This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC
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 10.3437 2461231.8437 11.82 01:01:18.28 +13:48:00.6
126.58470 -49.00159 galactic Psc Second-epoch detections are separated by 1.5" and 9.8 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 | 01:01:18.28 +13:48:00.6 (user input) | T | P | (position from user input) J-Ks=0.521+/-0.030 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 01:01:18.28 +13:48:00.6: 12.95 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 01:01:18.28 +13:48:00.6: 12.94 +/- 0.02 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,2461231.8437,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 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 10.3437 2461231.8437 12.03 00:34:59.71 +14:40:09.9
116.98184 -48.01228 galactic Psc Second-epoch detections are separated by 1.3" and 10.2 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 | 00:34:59.71 +14:40:09.9 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.031 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:34:59.71 +14:40:09.9: 13.26 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:34:59.71 +14:40:09.9: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 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,2461231.8437,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 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 10.3437 2461231.8437 12.03 00:56:43.00 +12:12:36.1
124.96603 -50.64087 galactic Psc Second-epoch detections are separated by 2.2" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:56:43.00 +12:12:36.1 (user input) | T | P | (position from user input) J-Ks=0.333+/-0.033 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:43.00 +12:12:36.1: 13.33 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:43.00 +12:12:36.1: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 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,2461231.8437,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 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 10.3437 2461231.8437 11.93 00:37:09.68 +14:31:12.6
117.74364 -48.20771 galactic Psc Second-epoch detections are separated by 2.4" and 10.1 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 | 00:37:09.68 +14:31:12.6 (user input) | T | P | (position from user input) J-Ks=0.574+/-0.028 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:09.68 +14:31:12.6: 13.31 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:09.68 +14:31:12.6: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8437,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.97 00:49:01.91 +14:37:14.4
122.05786 -48.24700 galactic Psc Second-epoch detections are separated by 0.7" and 10.0 pix
The object was found in VSX 1" Gaia DR3 2777943172985783808
Type: ROT
# Max. Min./Amp. JD0 Period
12.830 G 12.860 G G
The object was not found in astcheck.
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:49:01.91 +14:37:14.4: 13.03 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:49:01.91 +14:37:14.4: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2777943172985783808,2461231.8437,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2777943172985783808 20260710.3437 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.82 00:57:33.73 +14:43:29.7
125.15038 -48.12045 galactic Psc Second-epoch detections are separated by 1.4" and 9.8 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 | 00:57:33.73 +14:43:29.7 (user input) | T | P | (position from user input) J-Ks=0.301+/-0.033 (F)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:57:33.73 +14:43:29.7: 12.74 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:57:33.73 +14:43:29.7: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 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
target,2461231.8437,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 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 10.3437 2461231.8437 11.65 00:55:28.78 +15:07:53.5
124.38211 -47.72884 galactic Psc Second-epoch detections are separated by 0.6" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:55:28.78 +15:07:53.5 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.030 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:55:28.78 +15:07:53.5: 12.63 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:55:28.78 +15:07:53.5: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 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
target,2461231.8437,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.58 00:56:29.14 +12:36:09.8
124.85809 -50.25015 galactic Psc Second-epoch detections are separated by 0.9" and 10.1 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 2776526692771586048 | 00:56:29.10 +12:36:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.346+/-0.028 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:29.14 +12:36:09.8: 12.61 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:29.14 +12:36:09.8: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 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 2776526692771586048,2461231.8437,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2776526692771586048 20260710.3437 11.58CV 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 10.3437 2461231.8437 11.65 00:51:48.29 +13:19:26.9
123.06949 -49.54751 galactic Psc Second-epoch detections are separated by 0.4" and 10.0 pix
The object was found in VSX 1" Gaia DR3 2776848815318667264
Type: ROT
# Max. Min./Amp. JD0 Period
12.550 G 12.590 G G
The object was not found in astcheck.
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:51:48.29 +13:19:26.9: 12.61 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:51:48.29 +13:19:26.9: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 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 2776848815318667264,2461231.8437,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2776848815318667264 20260710.3437 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.39 00:38:07.41 +14:03:09.1
118.03703 -48.69264 galactic Psc Second-epoch detections are separated by 0.4" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2779387450228399360 | 00:38:07.43 +14:03:08.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.428+/-0.030 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:38:07.41 +14:03:09.1: 12.24 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:38:07.41 +14:03:09.1: 12.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.26 +/- 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 2779387450228399360,2461231.8437,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2779387450228399360 20260710.3437 11.39CV 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 10.3437 2461231.8437 11.88 00:35:43.44 +14:41:35.3
117.24746 -48.00510 galactic Psc Second-epoch detections are separated by 2.4" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:35:43.44 +14:41:35.3 (user input) | T | P | (position from user input) J-Ks=0.552+/-0.030 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:35:43.44 +14:41:35.3: 13.20 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:35:43.44 +14:41:35.3: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8437,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 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 10.3437 2461231.8437 11.54 00:36:08.16 +13:40:43.3
117.25847 -49.02442 galactic Psc Second-epoch detections are separated by 1.2" and 9.8 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 | 00:36:08.16 +13:40:43.3 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.028 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:36:08.16 +13:40:43.3: 12.56 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:36:08.16 +13:40:43.3: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 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
target,2461231.8437,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.3437 2461231.8437 11.66 00:52:36.32 +12:59:09.9
123.37329 -49.88466 galactic Psc Second-epoch detections are separated by 1.1" and 10.0 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 | Gaia DR3 2776775182399366272 | 00:52:36.30 +12:59:08.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.032 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:52:36.32 +12:59:09.9: 12.55 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:52:36.32 +12:59:09.9: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 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 2776775182399366272,2461231.8437,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2776775182399366272 20260710.3437 11.66CV 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 10.3437 2461231.8437 11.18 00:37:32.92 +15:19:52.2
117.98077 -47.40701 galactic Psc Second-epoch detections are separated by 0.5" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2780560148098853888 | 00:37:32.95 +15:19:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=10.722+/- (unrealisitic color!)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:32.92 +15:19:52.2: 12.19 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:32.92 +15:19:52.2: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 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 2780560148098853888,2461231.8437,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2780560148098853888 20260710.3437 11.18CV 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 10.3437 2461231.8437 11.53 00:56:17.94 +12:29:38.8
124.79192 -50.36008 galactic Psc Second-epoch detections are separated by 1.2" and 9.8 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 | Gaia DR3 2776502189982482688 | 00:56:17.99 +12:29:39.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.790+/-0.034 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:17.94 +12:29:38.8: 12.51 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:17.94 +12:29:38.8: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 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 2776502189982482688,2461231.8437,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2776502189982482688 20260710.3437 11.53CV 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 10.3437 2461231.8437 11.21 00:56:49.65 +14:31:13.5
124.89406 -48.33080 galactic Psc Second-epoch detections are separated by 0.2" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2777408496801546112 | 00:56:49.70 +14:31:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.315+/-0.030 (F)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:49.65 +14:31:13.5: 12.14 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:49.65 +14:31:13.5: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 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 2777408496801546112,2461231.8437,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2777408496801546112 20260710.3437 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.09 00:37:33.03 +14:21:24.7
117.86461 -48.37820 galactic Psc Second-epoch detections are separated by 0.8" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2779606905877352192 | 00:37:33.06 +14:21:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.759+/-0.026 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:33.03 +14:21:24.7: 12.13 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:33.03 +14:21:24.7: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 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 2779606905877352192,2461231.8437,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2779606905877352192 20260710.3437 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 12.03 00:50:04.13 +13:53:09.0
122.42561 -48.98457 galactic Psc Second-epoch detections are separated by 0.9" and 10.0 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 | 00:50:04.13 +13:53:09.0 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.030 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:50:04.13 +13:53:09.0: 13.16 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:50:04.13 +13:53:09.0: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8437,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 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 10.3437 2461231.8437 11.23 00:52:24.52 +13:15:10.7
123.29653 -49.61809 galactic Psc Second-epoch detections are separated by 0.8" and 9.8 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 | Gaia DR3 2776835101487568512 | 00:52:24.53 +13:15:10.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.335+/-0.030 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:52:24.52 +13:15:10.7: 12.07 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:52:24.52 +13:15:10.7: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 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 2776835101487568512,2461231.8437,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2776835101487568512 20260710.3437 11.23CV 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 10.3437 2461231.8437 11.35 00:55:55.61 +14:25:36.4
