LONEOS
07:51:49.78 +39:12:46.5 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 07:06 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
-rw-r--r-- 1 apache apache 5.6K Jul 10 07:06 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 10 07:06 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
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
20:59:14.423 -27:33:25.12 AT 2026spr 2026-07-07.32 23.4151
-rw-r--r-- 1 apache apache 30K Jul 10 07:06 tns_transients_list.txt
