This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA
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 10.3936 2461231.8936 10.49 23:49:42.53 +06:52:19.6
96.98233 -52.86133 galactic Psc Second-epoch detections are separated by 0.2" and 4.1 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 | Gaia DR3 2744921024872396416 | 23:49:42.52 +06:52:19.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.376+/-0.030 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:42.53 +06:52:19.6: 11.43 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:42.53 +06:52:19.6: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2744921024872396416,2461231.8936,10.49,0.05,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 2744921024872396416 20260710.3936 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 10.46 23:49:38.88 +06:54:37.1
96.98414 -52.82028 galactic Psc Second-epoch detections are separated by 0.2" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2744921402830568576 | 23:49:38.87 +06:54:37.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.329+/-0.030 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:38.88 +06:54:37.1: 11.42 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:38.88 +06:54:37.1: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2744921402830568576,2461231.8936,10.46,0.05,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 2744921402830568576 20260710.3936 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.3936 2461231.8936 10.24 23:50:25.49 +07:08:38.0
97.42767 -52.68014 galactic Psc Second-epoch detections are separated by 0.2" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2746435224183534336 | 23:50:25.48 +07:08:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.223+/-0.031 (F)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:25.49 +07:08:38.0: 11.18 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:25.49 +07:08:38.0: 11.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2746435224183534336,2461231.8936,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2746435224183534336 20260710.3936 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 10.60 23:49:31.54 +06:47:35.2
96.86157 -52.91610 galactic Psc Second-epoch detections are separated by 0.3" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2744918413533324416 | 23:49:31.55 +06:47:35.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.930+/-0.033 (M)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:31.54 +06:47:35.2: 11.60 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:31.54 +06:47:35.2: 11.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2744918413533324416,2461231.8936,10.60,0.05,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
Gaia DR3 2744918413533324416 20260710.3936 10.60CV 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 10.3936 2461231.8936 12.39 23:49:04.70 +06:35:43.9
96.56221 -53.05356 galactic Psc Second-epoch detections are separated by 1.1" and 4.1 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 | 23:49:04.70 +06:35:43.9 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.651+/-0.033 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:04.70 +06:35:43.9: 13.34 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:04.70 +06:35:43.9: 13.37 +/- 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,2461231.8936,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3936 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.36 23:48:46.50 +05:52:40.8
95.96330 -53.68033 galactic Psc Second-epoch detections are separated by 0.2" and 4.2 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 | 23:48:46.50 +05:52:40.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.431+/-0.032 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:48:46.50 +05:52:40.8: 13.38 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:48:46.50 +05:52:40.8: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.36,0.05,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 20260710.3936 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.3936 2461231.8936 12.00 00:13:14.27 +09:08:39.1
107.29948 -52.56424 galactic Psc Second-epoch detections are separated by 0.9" and 4.1 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 | 00:13:14.27 +09:08:39.1 (user input) | T | P | (position from user input) J-Ks=0.572+/-0.032 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:13:14.27 +09:08:39.1: 12.92 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:13:14.27 +09:08:39.1: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.00,0.05,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 20260710.3936 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.3936 2461231.8936 11.69 00:29:52.36 +02:39:28.5
112.19028 -59.76331 galactic Cet Second-epoch detections are separated by 0.7" and 4.2 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 | 00:29:52.36 +02:39:28.5 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.334+/-0.031 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:29:52.36 +02:39:28.5: 12.73 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:29:52.36 +02:39:28.5: 12.72 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3936* 00 29 52.36 +02 39 28.5 11.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,11.69,0.05,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 20260710.3936 11.69CV 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 10.3936 2461231.8936 12.90 23:49:48.44 +07:18:46.8
97.30306 -52.46492 galactic Psc Second-epoch detections are separated by 1.0" and 4.1 pix
The object was found in VSX 0" Gaia DR3 2746453022527978752
Type: ROT
# Max. Min./Amp. JD0 Period
13.730 G 13.760 G K
The object was not found in astcheck.
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:48.44 +07:18:46.8: 14.09 +/- 0.08 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:48.44 +07:18:46.8: 13.97 +/- 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
Gaia DR3 2746453022527978752,2461231.8936,12.90,0.05,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
Gaia DR3 2746453022527978752 20260710.3936 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 10.3936 2461231.8936 12.53 00:05:30.04 +08:49:24.1
104.13647 -52.36396 galactic Psc Second-epoch detections are separated by 0.7" and 4.2 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 | 00:05:30.04 +08:49:24.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.430+/-0.031 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:05:30.04 +08:49:24.1: 13.43 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:05:30.04 +08:49:24.1: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.53,0.05,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 20260710.3936 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 10.3936 2461231.8936 12.40 23:49:41.59 +06:26:29.5
96.69402 -53.25553 galactic Psc Second-epoch detections are separated by 1.9" and 4.4 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 | 23:49:41.59 +06:26:29.5 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.373+/-0.030 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:41.59 +06:26:29.5: 13.43 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:41.59 +06:26:29.5: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 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,2461231.8936,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3936 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.63 23:49:44.45 +05:31:23.1
96.09237 -54.10212 galactic Psc Second-epoch detections are separated by 1.8" and 4.3 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 | 23:49:44.45 +05:31:23.1 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.037 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:44.45 +05:31:23.1: 13.58 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:44.45 +05:31:23.1: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.63,0.05,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 20260710.3936 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 10.3936 2461231.8936 12.05 00:13:08.19 +09:11:18.6
107.27730 -52.51519 galactic Psc Second-epoch detections are separated by 0.2" and 4.2 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 | 00:13:08.19 +09:11:18.6 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.741+/-0.031 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:13:08.19 +09:11:18.6: 12.99 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:13:08.19 +09:11:18.6: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.05,0.05,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 20260710.3936 12.05CV 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 10.3936 2461231.8936 11.82 23:50:19.13 +06:33:14.4
97.00669 -53.21335 galactic Psc Second-epoch detections are separated by 0.6" and 4.1 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 | Gaia DR3 2744852717713582848 | 23:50:19.16 +06:33:14.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.378+/-0.033 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:19.13 +06:33:14.4: 12.74 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:19.13 +06:33:14.4: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2744852717713582848,2461231.8936,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2744852717713582848 20260710.3936 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 11.56 23:51:30.45 +06:21:20.9
97.33318 -53.51086 galactic Psc Second-epoch detections are separated by 0.8" and 4.3 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 | Gaia DR3 2744654973123307904 | 23:51:30.44 +06:21:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.366+/-0.032 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:30.45 +06:21:20.9: 12.50 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:30.45 +06:21:20.9: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2744654973123307904,2461231.8936,11.56,0.05,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
Gaia DR3 2744654973123307904 20260710.3936 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.82 23:49:07.09 +06:53:20.5
96.77033 -52.78806 galactic Psc Second-epoch detections are separated by 1.4" and 4.1 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 | 23:49:07.09 +06:53:20.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.447+/-0.035 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:07.09 +06:53:20.5: 14.05 +/- 0.08 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:07.09 +06:53:20.5: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 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,2461231.8936,12.82,0.05,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 20260710.3936 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 10.3936 2461231.8936 12.74 23:51:29.36 +06:05:49.1
97.15678 -53.74766 galactic Psc Second-epoch detections are separated by 0.2" and 4.1 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 | 23:51:29.36 +06:05:49.1 (user input) | T | P | (position from user input) J-Ks=0.457+/-0.032 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:29.36 +06:05:49.1: 13.89 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:29.36 +06:05:49.1: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 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,2461231.8936,12.74,0.05,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 20260710.3936 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 10.3936 2461231.8936 11.70 23:51:01.72 +06:44:13.4
97.39631 -53.11328 galactic Psc Second-epoch detections are separated by 0.9" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2746357261937170432 | 23:51:01.56 +06:44:13.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:01.72 +06:44:13.4: 12.54 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:01.72 +06:44:13.4: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2746357261937170432,2461231.8936,11.70,0.05,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
Gaia DR3 2746357261937170432 20260710.3936 11.70CV 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 10.3936 2461231.8936 11.92 23:50:46.23 +06:20:27.8
97.04004 -53.45322 galactic Psc Second-epoch detections are separated by 0.9" and 4.3 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 | 23:50:46.23 +06:20:27.8 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.342+/-0.033 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:46.23 +06:20:27.8: 12.85 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:46.23 +06:20:27.8: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,11.92,0.05,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 20260710.3936 11.92CV 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 10.3936 2461231.8936 12.79 23:51:02.80 +06:29:13.1
97.24138 -53.34557 galactic Psc Second-epoch detections are separated by 1.2" and 4.2 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 | 23:51:02.80 +06:29:13.1 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.610+/-0.032 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:02.80 +06:29:13.1: 13.93 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:02.80 +06:29:13.1: 13.89 +/- 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,2461231.8936,12.79,0.05,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 20260710.3936 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 10.3936 2461231.8936 12.51 23:36:23.40 +05:33:43.9
91.11595 -52.61109 galactic Psc Second-epoch detections are separated by 3.6" and 4.7 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 | 23:36:23.40 +05:33:43.9 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.573+/-0.033 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:36:23.40 +05:33:43.9: 13.51 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:36:23.40 +05:33:43.9: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3936 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.56 23:50:04.34 +07:18:18.3
97.39750 -52.49768 galactic Psc Second-epoch detections are separated by 2.3" and 4.0 pix
The object was found in VSX 3" Gaia DR3 2746450136309957248
Type: ROT
# Max. Min./Amp. JD0 Period
13.230 G 13.240 G M
The object was not found in astcheck.