124.57001 -48.43069 galactic Psc Second-epoch detections are separated by 3.3" and 10.2 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 2777782090236858880 | 00:55:55.58 +14:25:37.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.389+/-0.028 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:55:55.61 +14:25:36.4: 12.45 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:55:55.61 +14:25:36.4: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 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 2777782090236858880,2461231.8437,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2777782090236858880 20260710.3437 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 12.01 00:36:59.45 +14:27:00.3
117.67308 -48.27409 galactic Psc Second-epoch detections are separated by 1.4" and 9.8 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 | 00:36:59.45 +14:27:00.3 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.028 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:36:59.45 +14:27:00.3: 13.16 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:36:59.45 +14:27:00.3: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8437,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.72 01:08:30.18 +13:22:39.0
129.30182 -49.28307 galactic Psc Second-epoch detections are separated by 0.8" and 9.8 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 | 01:08:30.18 +13:22:39.0 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.030 (F)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 01:08:30.18 +13:22:39.0: 12.81 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 01:08:30.18 +13:22:39.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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
target,2461231.8437,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 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 10.3437 2461231.8437 10.80 00:52:23.70 +13:22:56.6
123.29025 -49.48869 galactic Psc Second-epoch detections are separated by 0.6" and 9.8 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 | Gaia DR3 2776850047973756416 | 00:52:23.67 +13:22:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.759+/-0.029 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:52:23.70 +13:22:56.6: 11.65 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:52:23.70 +13:22:56.6: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 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 2776850047973756416,2461231.8437,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2776850047973756416 20260710.3437 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.20 00:52:26.46 +13:20:22.7
123.30787 -49.53138 galactic Psc Second-epoch detections are separated by 0.6" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2776849639952389376 | 00:52:26.45 +13:20:21.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.780+/-0.029 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:52:26.46 +13:20:22.7: 11.99 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:52:26.46 +13:20:22.7: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 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 2776849639952389376,2461231.8437,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2776849639952389376 20260710.3437 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.69 00:36:58.85 +14:25:09.2
117.66555 -48.30464 galactic Psc Second-epoch detections are separated by 1.6" and 9.8 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 | 00:36:58.85 +14:25:09.2 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.028 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:36:58.85 +14:25:09.2: 12.79 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:36:58.85 +14:25:09.2: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 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
target,2461231.8437,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 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 10.3437 2461231.8437 11.71 00:54:46.10 +14:23:31.6
124.14839 -48.47177 galactic Psc Second-epoch detections are separated by 1.2" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:54:46.10 +14:23:31.6 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5) J-Ks=0.485+/-0.032 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:54:46.10 +14:23:31.6: 12.76 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:54:46.10 +14:23:31.6: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 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
target,2461231.8437,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 11.71CV 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 10.3437 2461231.8437 11.86 00:55:51.73 +12:29:41.6
124.62482 -50.36232 galactic Psc Second-epoch detections are separated by 0.3" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2776501674586407040 | 00:55:51.69 +12:29:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.619+/-0.036 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:55:51.73 +12:29:41.6: 12.75 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:55:51.73 +12:29:41.6: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 2776501674586407040,2461231.8437,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2776501674586407040 20260710.3437 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 10.3437 2461231.8437 12.04 00:56:27.53 +14:45:45.4
124.74928 -48.09142 galactic Psc Second-epoch detections are separated by 1.7" and 10.1 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 | 00:56:27.53 +14:45:45.4 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.032 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:27.53 +14:45:45.4: 13.13 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:27.53 +14:45:45.4: 13.20 +/- 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,2461231.8437,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.79 00:36:39.76 +15:08:20.4
117.64213 -47.58094 galactic Psc Second-epoch detections are separated by 1.2" and 10.1 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 2780550802249435648 | 00:36:39.65 +15:08:20.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:36:39.76 +15:08:20.4: 12.73 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:36:39.76 +15:08:20.4: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 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 2780550802249435648,2461231.8437,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2780550802249435648 20260710.3437 11.79CV 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 10.3437 2461231.8437 11.74 00:37:25.04 +13:37:23.0
117.72440 -49.10688 galactic Psc Second-epoch detections are separated by 2.7" and 10.3 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 | 00:37:25.04 +13:37:23.0 (user input) | T | P | (position from user input) J-Ks=0.313+/-0.028 (F)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:25.04 +13:37:23.0: 12.74 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:25.04 +13:37:23.0: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 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
target,2461231.8437,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 11.74CV 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 10.3437 2461231.8437 11.93 00:37:47.87 +13:55:11.1
117.90160 -48.81873 galactic Psc Second-epoch detections are separated by 1.5" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:37:47.87 +13:55:11.1 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.028 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:47.87 +13:55:11.1: 13.53 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:47.87 +13:55:11.1: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 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,2461231.8437,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.95 01:08:12.65 +13:16:38.7
129.20878 -49.38980 galactic Psc Second-epoch detections are separated by 1.4" and 10.0 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 | 01:08:12.65 +13:16:38.7 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.029 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 01:08:12.65 +13:16:38.7: 13.12 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 01:08:12.65 +13:16:38.7: 13.19 +/- 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,2461231.8437,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.38 00:38:02.16 +14:19:43.0
118.03776 -48.41574 galactic Psc Second-epoch detections are separated by 1.3" and 9.8 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 | Gaia DR3 2779604255881911808 | 00:38:02.26 +14:19:43.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.398+/-0.028 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:38:02.16 +14:19:43.0: 12.42 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:38:02.16 +14:19:43.0: 12.32 +/- 0.01 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 2779604255881911808,2461231.8437,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2779604255881911808 20260710.3437 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.38 01:08:14.04 +13:13:02.1
129.22666 -49.44910 galactic Psc Second-epoch detections are separated by 0.4" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2584733996160125952 | 01:08:14.02 +13:13:02.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.305+/-0.028 (F)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 01:08:14.04 +13:13:02.1: 12.39 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 01:08:14.04 +13:13:02.1: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 2584733996160125952,2461231.8437,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2584733996160125952 20260710.3437 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.10 00:35:28.95 +14:07:19.1
117.08068 -48.56842 galactic Psc Second-epoch detections are separated by 0.9" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2779587488329577088 | 00:35:28.96 +14:07:18.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.428+/-0.030 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:35:28.95 +14:07:19.1: 11.96 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:35:28.95 +14:07:19.1: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 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 2779587488329577088,2461231.8437,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2779587488329577088 20260710.3437 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 10.97 00:37:12.64 +15:07:56.7
117.83672 -47.59853 galactic Psc Second-epoch detections are separated by 0.7" and 9.8 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 | Gaia DR3 2779801004039346688 | 00:37:12.62 +15:07:56.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.244+/-0.029 (F)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:12.64 +15:07:56.7: 11.94 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:12.64 +15:07:56.7: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 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 2779801004039346688,2461231.8437,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2779801004039346688 20260710.3437 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.78 00:50:18.01 +13:47:52.7
122.51025 -49.07285 galactic Psc Second-epoch detections are separated by 0.2" and 10.0 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 | 00:50:18.01 +13:47:52.7 (user input) | T | P | (position from user input) J-Ks=0.618+/-0.029 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:50:18.01 +13:47:52.7: 12.70 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:50:18.01 +13:47:52.7: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 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
target,2461231.8437,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.87 00:35:50.50 +14:38:19.0
117.28243 -48.06198 galactic Psc Second-epoch detections are separated by 1.4" and 9.8 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 | 00:35:50.50 +14:38:19.0 (user input) | T | P | (position from user input) J-Ks=0.184+/-0.030 (F)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:35:50.50 +14:38:19.0: 13.05 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:35:50.50 +14:38:19.0: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 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,2461231.8437,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.86 00:38:15.29 +14:18:13.3
118.11449 -48.44470 galactic Psc Second-epoch detections are separated by 1.3" and 9.8 pix
The object was found in VSX 1" Gaia DR3 2779603263745088512
Type: ROT
# Max. Min./Amp. JD0 Period
12.800 G 12.820 G K
The object was not found in astcheck.
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:38:15.29 +14:18:13.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:38:15.29 +14:18:13.3: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 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 2779603263745088512,2461231.8437,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2779603263745088512 20260710.3437 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 10.3437 2461231.8437 11.95 01:08:35.41 +13:20:33.6
129.33960 -49.31556 galactic Psc Second-epoch detections are separated by 0.8" and 10.1 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 2584745270449780736 | 01:08:37.83 +13:21:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.392+/-0.030 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 01:08:35.41 +13:20:33.6: 13.33 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 01:08:35.41 +13:20:33.6: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 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 2584745270449780736,2461231.8437,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2584745270449780736 20260710.3437 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.84 00:35:23.86 +14:30:47.5
117.10492 -48.17699 galactic Psc Second-epoch detections are separated by 1.3" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:35:23.86 +14:30:47.5 (user input) | T | P | (position from user input) J-Ks=0.470+/-0.029 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:35:23.86 +14:30:47.5: 13.03 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:35:23.86 +14:30:47.5: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 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,2461231.8437,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 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 10.3437 2461231.8437 11.91 00:56:29.29 +14:50:04.7
124.75673 -48.01922 galactic Psc Second-epoch detections are separated by 0.7" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2778185095608011776 | 00:56:30.20 +14:50:48.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.494+/-0.032 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:29.29 +14:50:04.7: 13.00 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:29.29 +14:50:04.7: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 2778185095608011776,2461231.8437,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2778185095608011776 20260710.3437 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.96 00:52:13.28 +13:32:57.0
123.22403 -49.32214 galactic Psc Second-epoch detections are separated by 1.8" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:52:13.28 +13:32:57.0 (user input) | T | P | (position from user input) J-Ks=0.553+/-0.028 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:52:13.28 +13:32:57.0: 13.30 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:52:13.28 +13:32:57.0: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 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,2461231.8437,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 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
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 12.04 00:52:37.36 +13:29:32.5
123.37429 -49.37837 galactic Psc Second-epoch detections are separated by 0.9" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:52:37.36 +13:29:32.5 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.033 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:52:37.36 +13:29:32.5: 13.25 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:52:37.36 +13:29:32.5: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 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,2461231.8437,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.26 01:08:41.22 +13:12:24.3
129.39701 -49.44835 galactic Psc Second-epoch detections are separated by 1.4" and 9.8 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 | Gaia DR3 2584734305397771648 | 01:08:41.19 +13:12:25.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.611+/-0.028 (K)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 01:08:41.22 +13:12:24.3: 12.29 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 01:08:41.22 +13:12:24.3: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 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 2584734305397771648,2461231.8437,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2584734305397771648 20260710.3437 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.68 00:37:32.65 +15:12:16.0
117.96422 -47.53325 galactic Psc Second-epoch detections are separated by 1.8" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:37:32.65 +15:12:16.0 (user input) | T | P | (position from user input) J-Ks=0.382+/-0.024 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:32.65 +15:12:16.0: 12.96 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:32.65 +15:12:16.0: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 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,2461231.8437,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3437 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.75 00:56:31.74 +11:35:41.5
124.92440 -51.25719 galactic Psc Second-epoch detections are separated by 0.9" and 10.0 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 | Gaia DR3 2582783329389003648 | 00:56:31.72 +11:35:41.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.356+/-0.029 (G)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:31.74 +11:35:41.5: 12.69 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:31.74 +11:35:41.5: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 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 2582783329389003648,2461231.8437,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2582783329389003648 20260710.3437 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 12.13 00:56:24.36 +14:40:07.6
124.73423 -48.18558 galactic Psc Second-epoch detections are separated by 2.4" and 9.7 pix
The object was found in VSX 1" Gaia DR3 2778164793298293888
Type: ROT
# Max. Min./Amp. JD0 Period
13.210 G 13.240 G G
The object was not found in astcheck.
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:24.36 +14:40:07.6: 13.46 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:24.36 +14:40:07.6: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 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 2778164793298293888,2461231.8437,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2778164793298293888 20260710.3437 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3437 2461231.8437 11.59 00:36:21.65 +13:43:02.0
117.34666 -48.99095 galactic Psc Second-epoch detections are separated by 1.0" and 9.8 pix
The object was found in VSX 0" Gaia DR3 2778999013386315264
Type: VAR
# Max. Min./Amp. JD0 Period
12.300 G 12.320 G 0.017956300000 K
The object was not found in astcheck.
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:36:21.65 +13:43:02.0: 12.66 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:36:21.65 +13:43:02.0: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 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 2778999013386315264,2461231.8437,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2778999013386315264 20260710.3437 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.63018125 09.01.2026 03:07:17.660 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
First image: 2461049.63018125 09.01.2026 03:07:17.660 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
Last image: 2461231.84400557 10.07.2026 08:15:12.081 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.60
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4889
Objects passed selection criteria: 4853
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 2785.25
Average stars matched: 2719.75 (97.6483 %)
Memory usage VmPeak: 111676 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 06:26:50 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: 2461049.63018125 09.01.2026 03:07:17.660 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
First image: 2461049.63018125 09.01.2026 03:07:17.660 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
Last image: 2461231.84400557 10.07.2026 08:15:12.081 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 53
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 11 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): 27453
Objects passed selection criteria: 27364
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 16848.2
Average stars matched: 16330 (96.924 %)
Memory usage VmPeak: 133452 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 06:29:10 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
SExtractor catalog cache: saved Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.cat to cache
SExtractor catalog cache: saved Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.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-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.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: 2461231.84346693
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits exists and is non-empty
Saving wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits to local_wcs_cache/
'wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits' -> 'local_wcs_cache/wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits'
wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits exists and is non-empty
Saving wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits to local_wcs_cache/
'wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits' -> 'local_wcs_cache/wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits'
wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits exists and is non-empty
Saving wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits to local_wcs_cache/
'wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits' -> 'local_wcs_cache/wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits'
wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits exists and is non-empty
Saving wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits to local_wcs_cache/
'wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits' -> 'local_wcs_cache/wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits (1st reference image)
verification OK: wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:53:20.378 +13:59:58.19 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-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits (1st new image)
verification OK: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
Image size: 937.8'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:53:13.993 +14:01:25.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:53:20.378 +13:59:58.19
Second-epoch image center 00:53:13.993 +14:01:25.62
Angular distance between the image centers 0.0354 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits (2nd new image)
verification OK: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
Image size: 937.8'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:53:17.231 +14:02:01.04 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:53:20.378 +13:59:58.19
Second-epoch image center 00:53:17.231 +14:02:01.04
Angular distance between the image centers 0.0364 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 00:53:13.993 +14:01:25.62
Second-epoch second image center 00:53:17.231 +14:02:01.04
Angular distance between the image centers 0.01638 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-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits &> /tmp/tmp.rZ6eIK8nAx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits &> /tmp/tmp.n1vg8Yy1wn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits &> /tmp/tmp.GYCNMo9OBL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits &> /tmp/tmp.KTTQm0UYhP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.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-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits and wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.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-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits and wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat
Found non-empty wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits and wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat
The reference image (wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits) and catalog (wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat) found
'wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat' -> 'wcsmag.cat'
Read 7072 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.1026 to 21.6285 deg, Dec +8.6113 to +19.2850 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 5.1026 to 21.6285 deg, Dec 8.6113 to 19.2850 deg
Loaded 4673 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): 3734 out of 3960 total matches.