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:04.34 +07:18:18.3: 13.77 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:04.34 +07:18:18.3: 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
Gaia DR3 2746450136309957248,2461231.8936,12.56,0.05,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
Gaia DR3 2746450136309957248 20260710.3936 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 10.3936 2461231.8936 12.08 00:13:00.27 +08:58:53.9
107.14206 -52.70783 galactic Psc Second-epoch detections are separated by 1.0" and 4.0 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 | 00:13:00.27 +08:58:53.9 (user input) | T | P | (position from user input) J-Ks=0.363+/-0.035 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:13:00.27 +08:58:53.9: 13.13 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:13:00.27 +08:58:53.9: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3936 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 11.72 23:49:21.44 +06:34:17.3
96.65215 -53.10317 galactic Psc Second-epoch detections are separated by 0.5" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2744861101489711488 | 23:49:21.44 +06:34:17.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.569+/-0.029 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:21.44 +06:34:17.3: 12.66 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:21.44 +06:34:17.3: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2744861101489711488,2461231.8936,11.72,0.05,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
Gaia DR3 2744861101489711488 20260710.3936 11.72CV 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 10.3936 2461231.8936 12.39 23:49:03.24 +06:48:18.8
96.69124 -52.85871 galactic Psc Second-epoch detections are separated by 0.3" and 4.1 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 | 23:49:03.24 +06:48:18.8 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.514+/-0.034 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:03.24 +06:48:18.8: 13.68 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:03.24 +06:48:18.8: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3936 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.60 23:48:52.40 +07:07:27.9
96.83159 -52.54781 galactic Psc Second-epoch detections are separated by 1.8" and 4.1 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 | 23:48:52.40 +07:07:27.9 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.438+/-0.033 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:48:52.40 +07:07:27.9: 13.66 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:48:52.40 +07:07:27.9: 13.71 +/- 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,2461231.8936,12.60,0.05,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 20260710.3936 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 10.3936 2461231.8936 12.63 23:49:57.91 +07:32:13.1
97.50404 -52.27352 galactic Psc Second-epoch detections are separated by 0.7" and 4.3 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 | 23:49:57.91 +07:32:13.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.397+/-0.029 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:57.91 +07:32:13.1: 13.65 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:57.91 +07:32:13.1: 13.76 +/- 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,2461231.8936,12.63,0.05,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 20260710.3936 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 10.3936 2461231.8936 12.53 23:50:36.21 +07:01:54.9
97.42378 -52.80054 galactic Psc Second-epoch detections are separated by 0.2" and 4.2 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 | 23:50:36.21 +07:01:54.9 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5) J-Ks=0.851+/-0.028 (M)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:36.21 +07:01:54.9: 13.65 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:36.21 +07:01:54.9: 13.74 +/- 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,2461231.8936,12.53,0.05,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 20260710.3936 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 10.3936 2461231.8936 11.84 23:49:32.19 +06:54:17.1
96.93842 -52.81452 galactic Psc Second-epoch detections are separated by 0.5" and 4.3 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 | 23:49:32.19 +06:54:17.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:32.19 +06:54:17.1: 12.89 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:32.19 +06:54:17.1: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,11.84,0.05,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 20260710.3936 11.84CV 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 10.3936 2461231.8936 11.07 23:50:21.54 +07:10:28.3
97.42235 -52.64557 galactic Psc Second-epoch detections are separated by 0.3" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2746436117536707840 | 23:50:21.53 +07:10:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.299+/-0.032 (F)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:21.54 +07:10:28.3: 11.98 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:21.54 +07:10:28.3: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2746436117536707840,2461231.8936,11.07,0.05,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
Gaia DR3 2746436117536707840 20260710.3936 11.07CV 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 10.3936 2461231.8936 12.31 00:29:37.86 +02:52:07.9
112.14199 -59.54527 galactic Psc Second-epoch detections are separated by 3.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J007.4103+02.8677 | 00:29:37.86 +02:52:07.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.327+/-0.034 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:29:37.86 +02:52:07.9: 13.11 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:29:37.86 +02:52:07.9: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J007.4103+02.8677,2461231.8936,12.31,0.05,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 J007.4103+02.8677 20260710.3936 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.36 23:50:51.39 +06:50:13.0
97.39493 -53.00463 galactic Psc Second-epoch detections are separated by 0.3" and 4.1 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 | 23:50:51.39 +06:50:13.0 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.496+/-0.029 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:51.39 +06:50:13.0: 13.33 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:51.39 +06:50:13.0: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.34 +/- 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,2461231.8936,12.36,0.05,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 20260710.3936 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.3936 2461231.8936 12.40 23:30:09.06 +10:46:31.3
92.74333 -47.27569 galactic Peg Second-epoch detections are separated by 0.9" and 4.3 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 | 23:30:09.06 +10:46:31.3 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.390+/-0.034 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:30:09.06 +10:46:31.3: 13.32 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:30:09.06 +10:46:31.3: 13.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.34 +/- 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,2461231.8936,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3936 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.52 23:50:15.10 +07:11:39.8
97.39454 -52.61696 galactic Psc Second-epoch detections are separated by 0.3" and 4.2 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 | 23:50:15.10 +07:11:39.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.428+/-0.037 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:15.10 +07:11:39.8: 13.80 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:15.10 +07:11:39.8: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.52,0.05,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 20260710.3936 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.44 23:38:46.98 +05:49:18.3
92.18327 -52.65769 galactic Psc Second-epoch detections are separated by 1.0" and 4.1 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 | 23:38:46.98 +05:49:18.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.393+/-0.034 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:38:46.98 +05:49:18.3: 13.50 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:38:46.98 +05:49:18.3: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 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,2461231.8936,12.44,0.05,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 20260710.3936 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 10.3936 2461231.8936 11.86 23:50:31.15 +07:06:10.2
97.43714 -52.72705 galactic Psc Second-epoch detections are separated by 0.2" and 4.2 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 | 23:50:31.15 +07:06:10.2 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.271+/-0.030 (F)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:31.15 +07:06:10.2: 12.83 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:31.15 +07:06:10.2: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,11.86,0.05,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 20260710.3936 11.86CV 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 10.3936 2461231.8936 12.51 00:13:11.31 +09:08:45.5
107.28076 -52.55956 galactic Psc Second-epoch detections are separated by 0.2" and 4.2 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 | 00:13:11.31 +09:08:45.5 (user input) | T | P | (position from user input) J-Ks=0.647+/-0.033 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:13:11.31 +09:08:45.5: 13.62 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:13:11.31 +09:08:45.5: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3936 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.66 23:49:29.24 +06:50:51.2
96.88260 -52.86231 galactic Psc Second-epoch detections are separated by 0.9" and 4.1 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 | 23:49:29.24 +06:50:51.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.503+/-0.036 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:29.24 +06:50:51.2: 13.61 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:29.24 +06:50:51.2: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.66,0.05,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 20260710.3936 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 10.3936 2461231.8936 12.64 23:50:49.20 +07:21:11.6
97.70910 -52.52454 galactic Psc Second-epoch detections are separated by 0.7" and 4.2 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 | 23:50:49.20 +07:21:11.6 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.358+/-0.031 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:49.20 +07:21:11.6: 13.78 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:49.20 +07:21:11.6: 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,2461231.8936,12.64,0.05,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 20260710.3936 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.12 00:29:22.55 +02:31:55.6
111.90492 -59.86645 galactic Cet Second-epoch detections are separated by 1.4" and 4.5 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 | 00:29:22.55 +02:31:55.6 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.035 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:29:22.55 +02:31:55.6: 13.07 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:29:22.55 +02:31:55.6: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3936* 00 29 22.55 +02 31 55.6 12.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.12,0.05,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 20260710.3936 12.12CV 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 10.3936 2461231.8936 12.81 23:50:01.28 +07:08:09.1
97.27039 -52.64877 galactic Psc Second-epoch detections are separated by 0.5" and 4.2 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 | 23:50:01.28 +07:08:09.1 (user input) | T | P | (position from user input) J-Ks=0.539+/-0.035 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:01.28 +07:08:09.1: 14.13 +/- 0.09 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:01.28 +07:08:09.1: 13.96 +/- 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,2461231.8936,12.81,0.05,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 20260710.3936 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 10.3936 2461231.8936 12.59 23:50:25.62 +07:37:12.9
97.72892 -52.24056 galactic Psc Second-epoch detections are separated by 1.3" and 4.3 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 | 23:50:25.62 +07:37:12.9 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.515+/-0.031 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:25.62 +07:37:12.9: 13.74 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:25.62 +07:37:12.9: 13.70 +/- 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,2461231.8936,12.59,0.05,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 20260710.3936 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.3936 2461231.8936 12.28 00:07:07.06 +09:06:42.1
104.89634 -52.20121 galactic Psc Second-epoch detections are separated by 1.1" and 3.9 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 | 00:07:07.06 +09:06:42.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.752+/-0.030 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:07:07.06 +09:06:42.1: 13.26 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:07:07.06 +09:06:42.1: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.28,0.05,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 20260710.3936 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.28 00:29:48.02 +02:47:31.8
112.19914 -59.62793 galactic Psc Second-epoch detections are separated by 3.3" and 4.8 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 | 00:29:48.02 +02:47:31.8 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.034 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:29:48.02 +02:47:31.8: 13.26 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:29:48.02 +02:47:31.8: 13.55 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.39 +/- 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,2461231.8936,12.28,0.05,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 20260710.3936 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 11.59 23:51:01.59 +06:15:51.3
97.08805 -53.54878 galactic Psc Second-epoch detections are separated by 0.7" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2744648311630083328 | 23:51:01.58 +06:15:51.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.326+/-0.028 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:01.59 +06:15:51.3: 12.54 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:01.59 +06:15:51.3: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2744648311630083328,2461231.8936,11.59,0.05,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 2744648311630083328 20260710.3936 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.3936 2461231.8936 11.64 00:29:25.11 +02:37:36.8
111.95786 -59.77486 galactic Cet Second-epoch detections are separated by 1.0" and 4.1 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 | Gaia DR3 2547594181297232128 | 00:29:25.14 +02:37:37.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.497+/-0.037 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:29:25.11 +02:37:36.8: 12.54 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:29:25.11 +02:37:36.8: 12.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3936* 00 29 25.11 +02 37 36.8 11.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2547594181297232128,2461231.8936,11.64,0.05,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 2547594181297232128 20260710.3936 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 11.88 23:50:22.51 +06:18:17.5
96.86447 -53.44799 galactic Psc Second-epoch detections are separated by 0.4" and 4.2 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 | 23:50:22.51 +06:18:17.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.364+/-0.030 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:22.51 +06:18:17.5: 12.79 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:22.51 +06:18:17.5: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3936 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.19 23:49:34.19 +07:06:06.9
97.07860 -52.63638 galactic Psc Second-epoch detections are separated by 0.6" and 4.3 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 | 23:49:34.19 +07:06:06.9 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.396+/-0.033 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:34.19 +07:06:06.9: 13.25 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:34.19 +07:06:06.9: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3936 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.18 23:50:00.74 +07:37:13.7
97.57416 -52.20095 galactic Psc Second-epoch detections are separated by 0.8" and 4.3 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 | 23:50:00.74 +07:37:13.7 (user input) | T | P | (position from user input) SpType: em 1996AJ....112.1188B BPS CS 29522- 1 J-Ks=0.705+/-0.030 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:00.74 +07:37:13.7: 13.24 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:00.74 +07:37:13.7: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.18,0.05,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 20260710.3936 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.29 23:48:48.30 +06:52:28.8
96.64294 -52.77045 galactic Psc Second-epoch detections are separated by 0.6" and 4.1 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 | 23:48:48.30 +06:52:28.8 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.480+/-0.029 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:48:48.30 +06:52:28.8: 13.21 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:48:48.30 +06:52:28.8: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3936 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.43 23:51:18.69 +06:18:01.8
97.22159 -53.54296 galactic Psc Second-epoch detections are separated by 0.7" and 4.3 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 | 23:51:18.69 +06:18:01.8 (user input) | T | P | (position from user input) J-Ks=0.602+/-0.036 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:18.69 +06:18:01.8: 13.58 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:18.69 +06:18:01.8: 13.46 +/- 0.04 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,2461231.8936,12.43,0.05,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 20260710.3936 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.56 23:51:10.62 +06:13:16.5
97.11780 -53.60296 galactic Psc Second-epoch detections are separated by 1.9" and 4.1 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 | 23:51:10.62 +06:13:16.5 (user input) | T | P | (position from user input) J-Ks=0.527+/-0.028 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:10.62 +06:13:16.5: 13.74 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:10.62 +06:13:16.5: 13.72 +/- 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,2461231.8936,12.56,0.05,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 20260710.3936 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 10.3936 2461231.8936 12.03 00:29:58.13 +02:32:04.8
112.19670 -59.88884 galactic Cet Second-epoch detections are separated by 1.5" and 4.2 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 | 00:29:58.13 +02:32:04.8 (user input) | T | P | (position from user input) J-Ks=0.406+/-0.031 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:29:58.13 +02:32:04.8: 13.02 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:29:58.13 +02:32:04.8: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.08 +/- 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!