Matched with Tycho-2 3960 out of 7072 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.894000
a=0.000000 b=1.000000 c=22.894000
From vast_summary.log: estimated ref. image limiting mag.: -7.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7072 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.1026 to 21.6285 deg, Dec +8.6113 to +19.2850 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 5.1026 to 21.6285 deg, Dec 8.6113 to 19.2850 deg
Loaded 4673 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): 3734 out of 3960 total matches.
Matched with Tycho-2 3960 out of 7072 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits:
Forced-photometry filter: calibrated wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits -> calib.txt_param_ref_wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits (aperture=5.9)
Read 6269 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.1026 to 21.6286 deg, Dec +8.6114 to +19.2850 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 5.1026 to 21.6286 deg, Dec 8.6114 to 19.2850 deg
Loaded 4673 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): 3743 out of 3896 total matches.
Matched with Tycho-2 3896 out of 6269 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits:
Forced-photometry filter: calibrated wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits -> calib.txt_param_ref_wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
2.1 pix Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
2.3 pix fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
2.3 pix fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
2.0 pix wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
2.1 pix wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
Limiting magnitude estimates:
15.3 mag. Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
15.0 mag. Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
11.9 mag. fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
11.6 mag. fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
All-image limiting magnitude estimate: 11.6 (SNR ) 9.4 (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.rZ6eIK8nAx (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.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-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits' -> 'wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
WCS_IMAGE_NAME=wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
WCS-calibrated image found: wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
Checking if the catalog wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits alredy exist and is non-empty...
Catalog wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
WCS catalog name: wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=522, bad_region=1629, passed=7072
Got 7072 stars (including 5015 good ones) from the SExtractor catalog wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat
util/solve_plate_with_UCAC5 got 7072 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 5595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 5595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 5595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits N_match=960 sigma_overall_arcsec=0.304 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.273 sigma_q3_arcsec=0.289 sigma_q4_arcsec=0.247 n_q1=315 n_q2=198 n_q3=285 n_q4=162 worst_quadrant_to_overall_ratio=1.183
The image catalog is written to wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits -region wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.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.n1vg8Yy1wn (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.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-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits' -> 'wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
WCS_IMAGE_NAME=wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
WCS-calibrated image found: wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
Checking if the catalog wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits alredy exist and is non-empty...
Catalog wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
WCS catalog name: wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=413, bad_region=1431, passed=6269
Got 6269 stars (including 4507 good ones) from the SExtractor catalog wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat
util/solve_plate_with_UCAC5 got 6269 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 4972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 4973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 4973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits N_match=958 sigma_overall_arcsec=0.265 sigma_q1_arcsec=0.298 sigma_q2_arcsec=0.223 sigma_q3_arcsec=0.253 sigma_q4_arcsec=0.243 n_q1=319 n_q2=197 n_q3=286 n_q4=156 worst_quadrant_to_overall_ratio=1.126
The image catalog is written to wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits -region wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.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.GYCNMo9OBL (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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
WCS_IMAGE_NAME=wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
WCS-calibrated image found: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
Checking if the catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
WCS catalog name: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=32, bad_region=108, passed=563
Got 563 stars (including 429 good ones) from the SExtractor catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat
util/solve_plate_with_UCAC5 got 563 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 411 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 411 matched stars entering correct_measured_positions(), 341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 411 matched stars entering correct_measured_positions(), 377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 410 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 409 matched stars entering correct_measured_positions(), 376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 409 matched stars entering correct_measured_positions(), 376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 409 stars left (next iteration limit 452)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits N_match=409 sigma_overall_arcsec=0.572 sigma_q1_arcsec=0.530 sigma_q2_arcsec=0.638 sigma_q3_arcsec=0.613 sigma_q4_arcsec=0.514 n_q1=101 n_q2=49 n_q3=177 n_q4=82 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits -region wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.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.KTTQm0UYhP (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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
WCS_IMAGE_NAME=wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
WCS-calibrated image found: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
Checking if the catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
WCS catalog name: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=26, bad_region=117, passed=583
Got 583 stars (including 441 good ones) from the SExtractor catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat
util/solve_plate_with_UCAC5 got 583 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 547 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 420 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 420 matched stars entering correct_measured_positions(), 362 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 420 matched stars entering correct_measured_positions(), 400 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 547 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 419 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 418 matched stars entering correct_measured_positions(), 404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 418 matched stars entering correct_measured_positions(), 404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 418 stars left (next iteration limit 462)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits N_match=418 sigma_overall_arcsec=0.525 sigma_q1_arcsec=0.507 sigma_q2_arcsec=0.445 sigma_q3_arcsec=0.616 sigma_q4_arcsec=0.474 n_q1=109 n_q2=61 n_q3=174 n_q4=74 worst_quadrant_to_overall_ratio=1.174
The image catalog is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits -region wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.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-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits sigma_overall=0.304 worst_q_ratio=1.183
ref2=Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits sigma_overall=0.265 worst_q_ratio=1.126
new1=fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits sigma_overall=0.572 worst_q_ratio=1.116
new2=fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits sigma_overall=0.525 worst_q_ratio=1.174
reference average sigma_overall=0.2845 worst_q_ratio=1.1545
warn-on-ratio threshold: 2.0x reference
###################################
WCS_QUALITY_RETRY: 1st new image (fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits) flagged: sigma=0.572 (ref avg 0.2845), ratio=1.116 (ref avg 1.1545), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
WCS_IMAGE_NAME=wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/lib/make_outxyls_for_astrometric_calibration found 552 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out21109.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out21109.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
log-odds ratio 317.319 (6.45531e+137), 36 match, 0 conflict, 200 distractors, 42 index.
RA,Dec = (13.2699,14.0365), pixel scale 5.95174 arcsec/pix.
Hit/miss: Hit/miss: +++++-++-+++-+-+-++-+-+--+++++++-+------+-------+--+--+-+---------------------+----+---------------+
Field 1: solved with index index-4115.fits.
Field 1 solved: writing to file ./out21109.solved to indicate this.
Field: out21109.xyls
Field center: (RA,Dec) = (13.305836, 14.023301) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:53:13.401, +14:01:23.882).
Field size: 15.7423 x 10.5325 degrees
Field rotation angle: up is -0.894786 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits' -> 'fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 10 06:28 fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
-rw-r--r-- 1 apache apache 12K Jul 10 06:28 out21109.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits for reading... done!
Creating new image file (wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits (fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out21109.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out21109.axy"...
Only searching for solutions within 15.67 degrees of RA,Dec (13.3067,14.0241)
log-odds ratio 143.01 (1.28376e+62), 15 match, 0 conflict, 237 distractors, 18 index.
RA,Dec = (13.3144,14.0182), pixel scale 5.95181 arcsec/pix.
Hit/miss: Hit/miss: +--++++-+-+--+-++-+--+--------------------+-------------------------------+-------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out21109.solved to indicate this.
Field: out21109.xyls
Field center: (RA,Dec) = (13.306595, 14.023531) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:53:13.583, +14:01:24.711).
Field size: 15.7402 x 10.5325 degrees
Field rotation angle: up is -0.895177 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 10 06:28 fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
-rw-r--r-- 1 apache apache 12K Jul 10 06:28 out21109.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits for reading... done!
Creating new image file (wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 3961 sources.
Solving...
Reading file "./wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.axy"...
Verifying WCS using indices with quads of size [63.3866, 950.203] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
log-odds ratio 58.5588 (2.7024e+25), 6 match, 0 conflict, 27 distractors, 6 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: ---+-------+-+--+--+------------+(best)-------------------------------------------------------------------
--> log-odds 58.5588
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 187.952 (4.23202e+81), 18 match, 0 conflict, 110 distractors, 18 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+-+------++-++-++-+--+-------+-+---+---+++-------------------+-------------------------------------
--> log-odds 187.952
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 349.022 (3.78846e+151), 35 match, 0 conflict, 103 distractors, 42 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+++-+-+-+++-++-++-+--+-++++--+-+---+-+-+++------+-+----------+-+-------+--------------------+------
--> log-odds 349.022
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 610.407 (1.24841e+265), 74 match, 0 conflict, 504 distractors, 88 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+++-+++++++-++-++-+--+-+++++-+-+--++++-+++-++--++-++-+----+--+-+-+---+-+-------+-+-----+----+--+---
--> log-odds 610.407
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 1298.73 (inf), 161 match, 0 conflict, 497 distractors, 197 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+++-++++++++++-++-++++++++++++++++++++-++++++--++-++-+-++-+-++-+++---+-+--++++-+-++-+--+-++-++-++--
--> log-odds 1298.73
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 2201.9 (inf), 304 match, 0 conflict, 1354 distractors, 364 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+++-+++++++++++++-+++++++++++++++++++++++++++--+++++++-++++-++++++---+-+--++++-++++-+--++++-+++++++
--> log-odds 2201.9
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 3842.39 (inf), 565 match, 0 conflict, 1526 distractors, 726 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+++-+++++++++++++-+++++++++++++++++++++++++++--+++++++-++++-+++++++--+++--++++-++++-+-+++++-+++++++
--> log-odds 3842.39
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 6850.73 (inf), 1091 match, 0 conflict, 2094 distractors, 1452 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+++-+++++++++++++-+++++++++++++++++++++++++++--+++++++-++++-+++++++--+++--++++-++++-+++++++-+++++++
--> log-odds 6850.73
Verifying WCS using indices with quads of size [63.3866, 950.203] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
log-odds ratio 58.5588 (2.7024e+25), 6 match, 0 conflict, 27 distractors, 6 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: ---+-------+-+--+--+------------+(best)-------------------------------------------------------------------
--> log-odds 58.5588
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 187.952 (4.23202e+81), 18 match, 0 conflict, 110 distractors, 18 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+-+------++-++-++-+--+-------+-+---+---+++-------------------+-------------------------------------
--> log-odds 187.952
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 349.022 (3.78846e+151), 35 match, 0 conflict, 103 distractors, 42 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+++-+-+-+++-++-++-+--+-++++--+-+---+-+-+++------+-+----------+-+-------+--------------------+------
--> log-odds 349.022
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 610.407 (1.24841e+265), 74 match, 0 conflict, 504 distractors, 88 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+++-+++++++-++-++-+--+-+++++-+-+--++++-+++-++--++-++-+----+--+-+-+---+-+-------+-+-----+----+--+---
--> log-odds 610.407
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 1298.73 (inf), 161 match, 0 conflict, 497 distractors, 197 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+++-++++++++++-++-++++++++++++++++++++-++++++--++-++-+-++-+-++-+++---+-+--++++-+-++-+--+-++-++-++--
--> log-odds 1298.73
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 2201.9 (inf), 304 match, 0 conflict, 1354 distractors, 364 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+++-+++++++++++++-+++++++++++++++++++++++++++--+++++++-++++-++++++---+-+--++++-++++-+--++++-+++++++
--> log-odds 2201.9
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 3842.39 (inf), 565 match, 0 conflict, 1526 distractors, 726 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+++-+++++++++++++-+++++++++++++++++++++++++++--+++++++-++++-+++++++--+++--++++-++++-+-+++++-+++++++
--> log-odds 3842.39
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 6850.73 (inf), 1091 match, 0 conflict, 2094 distractors, 1452 index.
RA,Dec = (13.3058,14.0227), pixel scale 5.95366 arcsec/pix.
Hit/miss: Hit/miss: -+++-+++++++++++++-+++++++++++++++++++++++++++--+++++++-++++-+++++++--+++--++++-++++-+++++++-+++++++
--> log-odds 6850.73
Got 16 solutions.
Field: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
Field center: (RA,Dec) = (13.305628, 14.022997) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:53:13.351, +14:01:22.788).
Field size: 15.7399 x 10.5344 degrees
Field rotation angle: up is -0.899249 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.new"...
renamed 'wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.new' -> 'wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits'
Checking if the catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
verification OK: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
Generating wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat from image00003.cat
Catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits created.
verification OK: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
verification OK: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
Image size: 940.3'x625.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:53:13.552 +14:01:25.81 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 563 stars ###
'wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/correct_sextractor_wcs_catalog_usingxy2sky39412.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
WCS catalog name: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=32, bad_region=108, passed=563
Got 563 stars (including 429 good ones) from the SExtractor catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat
util/solve_plate_with_UCAC5 got 563 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.3'
Seting catalog search parameters based on the expected field of view 940.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013060 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010448 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 412 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 411 matched stars entering correct_measured_positions(), 337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.00"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 411 matched stars entering correct_measured_positions(), 373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.03"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 412 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 411 matched stars entering correct_measured_positions(), 375 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.16"
Accuracy estimation diagnostic: 411 matched stars entering correct_measured_positions(), 375 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.12"
Excluding outliers - 411 stars left (next iteration limit 452)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits N_match=411 sigma_overall_arcsec=1.462 sigma_q1_arcsec=1.567 sigma_q2_arcsec=1.895 sigma_q3_arcsec=1.273 sigma_q4_arcsec=1.389 n_q1=101 n_q2=49 n_q3=178 n_q4=83 worst_quadrant_to_overall_ratio=1.296
The image catalog is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits -region wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 1st new image (fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits): sigma 0.572->1.462, ratio 1.116->1.296; reverting to order 3
WARNING: 1st new image has sigma_overall_arcsec=1.462 -- 5.14x the reference average (0.2845); plate solution may be of low accuracy
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079_astrometric_residuals.png (960 matched stars from wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116_astrometric_residuals.png (958 matched stars from wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340_astrometric_residuals.png (409 matched stars from wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341_astrometric_residuals.png (418 matched stars from wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits'
Saving fully-calibrated image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits'
Preparing the HTML report for the field Psc-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Psc-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
SExtractor catalog cache: saved Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.cat to cache
SExtractor catalog cache: saved Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.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-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
Creating symlink local_wcs_cache/wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.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-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits exists and is non-empty
wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits exists and is non-empty
wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits exists and is non-empty
wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits (1st reference image)
verification OK: wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:53:20.378 +13:59:58.19 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-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits (1st new image)
verification OK: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
Image size: 937.8'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:53:13.993 +14:01:25.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:53:20.378 +13:59:58.19
Second-epoch image center 00:53:13.993 +14:01:25.62
Angular distance between the image centers 0.0354 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits (2nd new image)
verification OK: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
Image size: 937.8'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:53:17.231 +14:02:01.04 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:53:20.378 +13:59:58.19
Second-epoch image center 00:53:17.231 +14:02:01.04
Angular distance between the image centers 0.0364 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 00:53:13.993 +14:01:25.62
Second-epoch second image center 00:53:17.231 +14:02:01.04
Angular distance between the image centers 0.01638 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-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits &> /tmp/tmp.5s7GP5QJHK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits &> /tmp/tmp.2alTIL3HTa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits &> /tmp/tmp.JcajydmlUu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits &> /tmp/tmp.L63MuXiV7p
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.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-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits and wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.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-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits and wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat
Found non-empty wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits and wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat
The reference image (wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits) and catalog (wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat) found
'wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat' -> 'wcsmag.cat'
Read 39559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.0736 to 21.6692 deg, Dec +8.6113 to +19.2903 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 5.0736 to 21.6692 deg, Dec 8.6113 to 19.2903 deg
Loaded 4690 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): 3608 out of 4042 total matches.
Matched with Tycho-2 4042 out of 39559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.775350
a=0.000000 b=1.000000 c=22.775350
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 39559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.0736 to 21.6692 deg, Dec +8.6113 to +19.2903 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 5.0736 to 21.6692 deg, Dec 8.6113 to 19.2903 deg
Loaded 4690 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): 3608 out of 4042 total matches.