TCP 2026 07 10.3936* 00 29 58.13 +02 32 04.8 12.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.03,0.05,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 20260710.3936 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.81 23:50:09.14 +07:20:00.6
97.44558 -52.47914 galactic Psc Second-epoch detections are separated by 0.6" and 4.1 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 | 23:50:09.14 +07:20:00.6 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.032 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:09.14 +07:20:00.6: 13.83 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:09.14 +07:20:00.6: 14.01 +/- 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,2461231.8936,12.81,0.05,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 20260710.3936 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 10.3936 2461231.8936 12.23 00:17:34.44 +01:20:47.5
105.60638 -60.38110 galactic Psc Second-epoch detections are separated by 0.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J004.3935+01.3466 | 00:17:34.44 +01:20:47.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.370+/-0.034 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:17:34.44 +01:20:47.5: 13.18 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:17:34.44 +01:20:47.5: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J004.3935+01.3466,2461231.8936,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J004.3935+01.3466 20260710.3936 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 13.07 23:50:13.17 +06:52:49.7
97.18107 -52.90318 galactic Psc Second-epoch detections are separated by 1.7" and 4.4 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 | 23:50:13.17 +06:52:49.7 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.036 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:13.17 +06:52:49.7: 14.51 +/- 0.13 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:13.17 +06:52:49.7: 14.61 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461231.8936,13.07,0.05,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 20260710.3936 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 10.3936 2461231.8936 12.58 23:49:25.12 +07:31:17.5
97.29026 -52.23534 galactic Psc Second-epoch detections are separated by 0.7" and 4.3 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 | 23:49:25.12 +07:31:17.5 (user input) | T | P | (position from user input) J-Ks=0.800+/-0.034 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:25.12 +07:31:17.5: 13.71 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:25.12 +07:31:17.5: 13.61 +/- 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,2461231.8936,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3936 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.55 00:12:47.76 +09:06:03.0
107.10804 -52.57964 galactic Psc Second-epoch detections are separated by 0.7" and 4.3 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 | 00:12:47.76 +09:06:03.0 (user input) | T | P | (position from user input) J-Ks=0.390+/-0.035 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:12:47.76 +09:06:03.0: 13.67 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:12:47.76 +09:06:03.0: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.55,0.05,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 20260710.3936 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 10.3936 2461231.8936 11.16 23:49:53.52 +07:00:44.7
97.14232 -52.74999 galactic Psc Second-epoch detections are separated by 0.2" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2746426943486548480 | 23:49:53.53 +07:00:44.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.228+/-0.032 (F)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:53.52 +07:00:44.7: 12.10 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:53.52 +07:00:44.7: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2746426943486548480,2461231.8936,11.16,0.05,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
Gaia DR3 2746426943486548480 20260710.3936 11.16CV 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 10.3936 2461231.8936 12.76 23:50:23.79 +06:49:07.3
97.20832 -52.97718 galactic Psc Second-epoch detections are separated by 1.0" and 4.2 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 | 23:50:23.79 +06:49:07.3 (user input) | T | P | (position from user input) J-Ks=0.271+/-0.038 (F)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:23.79 +06:49:07.3: 13.98 +/- 0.08 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:23.79 +06:49:07.3: 13.91 +/- 0.07 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,2461231.8936,12.76,0.05,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 20260710.3936 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 10.3936 2461231.8936 12.58 23:50:06.36 +05:27:16.2
96.18719 -54.20151 galactic Psc Second-epoch detections are separated by 0.8" and 4.1 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 | 23:50:06.36 +05:27:16.2 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.033 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:06.36 +05:27:16.2: 13.56 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:06.36 +05:27:16.2: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3936 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.06 00:27:24.56 +03:00:28.4
111.11591 -59.31148 galactic Psc Second-epoch detections are separated by 2.2" and 4.5 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 | 00:27:24.56 +03:00:28.4 (user input) | T | P | (position from user input) J-Ks=0.455+/-0.030 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:27:24.56 +03:00:28.4: 12.96 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:27:24.56 +03:00:28.4: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 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,2461231.8936,12.06,0.05,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 20260710.3936 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.3936 2461231.8936 11.12 23:50:33.02 +07:21:04.6
97.60640 -52.50072 galactic Psc Second-epoch detections are separated by 0.5" and 4.3 pix
The object was found in VSX 1" Gaia DR3 2746451991734645888
Type: ROT
# Max. Min./Amp. JD0 Period
11.840 G 11.890 G 1.432840000000 G
The object was not found in astcheck.
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:33.02 +07:21:04.6: 12.06 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:33.02 +07:21:04.6: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2746451991734645888,2461231.8936,11.12,0.05,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
Gaia DR3 2746451991734645888 20260710.3936 11.12CV 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 10.3936 2461231.8936 12.71 23:52:01.58 +06:10:59.8
97.42133 -53.71980 galactic Psc Second-epoch detections are separated by 2.3" and 3.8 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 | 23:52:01.58 +06:10:59.8 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.033 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:52:01.58 +06:10:59.8: 13.83 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:52:01.58 +06:10:59.8: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461231.8936,12.71,0.05,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 20260710.3936 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 10.3936 2461231.8936 11.49 23:50:59.88 +07:21:02.4
97.77455 -52.54376 galactic Psc Second-epoch detections are separated by 0.2" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2746462883772936704 | 23:50:59.89 +07:21:02.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.656+/-0.028 (K)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:59.88 +07:21:02.4: 12.43 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:59.88 +07:21:02.4: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2746462883772936704,2461231.8936,11.49,0.05,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 2746462883772936704 20260710.3936 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.64 23:48:23.86 +07:01:55.8
96.59319 -52.58575 galactic Psc Second-epoch detections are separated by 1.4" and 4.4 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 | 23:48:23.86 +07:01:55.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.418+/-0.033 (G)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:48:23.86 +07:01:55.8: 13.68 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:48:23.86 +07:01:55.8: 13.61 +/- 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,2461231.8936,12.64,0.05,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 20260710.3936 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 12.49 23:50:18.34 +06:14:27.1
96.79544 -53.50001 galactic Psc Second-epoch detections are separated by 1.5" and 4.0 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 | 23:50:18.34 +06:14:27.1 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.286+/-0.040 (F)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:18.34 +06:14:27.1: 13.39 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:18.34 +06:14:27.1: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,12.49,0.05,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 20260710.3936 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3936 2461231.8936 11.96 23:50:19.37 +06:48:13.5
97.17068 -52.98383 galactic Psc Second-epoch detections are separated by 0.4" and 4.1 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 | 23:50:19.37 +06:48:13.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.238+/-0.033 (F)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:19.37 +06:48:13.5: 12.93 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:19.37 +06:48:13.5: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8936,11.96,0.05,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 20260710.3936 11.96CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.63355392 18.01.2026 03:12:09.059 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
First image: 2461058.63355392 18.01.2026 03:12:09.059 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
Last image: 2461231.89384866 10.07.2026 09:26:58.524 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.82
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4996
Objects passed selection criteria: 4978
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 3312.5
Average stars matched: 3128 (94.4302 %)
Memory usage VmPeak: 111360 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 05:12:54 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: 2461058.63355392 18.01.2026 03:12:09.059 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
First image: 2461058.63355392 18.01.2026 03:12:09.059 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
Last image: 2461231.89384866 10.07.2026 09:26:58.524 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 74
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
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): 28032
Objects passed selection criteria: 27959
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 19240.8
Average stars matched: 18274.5 (94.9781 %)
Memory usage VmPeak: 131864 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 05:15:49 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/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.cat to cache
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.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: 2461231.89335062
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'
Plate-solving the images
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits exists and is non-empty
Saving wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits to local_wcs_cache/
'wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits' -> 'local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits'
wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits exists and is non-empty
Saving wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits to local_wcs_cache/
'wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits' -> 'local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits'
wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits exists and is non-empty
Saving wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits to local_wcs_cache/
'wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits' -> 'local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits'
wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits exists and is non-empty
Saving wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits to local_wcs_cache/
'wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits' -> 'local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits (1st reference image)
verification OK: wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
Image size: 942.2'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:10.776 +05:59:34.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits (1st new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
Image size: 941.1'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: 00:00:00.988 +06:00:04.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:10.776 +05:59:34.31
Second-epoch image center 00:00:00.988 +06:00:04.51
Angular distance between the image centers 0.0414 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits (2nd new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
Image size: 941.1'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: 00:00:02.089 +05:59:45.52 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:10.776 +05:59:34.31
Second-epoch image center 00:00:02.089 +05:59:45.52
Angular distance between the image centers 0.0361 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 00:00:00.988 +06:00:04.51
Second-epoch second image center 00:00:02.089 +05:59:45.52
Angular distance between the image centers 0.00697 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits &> /tmp/tmp.rERHu8Qe1Z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits &> /tmp/tmp.mE6RfEt75r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits &> /tmp/tmp.w4dwUuL4ZE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits &> /tmp/tmp.RZz75u5Cbz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits and wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits and wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat
Found non-empty wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits and wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat
The reference image (wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits) and catalog (wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat) found
'wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat' -> 'wcsmag.cat'
Read 5105 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0007 to 359.9997 deg, Dec +0.7073 to +11.2786 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 0.0007 to 359.9997 deg, Dec 0.7073 to 11.2786 deg
Loaded 178998 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): 3523 out of 3630 total matches.
Matched with Tycho-2 3630 out of 5105 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.706600
a=0.000000 b=1.000000 c=22.706600
From vast_summary.log: estimated ref. image limiting mag.: -7.82
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5105 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0007 to 359.9997 deg, Dec +0.7073 to +11.2786 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 0.0007 to 359.9997 deg, Dec 0.7073 to 11.2786 deg
Loaded 178998 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): 3523 out of 3630 total matches.
Matched with Tycho-2 3630 out of 5105 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits:
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits (aperture=6.1)
Read 5657 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9997 deg, Dec +0.6890 to +11.2632 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 0.0001 to 359.9997 deg, Dec 0.6890 to 11.2632 deg
Loaded 178988 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): 3650 out of 3762 total matches.