Matched with Tycho-2 4042 out of 39559 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits:
Forced-photometry filter: calibrated wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits -> calib.txt_param_ref_wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits (aperture=4.6)
Read 33523 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.0736 to 21.6697 deg, Dec +8.6114 to +19.2916 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 5.0736 to 21.6697 deg, Dec 8.6114 to 19.2916 deg
Loaded 4692 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): 3697 out of 4037 total matches.
Matched with Tycho-2 4037 out of 33523 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits:
Forced-photometry filter: calibrated wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits -> calib.txt_param_ref_wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 49 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
2.1 pix Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
2.0 pix fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
2.0 pix fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
1.9 pix wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
2.1 pix wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
Limiting magnitude estimates:
15.5 mag. Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
15.2 mag. Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
12.1 mag. fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
12.3 mag. fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
All-image limiting magnitude estimate: 12.1 (SNR ) 12.0 (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.5s7GP5QJHK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.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-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits' -> 'wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
WCS_IMAGE_NAME=wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
WCS-calibrated image found: wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
Checking if the catalog wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits alredy exist and is non-empty...
Catalog wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits
WCS catalog name: wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1775, bad_region=7583, passed=39546
Got 39546 stars (including 30450 good ones) from the SExtractor catalog wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat
util/solve_plate_with_UCAC5 got 39546 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 32658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 32658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 32658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits N_match=961 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.365 sigma_q2_arcsec=0.275 sigma_q3_arcsec=0.304 sigma_q4_arcsec=0.238 n_q1=314 n_q2=191 n_q3=295 n_q4=161 worst_quadrant_to_overall_ratio=1.177
The image catalog is written to wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits -region wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.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.2alTIL3HTa (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.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-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits' -> 'wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
WCS_IMAGE_NAME=wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
WCS-calibrated image found: wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
Checking if the catalog wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits alredy exist and is non-empty...
Catalog wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits
WCS catalog name: wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1356, bad_region=6396, passed=33515
Got 33515 stars (including 25966 good ones) from the SExtractor catalog wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat
util/solve_plate_with_UCAC5 got 33515 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 27714 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 27714 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 27714 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits N_match=959 sigma_overall_arcsec=0.264 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.215 sigma_q3_arcsec=0.242 sigma_q4_arcsec=0.244 n_q1=323 n_q2=188 n_q3=291 n_q4=157 worst_quadrant_to_overall_ratio=1.152
The image catalog is written to wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits -region wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.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.JcajydmlUu (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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
WCS_IMAGE_NAME=wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
WCS-calibrated image found: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
Checking if the catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
WCS catalog name: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=136, bad_region=802, passed=5121
Got 5121 stars (including 4198 good ones) from the SExtractor catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat
util/solve_plate_with_UCAC5 got 5121 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 4324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 4324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 4324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits N_match=952 sigma_overall_arcsec=0.526 sigma_q1_arcsec=0.509 sigma_q2_arcsec=0.583 sigma_q3_arcsec=0.571 sigma_q4_arcsec=0.452 n_q1=242 n_q2=117 n_q3=379 n_q4=214 worst_quadrant_to_overall_ratio=1.106
The image catalog is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits -region wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.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.L63MuXiV7p (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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
WCS_IMAGE_NAME=wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
WCS-calibrated image found: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
Checking if the catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
WCS catalog name: wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=67, bad_region=749, passed=5195
Got 5195 stars (including 4382 good ones) from the SExtractor catalog wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat
util/solve_plate_with_UCAC5 got 5195 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 4439 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 4439 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 4439 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits N_match=957 sigma_overall_arcsec=0.521 sigma_q1_arcsec=0.476 sigma_q2_arcsec=0.495 sigma_q3_arcsec=0.568 sigma_q4_arcsec=0.484 n_q1=267 n_q2=138 n_q3=380 n_q4=172 worst_quadrant_to_overall_ratio=1.089
The image catalog is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits -region wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.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-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-14-25_20.00sec_5.00C_LIGHT_0340.fits
Saving fully-calibrated image wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.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-02-Q2b1x1_040302_TTUQ2b1x1_2750249_RE4PhTDC/wcs_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341.fits
Preparing the HTML report for the field Psc-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:55:28.78 +15:07:53.5: 12.63 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 01:01:18.28 +13:48:00.6: 12.95 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:34:59.71 +14:40:09.9: 13.26 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:09.68 +14:31:12.6: 13.31 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:51:48.29 +13:19:26.9: 12.61 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:29.14 +12:36:09.8: 12.61 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:43.00 +12:12:36.1: 13.33 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:38:07.41 +14:03:09.1: 12.24 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:57:33.73 +14:43:29.7: 12.74 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:49:01.91 +14:37:14.4: 13.03 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 01:01:18.28 +13:48:00.6: 12.94 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:55:28.78 +15:07:53.5: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:34:59.71 +14:40:09.9: 13.22 +/- 0.04 detection
Forced photometry filter KEPT candidate at 01:01:18.28 +13:48:00.6: ref_mag=12.95 +/- 0.02 new_mean_mag=11.7789 delta=1.17 (need > 0.90)
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 00:55:28.78 +15:07:53.5: ref_mag=12.64 +/- 0.01 new_mean_mag=11.5960 delta=1.05 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:51:48.29 +13:19:26.9: 12.64 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:09.68 +14:31:12.6: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:29.14 +12:36:09.8: 12.64 +/- 0.02 detection
Forced photometry filter KEPT candidate at 00:34:59.71 +14:40:09.9: ref_mag=13.24 +/- 0.02 new_mean_mag=12.0080 delta=1.24 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:38:07.41 +14:03:09.1: 12.30 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:57:33.73 +14:43:29.7: 12.75 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:43.00 +12:12:36.1: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:49:01.91 +14:37:14.4: 13.09 +/- 0.03 detection
Forced photometry filter KEPT candidate at 00:37:09.68 +14:31:12.6: ref_mag=13.31 +/- 0.02 new_mean_mag=11.9278 delta=1.39 (need > 0.90)
Forced photometry filter KEPT candidate at 00:51:48.29 +13:19:26.9: ref_mag=12.62 +/- 0.01 new_mean_mag=11.6487 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter KEPT candidate at 00:56:29.14 +12:36:09.8: ref_mag=12.62 +/- 0.01 new_mean_mag=11.5139 delta=1.11 (need > 0.90)
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 00:38:07.41 +14:03:09.1: ref_mag=12.26 +/- 0.01 new_mean_mag=11.2766 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 00:56:43.00 +12:12:36.1: ref_mag=13.29 +/- 0.02 new_mean_mag=12.0399 delta=1.25 (need > 0.90)
Forced photometry filter KEPT candidate at 00:57:33.73 +14:43:29.7: ref_mag=12.74 +/- 0.01 new_mean_mag=11.8313 delta=0.91 (need > 0.90)