Matched with Tycho-2 3762 out of 5657 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits:
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
2.1 pix Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
2.9 pix fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
2.8 pix fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
2.1 pix wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
2.1 pix wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Limiting magnitude estimates:
14.9 mag. Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
15.0 mag. Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
12.7 mag. fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
12.4 mag. fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 10.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.rERHu8Qe1Z (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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits' -> 'wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.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=343, bad_region=0, passed=5105
Got 5105 stars (including 4755 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat
util/solve_plate_with_UCAC5 got 5105 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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
RA wraps around 0/360 boundary: field RA 352.0700 through 0 to 8.0259, gap 8.0259 to 352.0700
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0700 through 0 to 8.0263, gap 8.0263 to 352.0700
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits N_match=975 sigma_overall_arcsec=0.339 sigma_q1_arcsec=0.369 sigma_q2_arcsec=0.320 sigma_q3_arcsec=0.322 sigma_q4_arcsec=0.325 n_q1=225 n_q2=266 n_q3=214 n_q4=270 worst_quadrant_to_overall_ratio=1.089
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits -region wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.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.mE6RfEt75r (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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits' -> 'wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.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=353, bad_region=1, passed=5657
Got 5657 stars (including 5295 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat
util/solve_plate_with_UCAC5 got 5657 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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
RA wraps around 0/360 boundary: field RA 352.0600 through 0 to 8.0260, gap 8.0260 to 352.0600
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5559 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
RA wraps around 0/360 boundary: field RA 352.0599 through 0 to 8.0264, gap 8.0264 to 352.0599
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits N_match=976 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.310 sigma_q2_arcsec=0.292 sigma_q3_arcsec=0.292 sigma_q4_arcsec=0.264 n_q1=215 n_q2=272 n_q3=214 n_q4=275 worst_quadrant_to_overall_ratio=1.081
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits -region wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.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.w4dwUuL4ZE (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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.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=67, bad_region=0, passed=1299
Got 1299 stars (including 1228 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat
util/solve_plate_with_UCAC5 got 1299 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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
RA wraps around 0/360 boundary: field RA 351.9320 through 0 to 8.1300, gap 8.1300 to 351.9320
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.5)
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: 967 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 1265 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
RA wraps around 0/360 boundary: field RA 351.9321 through 0 to 8.1302, gap 8.1302 to 351.9321
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.5)
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: 967 matched stars entering correct_measured_positions(), 1264 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 1264 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits N_match=967 sigma_overall_arcsec=0.319 sigma_q1_arcsec=0.324 sigma_q2_arcsec=0.368 sigma_q3_arcsec=0.291 sigma_q4_arcsec=0.293 n_q1=227 n_q2=280 n_q3=247 n_q4=213 worst_quadrant_to_overall_ratio=1.153
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits -region wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.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.RZz75u5Cbz (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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.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=73, bad_region=0, passed=1285
Got 1285 stars (including 1210 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat
util/solve_plate_with_UCAC5 got 1285 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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
RA wraps around 0/360 boundary: field RA 351.9320 through 0 to 8.1300, gap 8.1300 to 351.9320
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 967 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(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 1250 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9320 through 0 to 8.1301, gap 8.1301 to 351.9320
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 967 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(), 1247 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 1247 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits N_match=965 sigma_overall_arcsec=0.304 sigma_q1_arcsec=0.332 sigma_q2_arcsec=0.354 sigma_q3_arcsec=0.293 sigma_q4_arcsec=0.252 n_q1=239 n_q2=232 n_q3=288 n_q4=206 worst_quadrant_to_overall_ratio=1.164
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits -region wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.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=Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits sigma_overall=0.339 worst_q_ratio=1.089
ref2=Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits sigma_overall=0.286 worst_q_ratio=1.081
new1=fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits sigma_overall=0.319 worst_q_ratio=1.153
new2=fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits sigma_overall=0.304 worst_q_ratio=1.164
reference average sigma_overall=0.3125 worst_q_ratio=1.085
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080_astrometric_residuals.png (975 matched stars from wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080_astrometric_residuals.png (976 matched stars from wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368_astrometric_residuals.png (967 matched stars from wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369_astrometric_residuals.png (965 matched stars from wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits'
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits'
Preparing the HTML report for the field Psc-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:38.88 +06:54:37.1: 11.42 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:25.49 +07:08:38.0: 11.18 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:31.54 +06:47:35.2: 11.60 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:42.53 +06:52:19.6: 11.43 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:42.53 +06:52:19.6: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Forced photometry filter KEPT candidate at 23:49:42.53 +06:52:19.6: ref_mag=11.45 +/- 0.01 new_mean_mag=10.4895 delta=0.96 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:31.54 +06:47:35.2: 11.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:25.49 +07:08:38.0: 11.13 +/- 0.01 detection
Forced photometry filter KEPT candidate at 23:49:31.54 +06:47:35.2: ref_mag=11.59 +/- 0.01 new_mean_mag=10.5915 delta=0.99 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:38.88 +06:54:37.1: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Forced photometry filter KEPT candidate at 23:50:25.49 +07:08:38.0: ref_mag=11.15 +/- 0.00 new_mean_mag=10.2430 delta=0.91 (need > 0.90)
Forced photometry reference-image weighted average: 11.43 +/- 0.01
Forced photometry filter KEPT candidate at 23:49:38.88 +06:54:37.1: ref_mag=11.43 +/- 0.01 new_mean_mag=10.4550 delta=0.97 (need > 0.90)
Adding exclusion_list_local.txt__out02017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02187.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02136_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 02136_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02114_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 02114_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02017_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 02017_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02187_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 02187_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 20s
Prepared the HTML report for the field Psc-04-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 ####
23:50:25.49 +07:08:38.0
23:49:38.88 +06:54:37.1
23:49:42.53 +06:52:19.6
23:49:31.54 +06:47:35.2
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/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.cat to cache
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
Creating symlink local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.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_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits exists and is non-empty
wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits exists and is non-empty
wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits exists and is non-empty
wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits (1st reference image)
verification OK: wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
Image size: 942.2'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:10.776 +05:59:34.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits (1st new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
Image size: 941.1'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: 00:00:00.988 +06:00:04.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:10.776 +05:59:34.31
Second-epoch image center 00:00:00.988 +06:00:04.51
Angular distance between the image centers 0.0414 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits (2nd new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
Image size: 941.1'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: 00:00:02.089 +05:59:45.52 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:10.776 +05:59:34.31
Second-epoch image center 00:00:02.089 +05:59:45.52
Angular distance between the image centers 0.0361 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 00:00:00.988 +06:00:04.51
Second-epoch second image center 00:00:02.089 +05:59:45.52
Angular distance between the image centers 0.00697 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits &> /tmp/tmp.OKrvCDkFFD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits &> /tmp/tmp.5DiKXMCQ3g
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits &> /tmp/tmp.gAnwkWbSHs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits &> /tmp/tmp.X9UkAeDbDY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits and wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits and wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat
Found non-empty wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits and wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat
The reference image (wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits) and catalog (wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat) found
'wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat' -> 'wcsmag.cat'
Read 29260 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0006 to 360.0000 deg, Dec +0.7039 to +11.2824 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 0.0006 to 360.0000 deg, Dec 0.7039 to 11.2824 deg
Loaded 179124 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): 3728 out of 4002 total matches.
Matched with Tycho-2 4002 out of 29260 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.579100
a=0.000000 b=1.000000 c=22.579100
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.02
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.02
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29260 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0006 to 360.0000 deg, Dec +0.7039 to +11.2824 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 0.0006 to 360.0000 deg, Dec 0.7039 to 11.2824 deg
Loaded 179124 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): 3728 out of 4002 total matches.
Matched with Tycho-2 4002 out of 29260 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits:
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits (aperture=4.8)
Read 31418 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9997 deg, Dec +0.6886 to +11.2641 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 0.0001 to 359.9997 deg, Dec 0.6886 to 11.2641 deg
Loaded 179005 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): 3719 out of 3990 total matches.
Matched with Tycho-2 3990 out of 31418 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits:
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 68 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
2.0 pix Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
2.7 pix fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
2.7 pix fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
2.0 pix wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
2.0 pix wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Limiting magnitude estimates:
15.0 mag. Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
15.1 mag. Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
13.1 mag. fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
13.1 mag. fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.OKrvCDkFFD (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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits' -> 'wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1051, bad_region=0, passed=29256
Got 29256 stars (including 28151 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat
util/solve_plate_with_UCAC5 got 29256 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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
RA wraps around 0/360 boundary: field RA 352.0579 through 0 to 8.0336, gap 8.0336 to 352.0579
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 28858 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0577 through 0 to 8.0339, gap 8.0339 to 352.0577
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 28862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 28862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits N_match=974 sigma_overall_arcsec=0.329 sigma_q1_arcsec=0.345 sigma_q2_arcsec=0.306 sigma_q3_arcsec=0.319 sigma_q4_arcsec=0.330 n_q1=233 n_q2=264 n_q3=217 n_q4=260 worst_quadrant_to_overall_ratio=1.049
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits -region wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.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.5DiKXMCQ3g (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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits' -> 'wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.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=1105, bad_region=27, passed=31412
Got 31412 stars (including 30221 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat
util/solve_plate_with_UCAC5 got 31412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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
RA wraps around 0/360 boundary: field RA 352.0552 through 0 to 8.0260, gap 8.0260 to 352.0552
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 30996 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
RA wraps around 0/360 boundary: field RA 352.0551 through 0 to 8.0264, gap 8.0264 to 352.0551
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 30994 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 30994 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits N_match=973 sigma_overall_arcsec=0.292 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.297 sigma_q3_arcsec=0.298 sigma_q4_arcsec=0.262 n_q1=226 n_q2=265 n_q3=219 n_q4=263 worst_quadrant_to_overall_ratio=1.114
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits -region wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.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.gAnwkWbSHs (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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.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=3, blended=156, bad_region=2, passed=8275
Got 8275 stars (including 8105 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat
util/solve_plate_with_UCAC5 got 8275 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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
RA wraps around 0/360 boundary: field RA 351.9003 through 0 to 8.1300, gap 8.1300 to 351.9003
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
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: 962 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8033 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
RA wraps around 0/360 boundary: field RA 351.9003 through 0 to 8.1302, gap 8.1302 to 351.9003
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
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: 962 matched stars entering correct_measured_positions(), 8033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits N_match=962 sigma_overall_arcsec=0.313 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.363 sigma_q3_arcsec=0.281 sigma_q4_arcsec=0.281 n_q1=222 n_q2=273 n_q3=249 n_q4=218 worst_quadrant_to_overall_ratio=1.160
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits -region wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.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.X9UkAeDbDY (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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.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=3, blended=164, bad_region=4, passed=8585
Got 8585 stars (including 8403 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat
util/solve_plate_with_UCAC5 got 8585 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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
RA wraps around 0/360 boundary: field RA 351.9207 through 0 to 8.2037, gap 8.2037 to 351.9207
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 8300 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9203 through 0 to 8.2040, gap 8.2040 to 351.9203
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 965 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(), 8297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 8297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits N_match=963 sigma_overall_arcsec=0.313 sigma_q1_arcsec=0.345 sigma_q2_arcsec=0.353 sigma_q3_arcsec=0.286 sigma_q4_arcsec=0.270 n_q1=231 n_q2=230 n_q3=296 n_q4=206 worst_quadrant_to_overall_ratio=1.126
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits -region wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.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_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-15_20.00sec_-0.00C_LIGHTs_0368.fits
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.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_Psc-04-Q1b1x1_042734_TTUQ1b1x1_593932_lTfRZlvA/wcs_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369.fits
Preparing the HTML report for the field Psc-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:24:16.33 +01:48:40.4: 13.11 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:20:08.17 +06:40:40.1: 12.43 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:13:14.27 +09:08:39.1: 12.92 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:41.59 +06:26:29.5: 13.43 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:48.44 +07:18:46.8: 14.09 +/- 0.08 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:30:08.17 +04:52:55.7: 12.13 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:04.70 +06:35:43.9: 13.34 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:24:16.33 +01:48:40.4: 13.13 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:05:30.04 +08:49:24.1: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Forced photometry filter REJECTED candidate at 00:24:16.33 +01:48:40.4: ref_mag=13.12 +/- 0.03 new_mean_mag=12.9450 delta=0.18 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:20:08.17 +06:40:40.1: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter REJECTED candidate at 00:20:08.17 +06:40:40.1: ref_mag=12.42 +/- 0.01 new_mean_mag=12.3994 delta=0.02 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:48:46.50 +05:52:40.8: 13.38 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:13:14.27 +09:08:39.1: 12.98 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:29:52.36 +02:39:28.5: 12.73 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:41.59 +06:26:29.5: 13.44 +/- 0.04 detection
Forced photometry filter KEPT candidate at 00:13:14.27 +09:08:39.1: ref_mag=12.95 +/- 0.02 new_mean_mag=11.9948 delta=0.96 (need > 0.90)
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry filter KEPT candidate at 23:49:41.59 +06:26:29.5: ref_mag=13.44 +/- 0.03 new_mean_mag=12.3357 delta=1.10 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:48.44 +07:18:46.8: 13.97 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Forced photometry filter KEPT candidate at 23:49:48.44 +07:18:46.8: ref_mag=14.02 +/- 0.05 new_mean_mag=12.8575 delta=1.16 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:30:08.17 +04:52:55.7: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter REJECTED candidate at 00:30:08.17 +04:52:55.7: ref_mag=12.14 +/- 0.01 new_mean_mag=11.5941 delta=0.55 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:04.70 +06:35:43.9: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:05:30.04 +08:49:24.1: 13.44 +/- 0.04 detection
Forced photometry filter KEPT candidate at 23:49:04.70 +06:35:43.9: ref_mag=13.36 +/- 0.03 new_mean_mag=12.3258 delta=1.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter KEPT candidate at 00:05:30.04 +08:49:24.1: ref_mag=13.43 +/- 0.03 new_mean_mag=12.5045 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:48:46.50 +05:52:40.8: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter KEPT candidate at 23:48:46.50 +05:52:40.8: ref_mag=13.33 +/- 0.03 new_mean_mag=12.3126 delta=1.02 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:29:52.36 +02:39:28.5: 12.72 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry filter KEPT candidate at 00:29:52.36 +02:39:28.5: ref_mag=12.72 +/- 0.02 new_mean_mag=11.6657 delta=1.06 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:44.45 +05:31:23.1: 13.58 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:19.13 +06:33:14.4: 12.74 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:13:08.19 +09:11:18.6: 12.99 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:44.45 +05:31:23.1: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Forced photometry filter KEPT candidate at 23:49:44.45 +05:31:23.1: ref_mag=13.58 +/- 0.04 new_mean_mag=12.6268 delta=0.96 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:19.13 +06:33:14.4: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Forced photometry filter KEPT candidate at 23:50:19.13 +06:33:14.4: ref_mag=12.69 +/- 0.02 new_mean_mag=11.7753 delta=0.92 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:13:08.19 +09:11:18.6: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 00:13:08.19 +09:11:18.6: ref_mag=12.96 +/- 0.02 new_mean_mag=12.0476 delta=0.92 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:30.45 +06:21:20.9: 12.50 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:30.45 +06:21:20.9: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter KEPT candidate at 23:51:30.45 +06:21:20.9: ref_mag=12.45 +/- 0.01 new_mean_mag=11.5114 delta=0.94 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:07.09 +06:53:20.5: 14.05 +/- 0.08 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:07.09 +06:53:20.5: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Forced photometry filter KEPT candidate at 23:49:07.09 +06:53:20.5: ref_mag=13.98 +/- 0.05 new_mean_mag=12.8247 delta=1.15 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:29.36 +06:05:49.1: 13.89 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:29.36 +06:05:49.1: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Forced photometry filter KEPT candidate at 23:51:29.36 +06:05:49.1: ref_mag=13.85 +/- 0.05 new_mean_mag=12.7010 delta=1.15 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:01.72 +06:44:13.4: 12.54 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:46.23 +06:20:27.8: 12.85 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:02.80 +06:29:13.1: 13.93 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:01.72 +06:44:13.4: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 23:51:01.72 +06:44:13.4: ref_mag=12.54 +/- 0.01 new_mean_mag=11.6143 delta=0.92 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:46.23 +06:20:27.8: 12.88 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:02.80 +06:29:13.1: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter KEPT candidate at 23:50:46.23 +06:20:27.8: ref_mag=12.87 +/- 0.02 new_mean_mag=11.9063 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 23:51:02.80 +06:29:13.1: ref_mag=13.91 +/- 0.05 new_mean_mag=12.7011 delta=1.21 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:36:23.40 +05:33:43.9: 13.51 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:36:23.40 +05:33:43.9: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Forced photometry filter KEPT candidate at 23:36:23.40 +05:33:43.9: ref_mag=13.48 +/- 0.04 new_mean_mag=12.4739 delta=1.00 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:04.34 +07:18:18.3: 13.77 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:13:00.27 +08:58:53.9: 13.13 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:21.44 +06:34:17.3: 12.66 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:04.34 +07:18:18.3: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter KEPT candidate at 23:50:04.34 +07:18:18.3: ref_mag=13.79 +/- 0.04 new_mean_mag=12.5656 delta=1.23 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:13:00.27 +08:58:53.9: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 00:13:00.27 +08:58:53.9: ref_mag=13.15 +/- 0.02 new_mean_mag=12.0767 delta=1.08 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:21.44 +06:34:17.3: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Forced photometry filter KEPT candidate at 23:49:21.44 +06:34:17.3: ref_mag=12.67 +/- 0.02 new_mean_mag=11.6879 delta=0.98 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:03.24 +06:48:18.8: 13.68 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:03.24 +06:48:18.8: 13.65 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:48:52.40 +07:07:27.9: 13.66 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Forced photometry filter KEPT candidate at 23:49:03.24 +06:48:18.8: ref_mag=13.66 +/- 0.04 new_mean_mag=12.3560 delta=1.31 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:48:52.40 +07:07:27.9: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter KEPT candidate at 23:48:52.40 +07:07:27.9: ref_mag=13.69 +/- 0.04 new_mean_mag=12.5179 delta=1.17 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:57.91 +07:32:13.1: 13.65 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:57.91 +07:32:13.1: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Forced photometry filter KEPT candidate at 23:49:57.91 +07:32:13.1: ref_mag=13.71 +/- 0.04 new_mean_mag=12.6014 delta=1.11 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:36.21 +07:01:54.9: 13.65 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:36.21 +07:01:54.9: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Forced photometry filter KEPT candidate at 23:50:36.21 +07:01:54.9: ref_mag=13.70 +/- 0.04 new_mean_mag=12.5256 delta=1.17 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:32.19 +06:54:17.1: 12.89 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:29:37.86 +02:52:07.9: 13.11 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:21.54 +07:10:28.3: 11.98 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:32.19 +06:54:17.1: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry filter KEPT candidate at 23:49:32.19 +06:54:17.1: ref_mag=12.88 +/- 0.02 new_mean_mag=11.7950 delta=1.09 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:51.39 +06:50:13.0: 13.33 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:29:37.86 +02:52:07.9: 13.20 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:21.54 +07:10:28.3: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter KEPT candidate at 00:29:37.86 +02:52:07.9: ref_mag=13.16 +/- 0.03 new_mean_mag=12.2278 delta=0.93 (need > 0.90)