Forced photometry filter KEPT candidate at 00:49:01.91 +14:37:14.4: ref_mag=13.05 +/- 0.02 new_mean_mag=11.9663 delta=1.08 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:35:43.44 +14:41:35.3: 13.20 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:35:43.44 +14:41:35.3: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 00:35:43.44 +14:41:35.3: ref_mag=13.19 +/- 0.02 new_mean_mag=11.8897 delta=1.30 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:36:08.16 +13:40:43.3: 12.56 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:36:08.16 +13:40:43.3: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 00:36:08.16 +13:40:43.3: ref_mag=12.56 +/- 0.01 new_mean_mag=11.5223 delta=1.03 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:52:36.32 +12:59:09.9: 12.55 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:52:36.32 +12:59:09.9: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 00:52:36.32 +12:59:09.9: ref_mag=12.57 +/- 0.01 new_mean_mag=11.5521 delta=1.01 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:32.92 +15:19:52.2: 12.19 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:17.94 +12:29:38.8: 12.51 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:32.92 +15:19:52.2: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter KEPT candidate at 00:37:32.92 +15:19:52.2: ref_mag=12.18 +/- 0.01 new_mean_mag=11.1504 delta=1.03 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:17.94 +12:29:38.8: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter KEPT candidate at 00:56:17.94 +12:29:38.8: ref_mag=12.51 +/- 0.01 new_mean_mag=11.4629 delta=1.05 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:49.65 +14:31:13.5: 12.14 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:33.03 +14:21:24.7: 12.13 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:49.65 +14:31:13.5: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter KEPT candidate at 00:56:49.65 +14:31:13.5: ref_mag=12.14 +/- 0.01 new_mean_mag=11.1765 delta=0.96 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:50:04.13 +13:53:09.0: 13.16 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:33.03 +14:21:24.7: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter KEPT candidate at 00:37:33.03 +14:21:24.7: ref_mag=12.14 +/- 0.01 new_mean_mag=11.0609 delta=1.08 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:50:04.13 +13:53:09.0: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 00:50:04.13 +13:53:09.0: ref_mag=13.13 +/- 0.02 new_mean_mag=12.0347 delta=1.09 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:52:24.52 +13:15:10.7: 12.07 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:52:24.52 +13:15:10.7: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry filter KEPT candidate at 00:52:24.52 +13:15:10.7: ref_mag=12.08 +/- 0.01 new_mean_mag=11.1191 delta=0.96 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:55:55.61 +14:25:36.4: 12.45 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:55:55.61 +14:25:36.4: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter KEPT candidate at 00:55:55.61 +14:25:36.4: ref_mag=12.44 +/- 0.01 new_mean_mag=11.2530 delta=1.19 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:36:59.45 +14:27:00.3: 13.16 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:36:59.45 +14:27:00.3: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 00:36:59.45 +14:27:00.3: ref_mag=13.13 +/- 0.02 new_mean_mag=12.0019 delta=1.13 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 01:08:30.18 +13:22:39.0: 12.81 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 01:08:30.18 +13:22:39.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 01:08:30.18 +13:22:39.0: ref_mag=12.84 +/- 0.01 new_mean_mag=11.7321 delta=1.11 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:52:23.70 +13:22:56.6: 11.65 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:52:26.46 +13:20:22.7: 11.99 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:52:23.70 +13:22:56.6: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 0.00
Forced photometry filter KEPT candidate at 00:52:23.70 +13:22:56.6: ref_mag=11.65 +/- 0.00 new_mean_mag=10.7456 delta=0.91 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:52:26.46 +13:20:22.7: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter KEPT candidate at 00:52:26.46 +13:20:22.7: ref_mag=12.00 +/- 0.01 new_mean_mag=11.0843 delta=0.92 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:36:58.85 +14:25:09.2: 12.79 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:36:58.85 +14:25:09.2: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 00:36:58.85 +14:25:09.2: ref_mag=12.78 +/- 0.01 new_mean_mag=11.6530 delta=1.13 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:54:46.10 +14:23:31.6: 12.76 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:54:46.10 +14:23:31.6: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 00:54:46.10 +14:23:31.6: ref_mag=12.78 +/- 0.01 new_mean_mag=11.7043 delta=1.07 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:55:51.73 +12:29:41.6: 12.75 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:55:51.73 +12:29:41.6: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 00:55:51.73 +12:29:41.6: ref_mag=12.77 +/- 0.01 new_mean_mag=11.8098 delta=0.96 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:36:39.76 +15:08:20.4: 12.73 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:27.53 +14:45:45.4: 13.13 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:25.04 +13:37:23.0: 12.74 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:36:39.76 +15:08:20.4: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 00:36:39.76 +15:08:20.4: ref_mag=12.70 +/- 0.01 new_mean_mag=11.7964 delta=0.91 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:27.53 +14:45:45.4: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:25.04 +13:37:23.0: 12.73 +/- 0.02 detection
Forced photometry filter KEPT candidate at 00:56:27.53 +14:45:45.4: ref_mag=13.15 +/- 0.02 new_mean_mag=12.0425 delta=1.11 (need > 0.90)
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 00:37:25.04 +13:37:23.0: ref_mag=12.73 +/- 0.01 new_mean_mag=11.6607 delta=1.07 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 01:08:12.65 +13:16:38.7: 13.12 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:47.87 +13:55:11.1: 13.53 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:47.87 +13:55:11.1: 13.54 +/- 0.04 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 01:08:12.65 +13:16:38.7: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Forced photometry filter KEPT candidate at 01:08:12.65 +13:16:38.7: ref_mag=13.15 +/- 0.02 new_mean_mag=11.9456 delta=1.20 (need > 0.90)
Forced photometry filter KEPT candidate at 00:37:47.87 +13:55:11.1: ref_mag=13.53 +/- 0.03 new_mean_mag=11.8968 delta=1.64 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:38:02.16 +14:19:43.0: 12.42 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 01:08:14.04 +13:13:02.1: 12.39 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:38:02.16 +14:19:43.0: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 00:38:02.16 +14:19:43.0: ref_mag=12.38 +/- 0.01 new_mean_mag=11.3789 delta=1.00 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 01:08:14.04 +13:13:02.1: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter KEPT candidate at 01:08:14.04 +13:13:02.1: ref_mag=12.39 +/- 0.01 new_mean_mag=11.3708 delta=1.02 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:35:28.95 +14:07:19.1: 11.96 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:35:28.95 +14:07:19.1: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Forced photometry filter KEPT candidate at 00:35:28.95 +14:07:19.1: ref_mag=11.96 +/- 0.01 new_mean_mag=11.0205 delta=0.94 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:12.64 +15:07:56.7: 11.94 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:12.64 +15:07:56.7: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Forced photometry filter KEPT candidate at 00:37:12.64 +15:07:56.7: ref_mag=11.91 +/- 0.01 new_mean_mag=10.9578 delta=0.95 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:50:18.01 +13:47:52.7: 12.70 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:35:50.50 +14:38:19.0: 13.05 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:38:15.29 +14:18:13.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:50:18.01 +13:47:52.7: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 00:50:18.01 +13:47:52.7: ref_mag=12.71 +/- 0.01 new_mean_mag=11.7457 delta=0.96 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:35:50.50 +14:38:19.0: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 00:35:50.50 +14:38:19.0: ref_mag=13.04 +/- 0.02 new_mean_mag=11.8765 delta=1.17 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:38:15.29 +14:18:13.3: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 00:38:15.29 +14:18:13.3: ref_mag=13.07 +/- 0.02 new_mean_mag=11.8708 delta=1.20 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 01:08:35.41 +13:20:33.6: 13.33 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 01:08:35.41 +13:20:33.6: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter KEPT candidate at 01:08:35.41 +13:20:33.6: ref_mag=13.33 +/- 0.02 new_mean_mag=11.9448 delta=1.38 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:35:23.86 +14:30:47.5: 13.03 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:35:23.86 +14:30:47.5: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 00:35:23.86 +14:30:47.5: ref_mag=12.99 +/- 0.02 new_mean_mag=11.8031 delta=1.19 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:29.29 +14:50:04.7: 13.00 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:52:13.28 +13:32:57.0: 13.30 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:29.29 +14:50:04.7: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Forced photometry filter KEPT candidate at 00:56:29.29 +14:50:04.7: ref_mag=13.00 +/- 0.01 new_mean_mag=11.9048 delta=1.10 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:52:13.28 +13:32:57.0: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter KEPT candidate at 00:52:13.28 +13:32:57.0: ref_mag=13.32 +/- 0.02 new_mean_mag=11.9278 delta=1.39 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:52:37.36 +13:29:32.5: 13.25 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:52:37.36 +13:29:32.5: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 00:52:37.36 +13:29:32.5: ref_mag=13.27 +/- 0.02 new_mean_mag=11.9740 delta=1.30 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 01:08:41.22 +13:12:24.3: 12.29 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 01:08:41.22 +13:12:24.3: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 01:08:41.22 +13:12:24.3: ref_mag=12.31 +/- 0.01 new_mean_mag=11.2352 delta=1.07 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:37:32.65 +15:12:16.0: 12.96 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:37:32.65 +15:12:16.0: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 00:37:32.65 +15:12:16.0: ref_mag=12.94 +/- 0.02 new_mean_mag=11.6603 delta=1.28 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:31.74 +11:35:41.5: 12.69 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:31.74 +11:35:41.5: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 00:56:31.74 +11:35:41.5: ref_mag=12.68 +/- 0.01 new_mean_mag=11.7042 delta=0.98 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:56:24.36 +14:40:07.6: 13.46 +/- 0.03 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:56:24.36 +14:40:07.6: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 00:56:24.36 +14:40:07.6: ref_mag=13.50 +/- 0.02 new_mean_mag=12.1342 delta=1.36 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-08_21-07-17_20.00sec_-15.00C_LIGHT_0079.fits at 00:36:21.65 +13:43:02.0: 12.66 +/- 0.02 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-01-17_21-50-33_20.00sec_-14.90C_LIGHT_0116.fits at 00:36:21.65 +13:43:02.0: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 00:36:21.65 +13:43:02.0: ref_mag=12.63 +/- 0.01 new_mean_mag=11.5636 delta=1.07 (need > 0.90)