Forced photometry filter KEPT candidate at 23:50:21.54 +07:10:28.3: ref_mag=11.99 +/- 0.01 new_mean_mag=11.0718 delta=0.92 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:51.39 +06:50:13.0: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Forced photometry filter KEPT candidate at 23:50:51.39 +06:50:13.0: ref_mag=13.34 +/- 0.03 new_mean_mag=12.2876 delta=1.05 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:30:09.06 +10:46:31.3: 13.32 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:30:09.06 +10:46:31.3: 13.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Forced photometry filter KEPT candidate at 23:30:09.06 +10:46:31.3: ref_mag=13.34 +/- 0.04 new_mean_mag=12.4178 delta=0.92 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:15.10 +07:11:39.8: 13.80 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:15.10 +07:11:39.8: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry filter KEPT candidate at 23:50:15.10 +07:11:39.8: ref_mag=13.82 +/- 0.05 new_mean_mag=12.5203 delta=1.30 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:38:46.98 +05:49:18.3: 13.50 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:38:46.98 +05:49:18.3: 13.33 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:31.15 +07:06:10.2: 12.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Forced photometry filter KEPT candidate at 23:38:46.98 +05:49:18.3: ref_mag=13.39 +/- 0.04 new_mean_mag=12.3915 delta=1.00 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:31.15 +07:06:10.2: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter KEPT candidate at 23:50:31.15 +07:06:10.2: ref_mag=12.82 +/- 0.02 new_mean_mag=11.8567 delta=0.97 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:13:11.31 +09:08:45.5: 13.62 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:13:11.31 +09:08:45.5: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Forced photometry filter KEPT candidate at 00:13:11.31 +09:08:45.5: ref_mag=13.63 +/- 0.04 new_mean_mag=12.5199 delta=1.11 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:29.24 +06:50:51.2: 13.61 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:29.24 +06:50:51.2: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Forced photometry filter KEPT candidate at 23:49:29.24 +06:50:51.2: ref_mag=13.62 +/- 0.04 new_mean_mag=12.6560 delta=0.97 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:49.20 +07:21:11.6: 13.78 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:49.20 +07:21:11.6: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter KEPT candidate at 23:50:49.20 +07:21:11.6: ref_mag=13.74 +/- 0.04 new_mean_mag=12.6341 delta=1.11 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:29:22.55 +02:31:55.6: 13.07 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:01.28 +07:08:09.1: 14.13 +/- 0.09 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:29:22.55 +02:31:55.6: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Forced photometry filter KEPT candidate at 00:29:22.55 +02:31:55.6: ref_mag=13.13 +/- 0.03 new_mean_mag=12.1150 delta=1.02 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:01.28 +07:08:09.1: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.05
Forced photometry filter KEPT candidate at 23:50:01.28 +07:08:09.1: ref_mag=14.03 +/- 0.05 new_mean_mag=12.8037 delta=1.22 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:25.62 +07:37:12.9: 13.74 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:25.62 +07:37:12.9: 13.70 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:07:07.06 +09:06:42.1: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Forced photometry filter KEPT candidate at 23:50:25.62 +07:37:12.9: ref_mag=13.72 +/- 0.04 new_mean_mag=12.5905 delta=1.13 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:29:48.02 +02:47:31.8: 13.26 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:07:07.06 +09:06:42.1: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 00:07:07.06 +09:06:42.1: ref_mag=13.21 +/- 0.02 new_mean_mag=12.2772 delta=0.94 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:29:48.02 +02:47:31.8: 13.55 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Forced photometry filter KEPT candidate at 00:29:48.02 +02:47:31.8: ref_mag=13.39 +/- 0.04 new_mean_mag=12.2784 delta=1.11 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:01.59 +06:15:51.3: 12.54 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:01.59 +06:15:51.3: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter KEPT candidate at 23:51:01.59 +06:15:51.3: ref_mag=12.47 +/- 0.01 new_mean_mag=11.5353 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:29:25.11 +02:37:36.8: 12.54 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:29:25.11 +02:37:36.8: 12.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.02
Forced photometry filter KEPT candidate at 00:29:25.11 +02:37:36.8: ref_mag=12.59 +/- 0.02 new_mean_mag=11.6412 delta=0.95 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:22.51 +06:18:17.5: 12.79 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:22.51 +06:18:17.5: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter KEPT candidate at 23:50:22.51 +06:18:17.5: ref_mag=12.84 +/- 0.02 new_mean_mag=11.8695 delta=0.97 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:34.19 +07:06:06.9: 13.25 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:34.19 +07:06:06.9: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Forced photometry filter KEPT candidate at 23:49:34.19 +07:06:06.9: ref_mag=13.23 +/- 0.03 new_mean_mag=12.1648 delta=1.06 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:00.74 +07:37:13.7: 13.24 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:00.74 +07:37:13.7: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Forced photometry filter KEPT candidate at 23:50:00.74 +07:37:13.7: ref_mag=13.26 +/- 0.03 new_mean_mag=12.1552 delta=1.10 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:48:48.30 +06:52:28.8: 13.21 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:18.69 +06:18:01.8: 13.58 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:18.69 +06:18:01.8: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter KEPT candidate at 23:51:18.69 +06:18:01.8: ref_mag=13.50 +/- 0.03 new_mean_mag=12.4115 delta=1.09 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:48:48.30 +06:52:28.8: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry filter KEPT candidate at 23:48:48.30 +06:52:28.8: ref_mag=13.20 +/- 0.03 new_mean_mag=12.2890 delta=0.91 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:51:10.62 +06:13:16.5: 13.74 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:29:58.13 +02:32:04.8: 13.02 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:51:10.62 +06:13:16.5: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry filter KEPT candidate at 23:51:10.62 +06:13:16.5: ref_mag=13.73 +/- 0.04 new_mean_mag=12.5315 delta=1.20 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:09.14 +07:20:00.6: 13.83 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:29:58.13 +02:32:04.8: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry filter KEPT candidate at 00:29:58.13 +02:32:04.8: ref_mag=13.08 +/- 0.03 new_mean_mag=12.0202 delta=1.06 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:09.14 +07:20:00.6: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Forced photometry filter KEPT candidate at 23:50:09.14 +07:20:00.6: ref_mag=13.92 +/- 0.05 new_mean_mag=12.8133 delta=1.10 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:17:34.44 +01:20:47.5: 13.18 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:17:34.44 +01:20:47.5: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry filter KEPT candidate at 00:17:34.44 +01:20:47.5: ref_mag=13.16 +/- 0.03 new_mean_mag=12.2237 delta=0.94 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:13.17 +06:52:49.7: 14.51 +/- 0.13 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:13.17 +06:52:49.7: 14.61 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.09
Forced photometry filter KEPT candidate at 23:50:13.17 +06:52:49.7: ref_mag=14.56 +/- 0.09 new_mean_mag=13.0737 delta=1.49 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:25.12 +07:31:17.5: 13.71 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:25.12 +07:31:17.5: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter KEPT candidate at 23:49:25.12 +07:31:17.5: ref_mag=13.65 +/- 0.04 new_mean_mag=12.5357 delta=1.11 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:12:47.76 +09:06:03.0: 13.67 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:12:47.76 +09:06:03.0: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Forced photometry filter KEPT candidate at 00:12:47.76 +09:06:03.0: ref_mag=13.61 +/- 0.04 new_mean_mag=12.5285 delta=1.08 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:49:53.52 +07:00:44.7: 12.10 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:49:53.52 +07:00:44.7: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter KEPT candidate at 23:49:53.52 +07:00:44.7: ref_mag=12.09 +/- 0.01 new_mean_mag=11.1490 delta=0.94 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:23.79 +06:49:07.3: 13.98 +/- 0.08 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:23.79 +06:49:07.3: 13.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Forced photometry filter KEPT candidate at 23:50:23.79 +06:49:07.3: ref_mag=13.94 +/- 0.05 new_mean_mag=12.7600 delta=1.18 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:06.36 +05:27:16.2: 13.56 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:06.36 +05:27:16.2: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Forced photometry filter KEPT candidate at 23:50:06.36 +05:27:16.2: ref_mag=13.46 +/- 0.03 new_mean_mag=12.5277 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:27:24.56 +03:00:28.4: 12.96 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 00:24:55.93 +00:57:09.3: 12.96 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:33.02 +07:21:04.6: 12.06 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:52:01.58 +06:10:59.8: 13.83 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:27:24.56 +03:00:28.4: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Forced photometry filter KEPT candidate at 00:27:24.56 +03:00:28.4: ref_mag=13.00 +/- 0.03 new_mean_mag=12.0487 delta=0.95 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:24:55.93 +00:57:09.3: 13.07 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Forced photometry filter REJECTED candidate at 00:24:55.93 +00:57:09.3: ref_mag=13.02 +/- 0.03 new_mean_mag=12.1256 delta=0.89 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:33.02 +07:21:04.6: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry filter KEPT candidate at 23:50:33.02 +07:21:04.6: ref_mag=12.06 +/- 0.01 new_mean_mag=11.1251 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:52:01.58 +06:10:59.8: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Forced photometry filter KEPT candidate at 23:52:01.58 +06:10:59.8: ref_mag=13.89 +/- 0.05 new_mean_mag=12.6853 delta=1.20 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:59.88 +07:21:02.4: 12.43 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:59.88 +07:21:02.4: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 23:50:59.88 +07:21:02.4: ref_mag=12.38 +/- 0.01 new_mean_mag=11.4498 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:48:23.86 +07:01:55.8: 13.68 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:18.34 +06:14:27.1: 13.39 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:48:23.86 +07:01:55.8: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Forced photometry filter KEPT candidate at 23:48:23.86 +07:01:55.8: ref_mag=13.64 +/- 0.04 new_mean_mag=12.5697 delta=1.07 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:18.34 +06:14:27.1: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter KEPT candidate at 23:50:18.34 +06:14:27.1: ref_mag=13.43 +/- 0.03 new_mean_mag=12.4964 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-17_21-12-09_20.00sec_-14.90C_LIGHT_0080.fits at 23:50:19.37 +06:48:13.5: 12.93 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:50:19.37 +06:48:13.5: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter KEPT candidate at 23:50:19.37 +06:48:13.5: ref_mag=12.95 +/- 0.02 new_mean_mag=11.9567 delta=0.99 (need > 0.90)
Adding exclusion_list_local.txt__out01205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24867.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 97s
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: 31s
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Considering the candidate 33426_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
The candidate 33426_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369 did not pass the final checks
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Considering the candidate 33427_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
The candidate 33427_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369 did not pass the final checks
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Considering the candidate 33536_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
The candidate 33536_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369 did not pass the final checks
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Considering the candidate 13458_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 13458_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 15611_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 15611_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 06142_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 06142_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 23898_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 23898_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 11404_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 11404_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 07091_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 07091_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 13943_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 13943_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 16658_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 16658_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 05998_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 05998_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 13570_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 13570_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 14174_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 14174_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 12614_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12614_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 14988_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 14988_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 13043_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 13043_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 14222_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 14222_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 13817_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 13817_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 16449_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 16449_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 11413_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 11413_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 06621_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 06621_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 13493_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 13493_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 12849_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12849_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 11941_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 11941_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 10746_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 10746_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 12205_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12205_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 12557_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12557_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 11762_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 11762_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 24444_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 24444_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 12762_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12762_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 01205_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 01205_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 11732_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 11732_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 15723_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 15723_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 11991_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 11991_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 06137_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 06137_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 12725_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12725_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 11296_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 11296_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 23474_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 23474_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 11928_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 11928_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 10524_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 10524_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 06261_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 06261_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 24277_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 24277_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 14454_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 14454_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 23724_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 23724_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 14321_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 14321_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 12003_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12003_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 10510_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 10510_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 12638_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12638_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 14365_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 14365_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 14622_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 14622_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 23455_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 23455_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 11353_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 11353_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 19785_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 19785_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 12635_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12635_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 10790_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 10790_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 06280_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 06280_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 12233_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12233_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 12830_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12830_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 16848_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 16848_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 24867_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 24867_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 18863_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
The candidate 18863_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369 did not pass the final checks
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Considering the candidate 11265_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 11265_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 14743_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 14743_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 11277_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 11277_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 12208_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12208_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
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Considering the candidate 14548_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 14548_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12853_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
Preparing report for the candidate 12853_fd_Psc-04-Q1b1x1_2026-07-10_04-26-58_20.00sec_-0.00C_LIGHTs_0369
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 133s
Prepared the HTML report for the field Psc-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:50:25.49 +07:08:38.0
23:49:38.88 +06:54:37.1
23:49:42.53 +06:52:19.6
23:49:31.54 +06:47:35.2
23:30:09.06 +10:46:31.3
00:13:08.19 +09:11:18.6
00:13:11.31 +09:08:45.5
00:13:14.27 +09:08:39.1
00:07:07.06 +09:06:42.1
00:12:47.76 +09:06:03.0
00:13:00.27 +08:58:53.9
00:05:30.04 +08:49:24.1
23:50:00.74 +07:37:13.7
23:50:25.62 +07:37:12.9
23:49:57.91 +07:32:13.1
23:49:25.12 +07:31:17.5
23:50:33.02 +07:21:04.6
23:50:59.88 +07:21:02.4
23:50:49.20 +07:21:11.6
23:50:09.14 +07:20:00.6
23:49:48.44 +07:18:46.8
23:50:04.34 +07:18:18.3
23:50:15.10 +07:11:39.8
23:50:21.54 +07:10:28.3
23:50:01.28 +07:08:09.1
23:48:52.40 +07:07:27.9
23:50:31.15 +07:06:10.2
23:49:34.19 +07:06:06.9
23:50:36.21 +07:01:54.9
23:48:23.86 +07:01:55.8
23:49:53.52 +07:00:44.7
23:49:32.19 +06:54:17.1
23:49:07.09 +06:53:20.5
23:50:13.17 +06:52:49.7
23:48:48.30 +06:52:28.8
23:49:29.24 +06:50:51.2
23:50:51.39 +06:50:13.0
23:50:23.79 +06:49:07.3
23:49:03.24 +06:48:18.8
23:50:19.37 +06:48:13.5
23:51:01.72 +06:44:13.4
23:49:04.70 +06:35:43.9
23:49:21.44 +06:34:17.3
23:50:19.13 +06:33:14.4
23:51:02.80 +06:29:13.1
23:49:41.59 +06:26:29.5
23:51:30.45 +06:21:20.9
23:50:46.23 +06:20:27.8
23:50:22.51 +06:18:17.5
23:51:18.69 +06:18:01.8
23:51:01.59 +06:15:51.3
23:50:18.34 +06:14:27.1
23:51:10.62 +06:13:16.5
23:52:01.58 +06:10:59.8
23:51:29.36 +06:05:49.1
23:48:46.50 +05:52:40.8
23:38:46.98 +05:49:18.3
23:36:23.40 +05:33:43.9
23:49:44.45 +05:31:23.1
23:50:06.36 +05:27:16.2
00:17:34.44 +01:20:47.5
00:29:58.13 +02:32:04.8
00:29:22.55 +02:31:55.6
00:29:25.11 +02:37:36.8
00:29:52.36 +02:39:28.5
00:29:48.02 +02:47:31.8
00:29:37.86 +02:52:07.9
00:27:24.56 +03:00:28.4
########### Completed Psc-04-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 ####
23:49:42.53 +06:52:19.6
23:49:38.88 +06:54:37.1
23:50:25.49 +07:08:38.0
23:49:31.54 +06:47:35.2
23:49:04.70 +06:35:43.9
23:48:46.50 +05:52:40.8
00:13:14.27 +09:08:39.1
00:29:52.36 +02:39:28.5
23:49:48.44 +07:18:46.8
00:05:30.04 +08:49:24.1
23:49:41.59 +06:26:29.5
23:49:44.45 +05:31:23.1
00:13:08.19 +09:11:18.6
23:50:19.13 +06:33:14.4
23:51:30.45 +06:21:20.9
23:49:07.09 +06:53:20.5
23:51:29.36 +06:05:49.1
23:51:01.72 +06:44:13.4
23:50:46.23 +06:20:27.8
23:51:02.80 +06:29:13.1
23:36:23.40 +05:33:43.9
23:50:04.34 +07:18:18.3
00:13:00.27 +08:58:53.9
23:49:21.44 +06:34:17.3
23:49:03.24 +06:48:18.8
23:48:52.40 +07:07:27.9
23:49:57.91 +07:32:13.1
23:50:36.21 +07:01:54.9
23:49:32.19 +06:54:17.1
23:50:21.54 +07:10:28.3
00:29:37.86 +02:52:07.9
23:50:51.39 +06:50:13.0
23:30:09.06 +10:46:31.3
23:50:15.10 +07:11:39.8
23:38:46.98 +05:49:18.3
23:50:31.15 +07:06:10.2
00:13:11.31 +09:08:45.5
23:49:29.24 +06:50:51.2
23:50:49.20 +07:21:11.6
00:29:22.55 +02:31:55.6
23:50:01.28 +07:08:09.1
23:50:25.62 +07:37:12.9
00:07:07.06 +09:06:42.1
00:29:48.02 +02:47:31.8
23:51:01.59 +06:15:51.3
00:29:25.11 +02:37:36.8
23:50:22.51 +06:18:17.5
23:49:34.19 +07:06:06.9
23:50:00.74 +07:37:13.7
23:48:48.30 +06:52:28.8
23:51:18.69 +06:18:01.8
23:51:10.62 +06:13:16.5
00:29:58.13 +02:32:04.8
23:50:09.14 +07:20:00.6
00:17:34.44 +01:20:47.5
23:50:13.17 +06:52:49.7
23:49:25.12 +07:31:17.5
00:12:47.76 +09:06:03.0
23:49:53.52 +07:00:44.7
23:50:23.79 +06:49:07.3
23:50:06.36 +05:27:16.2
00:27:24.56 +03:00:28.4
23:50:33.02 +07:21:04.6
23:52:01.58 +06:10:59.8
23:50:59.88 +07:21:02.4
23:48:23.86 +07:01:55.8
23:50:18.34 +06:14:27.1
23:50:19.37 +06:48:13.5
###################################################################################
23:49:42.53 +06:52:19.6 -- not an asteroid (will add it to exclusion list)
23:49:38.88 +06:54:37.1 -- not an asteroid (will add it to exclusion list)
23:50:25.49 +07:08:38.0 -- not an asteroid (will add it to exclusion list)
23:49:31.54 +06:47:35.2 -- not an asteroid (will add it to exclusion list)
23:49:04.70 +06:35:43.9 -- not an asteroid (will add it to exclusion list)
23:48:46.50 +05:52:40.8 -- not an asteroid (will add it to exclusion list)
00:13:14.27 +09:08:39.1 -- not an asteroid (will add it to exclusion list)
00:29:52.36 +02:39:28.5 -- not an asteroid (will add it to exclusion list)
23:49:48.44 +07:18:46.8 -- not an asteroid (will add it to exclusion list)
00:05:30.04 +08:49:24.1 -- not an asteroid (will add it to exclusion list)
23:49:41.59 +06:26:29.5 -- not an asteroid (will add it to exclusion list)
23:49:44.45 +05:31:23.1 -- not an asteroid (will add it to exclusion list)
00:13:08.19 +09:11:18.6 -- not an asteroid (will add it to exclusion list)
23:50:19.13 +06:33:14.4 -- not an asteroid (will add it to exclusion list)
23:51:30.45 +06:21:20.9 -- not an asteroid (will add it to exclusion list)
23:49:07.09 +06:53:20.5 -- not an asteroid (will add it to exclusion list)
23:51:29.36 +06:05:49.1 -- not an asteroid (will add it to exclusion list)
23:51:01.72 +06:44:13.4 -- not an asteroid (will add it to exclusion list)
23:50:46.23 +06:20:27.8 -- not an asteroid (will add it to exclusion list)
23:51:02.80 +06:29:13.1 -- not an asteroid (will add it to exclusion list)
23:36:23.40 +05:33:43.9 -- not an asteroid (will add it to exclusion list)
23:50:04.34 +07:18:18.3 -- not an asteroid (will add it to exclusion list)
00:13:00.27 +08:58:53.9 -- not an asteroid (will add it to exclusion list)
23:49:21.44 +06:34:17.3 -- not an asteroid (will add it to exclusion list)
23:49:03.24 +06:48:18.8 -- not an asteroid (will add it to exclusion list)
23:48:52.40 +07:07:27.9 -- not an asteroid (will add it to exclusion list)
23:49:57.91 +07:32:13.1 -- not an asteroid (will add it to exclusion list)
23:50:36.21 +07:01:54.9 -- not an asteroid (will add it to exclusion list)
23:49:32.19 +06:54:17.1 -- not an asteroid (will add it to exclusion list)
23:50:21.54 +07:10:28.3 -- not an asteroid (will add it to exclusion list)
00:29:37.86 +02:52:07.9 -- not an asteroid (will add it to exclusion list)
23:50:51.39 +06:50:13.0 -- not an asteroid (will add it to exclusion list)
23:30:09.06 +10:46:31.3 -- not an asteroid (will add it to exclusion list)
23:50:15.10 +07:11:39.8 -- not an asteroid (will add it to exclusion list)
23:38:46.98 +05:49:18.3 -- not an asteroid (will add it to exclusion list)
23:50:31.15 +07:06:10.2 -- not an asteroid (will add it to exclusion list)
00:13:11.31 +09:08:45.5 -- not an asteroid (will add it to exclusion list)
23:49:29.24 +06:50:51.2 -- not an asteroid (will add it to exclusion list)
23:50:49.20 +07:21:11.6 -- not an asteroid (will add it to exclusion list)
00:29:22.55 +02:31:55.6 -- not an asteroid (will add it to exclusion list)
23:50:01.28 +07:08:09.1 -- not an asteroid (will add it to exclusion list)
23:50:25.62 +07:37:12.9 -- not an asteroid (will add it to exclusion list)
00:07:07.06 +09:06:42.1 -- not an asteroid (will add it to exclusion list)
00:29:48.02 +02:47:31.8 -- not an asteroid (will add it to exclusion list)
23:51:01.59 +06:15:51.3 -- not an asteroid (will add it to exclusion list)
00:29:25.11 +02:37:36.8 -- not an asteroid (will add it to exclusion list)
23:50:22.51 +06:18:17.5 -- not an asteroid (will add it to exclusion list)
23:49:34.19 +07:06:06.9 -- not an asteroid (will add it to exclusion list)
23:50:00.74 +07:37:13.7 -- not an asteroid (will add it to exclusion list)
23:48:48.30 +06:52:28.8 -- not an asteroid (will add it to exclusion list)
23:51:18.69 +06:18:01.8 -- not an asteroid (will add it to exclusion list)
23:51:10.62 +06:13:16.5 -- not an asteroid (will add it to exclusion list)
00:29:58.13 +02:32:04.8 -- not an asteroid (will add it to exclusion list)
23:50:09.14 +07:20:00.6 -- not an asteroid (will add it to exclusion list)
00:17:34.44 +01:20:47.5 -- not an asteroid (will add it to exclusion list)
23:50:13.17 +06:52:49.7 -- not an asteroid (will add it to exclusion list)
23:49:25.12 +07:31:17.5 -- not an asteroid (will add it to exclusion list)
00:12:47.76 +09:06:03.0 -- not an asteroid (will add it to exclusion list)
23:49:53.52 +07:00:44.7 -- not an asteroid (will add it to exclusion list)
23:50:23.79 +06:49:07.3 -- not an asteroid (will add it to exclusion list)
23:50:06.36 +05:27:16.2 -- not an asteroid (will add it to exclusion list)
00:27:24.56 +03:00:28.4 -- not an asteroid (will add it to exclusion list)
23:50:33.02 +07:21:04.6 -- not an asteroid (will add it to exclusion list)
23:52:01.58 +06:10:59.8 -- not an asteroid (will add it to exclusion list)
23:50:59.88 +07:21:02.4 -- not an asteroid (will add it to exclusion list)
23:48:23.86 +07:01:55.8 -- not an asteroid (will add it to exclusion list)
23:50:18.34 +06:14:27.1 -- not an asteroid (will add it to exclusion list)
23:50:19.37 +06:48:13.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:05:30.04 +08:49:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:07.06 +09:06:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:47.76 +09:06:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:00.27 +08:58:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:08.19 +09:11:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:11.31 +09:08:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:14.27 +09:08:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:34.44 +01:20:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:24.56 +03:00:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:22.55 +02:31:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:25.11 +02:37:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:37.86 +02:52:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:48.02 +02:47:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:52.36 +02:39:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:58.13 +02:32:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:09.06 +10:46:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:23.40 +05:33:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:46.98 +05:49:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:23.86 +07:01:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:46.50 +05:52:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:48.30 +06:52:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:52.40 +07:07:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:03.24 +06:48:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:04.70 +06:35:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:07.09 +06:53:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:21.44 +06:34:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:25.12 +07:31:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:29.24 +06:50:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:31.54 +06:47:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:32.19 +06:54:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:34.19 +07:06:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:38.88 +06:54:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:41.59 +06:26:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:42.53 +06:52:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:44.45 +05:31:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:48.44 +07:18:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:53.52 +07:00:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:57.91 +07:32:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:00.74 +07:37:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:01.28 +07:08:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:04.34 +07:18:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:06.36 +05:27:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:09.14 +07:20:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:13.17 +06:52:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:15.10 +07:11:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:18.34 +06:14:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:19.13 +06:33:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:19.37 +06:48:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:21.54 +07:10:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:22.51 +06:18:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:23.79 +06:49:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:25.49 +07:08:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:25.62 +07:37:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:31.15 +07:06:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:33.02 +07:21:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:36.21 +07:01:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:46.23 +06:20:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:49.20 +07:21:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:51.39 +06:50:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:59.88 +07:21:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:01.59 +06:15:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:01.72 +06:44:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:02.80 +06:29:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:10.62 +06:13:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:18.69 +06:18:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:29.36 +06:05:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:30.45 +06:21:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:01.58 +06:10:59.8 -- 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)
00:05:30.04 +08:49:24.1 -- not a known variable star
00:07:07.06 +09:06:42.1 -- not a known variable star
00:12:47.76 +09:06:03.0 -- not a known variable star
00:13:00.27 +08:58:53.9 -- not a known variable star
00:13:08.19 +09:11:18.6 -- not a known variable star
00:13:11.31 +09:08:45.5 -- not a known variable star
00:13:14.27 +09:08:39.1 -- not a known variable star
00:17:34.44 +01:20:47.5 -- not a known variable star
00:27:24.56 +03:00:28.4 -- not a known variable star
00:29:22.55 +02:31:55.6 -- not a known variable star
00:29:25.11 +02:37:36.8 -- not a known variable star
00:29:37.86 +02:52:07.9 -- not a known variable star
00:29:48.02 +02:47:31.8 -- not a known variable star
00:29:52.36 +02:39:28.5 -- not a known variable star
00:29:58.13 +02:32:04.8 -- not a known variable star
23:30:09.06 +10:46:31.3 -- not a known variable star
23:36:23.40 +05:33:43.9 -- not a known variable star
23:38:46.98 +05:49:18.3 -- not a known variable star
23:48:23.86 +07:01:55.8 -- not a known variable star
23:48:46.50 +05:52:40.8 -- not a known variable star
23:48:48.30 +06:52:28.8 -- not a known variable star
23:48:52.40 +07:07:27.9 -- not a known variable star
23:49:03.24 +06:48:18.8 -- not a known variable star
23:49:04.70 +06:35:43.9 -- not a known variable star
23:49:07.09 +06:53:20.5 -- not a known variable star
23:49:21.44 +06:34:17.3 -- not a known variable star
23:49:25.12 +07:31:17.5 -- not a known variable star
23:49:29.24 +06:50:51.2 -- not a known variable star
23:49:31.54 +06:47:35.2 -- not a known variable star
23:49:32.19 +06:54:17.1 -- not a known variable star
23:49:34.19 +07:06:06.9 -- not a known variable star
23:49:38.88 +06:54:37.1 -- not a known variable star
23:49:41.59 +06:26:29.5 -- not a known variable star
23:49:42.53 +06:52:19.6 -- not a known variable star
23:49:44.45 +05:31:23.1 -- not a known variable star
23:49:48.44 +07:18:46.8 -- a known variable star
23:49:53.52 +07:00:44.7 -- not a known variable star
23:49:57.91 +07:32:13.1 -- not a known variable star
23:50:00.74 +07:37:13.7 -- not a known variable star
23:50:01.28 +07:08:09.1 -- not a known variable star
23:50:04.34 +07:18:18.3 -- a known variable star
23:50:06.36 +05:27:16.2 -- not a known variable star
23:50:09.14 +07:20:00.6 -- not a known variable star
23:50:13.17 +06:52:49.7 -- not a known variable star
23:50:15.10 +07:11:39.8 -- not a known variable star
23:50:18.34 +06:14:27.1 -- not a known variable star
23:50:19.13 +06:33:14.4 -- not a known variable star
23:50:19.37 +06:48:13.5 -- not a known variable star
23:50:21.54 +07:10:28.3 -- not a known variable star
23:50:22.51 +06:18:17.5 -- not a known variable star
23:50:23.79 +06:49:07.3 -- not a known variable star
23:50:25.49 +07:08:38.0 -- not a known variable star
23:50:25.62 +07:37:12.9 -- not a known variable star
23:50:31.15 +07:06:10.2 -- not a known variable star
23:50:33.02 +07:21:04.6 -- a known variable star
23:50:36.21 +07:01:54.9 -- not a known variable star
23:50:46.23 +06:20:27.8 -- not a known variable star
23:50:49.20 +07:21:11.6 -- not a known variable star
23:50:51.39 +06:50:13.0 -- not a known variable star
23:50:59.88 +07:21:02.4 -- not a known variable star
23:51:01.59 +06:15:51.3 -- not a known variable star
23:51:01.72 +06:44:13.4 -- not a known variable star
23:51:02.80 +06:29:13.1 -- not a known variable star
23:51:10.62 +06:13:16.5 -- not a known variable star
23:51:18.69 +06:18:01.8 -- not a known variable star
23:51:29.36 +06:05:49.1 -- not a known variable star
23:51:30.45 +06:21:20.9 -- not a known variable star
23:52:01.58 +06:10:59.8 -- not a known variable star
Found 65 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
68 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 68 (excluding asteroids and hot pixels, 65 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)2461231.89335062 -observatory V36
07:32:10.14 +17:07:55.4 Mercury (5.1mag)
10:11:49.67 +12:39:52.3 Venus (-4.1mag)
04:24:17.96 +21:25:31.9 Mars (1.3mag)
08:16:42.92 +20:11:21.6 Jupiter (-1.8mag)
00:55:51.19 +03:20:29.9 Saturn (0.7mag)
04:07:14.53 +20:45:04.7 Uranus (5.8mag)
00:17:01.49 +00:20:41.0 Neptune (7.8mag)
20:30:54.70 -23:18:01.8 Pluto (14.4mag)
03:14:21.44 +22:36:27.4 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 361 Jul 10 05:12 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461231.89335062:
08:16:50.10 +20:10:56.4 Io (6.1mag)
08:16:46.52 +20:11:10.0 Europa (6.3mag)
08:17:00.14 +20:10:19.3 Ganymede (5.6mag)
08:17:10.71 +20:09:38.9 Callisto (6.8mag)
08:15:14.29 +19:55:32.4 Himalia (15.7mag)
08:16:43.36 +20:11:20.8 Thebe (16.6mag)
08:14:35.61 +20:00:01.3 Elara (17.6mag)
08:20:15.22 +20:05:30.4 Pasiphae (17.8mag)
08:21:40.62 +20:16:27.0 Carme (19.0mag)
00:55:41.16 +03:20:20.2 Titan (8.5mag)
00:55:45.95 +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)
00:55:51.85 +03:17:43.3 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 05:13 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.89335062:
17:46:01.77 -32:57:30.4 JWST
16:21:14.34 +47:25:55.8 Chandra
05:01:08.87 +47:52:15.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 05:12 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.89335062 -observatory V36
02:36:19.75 +14:26:00.0 17.9mag P/1996 R2 (Lagerkvist)
18:17:54.38 -34:21:49.5 13.7mag P/2010 H2 (Vales)
06:25:43.01 -68:08:25.4 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:49.25 +32:26:51.7 17.6mag C/2017 K2 (PANSTARRS)
17:03:06.23 +16:02:53.6 18.0mag C/2021 G2 (ATLAS)
01:48:02.60 +08:18:20.2 15.4mag P/2021 N1 (ZTF)
22:59:30.38 +32:17:08.0 17.3mag C/2022 E2 (ATLAS)
06:12:26.86 +26:55:33.5 16.7mag C/2022 N2 (PANSTARRS)
09:55:33.10 +29:46:44.5 16.8mag C/2022 QE78 (ATLAS)
09:09:45.74 +05:00:00.1 17.8mag C/2022 R6 (PANSTARRS)
18:07:11.53 +21:17:32.3 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:34.96 -11:23:19.3 17.7mag P/2023 B1 (PANSTARRS)
21:49:11.04 +67:37:16.2 17.8mag C/2023 H5 (Lemmon)
16:30:48.13 -10:04:57.2 13.9mag C/2023 R1 (PANSTARRS)
08:00:43.40 +65:42:38.4 17.9mag C/2024 A1 (ATLAS)
07:32:52.20 +30:00:19.9 14.6mag C/2024 E1 (Wierzchos)
15:16:18.34 +15:19:46.1 17.5mag C/2024 G6 (ATLAS)
19:41:15.38 +39:24:04.6 13.8mag C/2024 J3 (ATLAS)
21:47:32.39 +46:00:34.6 17.8mag C/2024 R4 (PANSTARRS)
04:49:40.73 -13:47:38.4 15.7mag C/2024 T5 (ATLAS)
06:34:36.49 +29:03:46.7 18.0mag C/2025 J1 (Borisov)
07:14:22.18 -12:53:35.9 16.5mag C/2025 R3 (PANSTARRS)
09:56:08.41 +22:26:06.3 17.6mag C/2025 V2 (Rankin)
12:44:37.85 +03:56:09.9 17.1mag C/2025 Y1 (ATLAS)
16:51:49.98 +79:07:16.1 17.4mag C/2026 A2 (Bok)
02:46:19.23 +45:14:30.5 16.7mag C/2026 B2 (Sun-Gao)
11:25:32.27 +04:33:05.8 16.9mag A/2026 E1
21:19:05.83 -15:05:27.5 7.3mag 10P/Tempel
11:13:28.47 -01:53:20.1 16.1mag 29P/Schwassmann-Wachmann
04:00:13.93 +29:33:28.0 17.8mag 47P/Ashbrook-Jackson
10:08:09.82 +13:59:53.9 17.0mag 63P/Wild
00:48:22.82 -05:05:33.4 15.5mag 65P/Gunn
08:27:04.98 +34:13:01.1 17.9mag 76P/West-Kohoutek-Ikemura
04:27:29.89 +20:10:51.9 13.7mag 78P/Gehrels
02:22:24.08 +10:36:55.3 16.2mag 88P/Howell
06:35:39.26 +30:31:57.2 15.7mag 93P/Lovas
04:21:07.97 +31:07:30.0 16.9mag 114P/Wiseman-Skiff
08:08:47.75 +30:41:56.5 15.2mag 123P/West-Hartley
10:48:12.53 +01:10:12.5 16.8mag 124P/Mrkos
04:51:47.68 +20:48:51.3 16.2mag 128P/Shoemaker-Holt
05:36:20.02 +19:42:49.8 17.8mag 131P/Mueller
00:01:33.39 +02:56:12.9 17.9mag 139P/Vaisala-Oterma
07:13:42.95 +17:00:43.0 15.5mag 141P-D/Machholz
03:16:52.02 -21:06:09.1 15.5mag 161P/Hartley-IRAS
05:33:12.73 +33:57:28.1 15.3mag 162P/SidingSpring
19:04:22.01 +15:06:25.6 14.7mag 169P/NEAT
01:41:07.70 +07:36:12.4 17.7mag 220P/McNaught
16:35:57.72 -08:23:12.7 17.0mag 235P/LINEAR
08:45:22.39 +33:17:44.6 17.9mag 240P/NEAT
20:42:09.27 -49:34:47.2 17.8mag 259P/Garradd
01:59:25.24 +12:06:50.8 15.7mag 260P/McNaught
05:37:21.07 +36:50:47.2 17.4mag 295P/LINEAR
15:06:36.63 +06:03:11.8 17.6mag 391P/Kowalski
08:34:38.45 +19:40:30.5 17.9mag 450P/LONEOS
07:51:49.91 +39:12:46.1 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 05:12 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 05:12 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 10 05:12 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
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
20:31:34.503 -19:06:25.71 AT 2026spq 2026-07-07.33 22.7105
-rw-r--r-- 1 apache apache 30K Jul 10 05:13 tns_transients_list.txt