Adding exclusion_list_local.txt__out15925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39442.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 89s
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: 24s
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Considering the candidate 22051_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 22051_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
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Considering the candidate 18584_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 18584_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
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Considering the candidate 38140_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 38140_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
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Considering the candidate 19249_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 19249_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
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Considering the candidate 18864_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 18864_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
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Considering the candidate 18400_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 18400_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
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Considering the candidate 16751_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 16751_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
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Considering the candidate 39442_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 39442_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
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Considering the candidate 23940_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 23940_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21035_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 21035_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18524_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 18524_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22546_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 22546_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25208_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 25208_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15925_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 15925_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39229_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 39229_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19197_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 19197_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19835_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 19835_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21805_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 21805_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24188_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 24188_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19606_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 19606_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19514_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 19514_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23536_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 23536_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23689_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 23689_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23854_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 23854_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19620_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 19620_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19760_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 19760_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39338_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 39338_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18266_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 18266_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16707_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 16707_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22800_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 22800_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21639_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 21639_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23953_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 23953_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19994_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 19994_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24122_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 24122_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20748_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 20748_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16691_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 16691_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22144_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 22144_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18718_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 18718_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20096_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 20096_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23683_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 23683_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19246_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 19246_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17933_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 17933_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23101_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 23101_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23341_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 23341_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24161_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 24161_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16451_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 16451_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35730_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 35730_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18620_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 18620_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22382_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
Preparing report for the candidate 22382_fd_Psc-02-Q2b1x1_2026-07-10_03-15-12_20.00sec_5.00C_LIGHT_0341
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 117s
Prepared the HTML report for the field Psc-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:37:32.92 +15:19:52.2
00:37:32.65 +15:12:16.0
00:37:12.64 +15:07:56.7
00:36:39.76 +15:08:20.4
00:55:28.78 +15:07:53.5
00:56:29.29 +14:50:04.7
00:56:27.53 +14:45:45.4
00:57:33.73 +14:43:29.7
00:35:43.44 +14:41:35.3
00:34:59.71 +14:40:09.9
00:56:24.36 +14:40:07.6
00:35:50.50 +14:38:19.0
00:49:01.91 +14:37:14.4
00:56:49.65 +14:31:13.5
00:35:23.86 +14:30:47.5
00:37:09.68 +14:31:12.6
00:36:59.45 +14:27:00.3
00:55:55.61 +14:25:36.4
00:36:58.85 +14:25:09.2
00:54:46.10 +14:23:31.6
00:37:33.03 +14:21:24.7
00:38:02.16 +14:19:43.0
00:38:15.29 +14:18:13.3
00:35:28.95 +14:07:19.1
00:38:07.41 +14:03:09.1
00:37:47.87 +13:55:11.1
00:50:04.13 +13:53:09.0
01:01:18.28 +13:48:00.6
00:50:18.01 +13:47:52.7
00:36:21.65 +13:43:02.0
00:36:08.16 +13:40:43.3
00:37:25.04 +13:37:23.0
00:52:13.28 +13:32:57.0
00:52:37.36 +13:29:32.5
01:08:30.18 +13:22:39.0
01:08:35.41 +13:20:33.6
00:52:23.70 +13:22:56.6
00:52:26.46 +13:20:22.7
00:51:48.29 +13:19:26.9
01:08:12.65 +13:16:38.7
01:08:14.04 +13:13:02.1
01:08:41.22 +13:12:24.3
00:52:24.52 +13:15:10.7
00:52:36.32 +12:59:09.9
00:56:31.74 +11:35:41.5
00:56:43.00 +12:12:36.1
00:56:17.94 +12:29:38.8
00:55:51.73 +12:29:41.6
00:56:29.14 +12:36:09.8
########### Completed Psc-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:01:18.28 +13:48:00.6
00:34:59.71 +14:40:09.9
00:56:43.00 +12:12:36.1
00:37:09.68 +14:31:12.6
00:49:01.91 +14:37:14.4
00:57:33.73 +14:43:29.7
00:55:28.78 +15:07:53.5
00:56:29.14 +12:36:09.8
00:51:48.29 +13:19:26.9
00:38:07.41 +14:03:09.1
00:35:43.44 +14:41:35.3
00:36:08.16 +13:40:43.3
00:52:36.32 +12:59:09.9
00:37:32.92 +15:19:52.2
00:56:17.94 +12:29:38.8
00:56:49.65 +14:31:13.5
00:37:33.03 +14:21:24.7
00:50:04.13 +13:53:09.0
00:52:24.52 +13:15:10.7
00:55:55.61 +14:25:36.4
00:36:59.45 +14:27:00.3
01:08:30.18 +13:22:39.0
00:52:23.70 +13:22:56.6
00:52:26.46 +13:20:22.7
00:36:58.85 +14:25:09.2
00:54:46.10 +14:23:31.6
00:55:51.73 +12:29:41.6
00:56:27.53 +14:45:45.4
00:36:39.76 +15:08:20.4
00:37:25.04 +13:37:23.0
00:37:47.87 +13:55:11.1
01:08:12.65 +13:16:38.7
00:38:02.16 +14:19:43.0
01:08:14.04 +13:13:02.1
00:35:28.95 +14:07:19.1
00:37:12.64 +15:07:56.7
00:50:18.01 +13:47:52.7
00:35:50.50 +14:38:19.0
00:38:15.29 +14:18:13.3
01:08:35.41 +13:20:33.6
00:35:23.86 +14:30:47.5
00:56:29.29 +14:50:04.7
00:52:13.28 +13:32:57.0
00:52:37.36 +13:29:32.5
01:08:41.22 +13:12:24.3
00:37:32.65 +15:12:16.0
00:56:31.74 +11:35:41.5
00:56:24.36 +14:40:07.6
00:36:21.65 +13:43:02.0
###################################################################################
01:01:18.28 +13:48:00.6 -- not an asteroid (will add it to exclusion list)
00:34:59.71 +14:40:09.9 -- not an asteroid (will add it to exclusion list)
00:56:43.00 +12:12:36.1 -- not an asteroid (will add it to exclusion list)
00:37:09.68 +14:31:12.6 -- not an asteroid (will add it to exclusion list)
00:49:01.91 +14:37:14.4 -- not an asteroid (will add it to exclusion list)
00:57:33.73 +14:43:29.7 -- not an asteroid (will add it to exclusion list)
00:55:28.78 +15:07:53.5 -- not an asteroid (will add it to exclusion list)
00:56:29.14 +12:36:09.8 -- not an asteroid (will add it to exclusion list)
00:51:48.29 +13:19:26.9 -- not an asteroid (will add it to exclusion list)
00:38:07.41 +14:03:09.1 -- not an asteroid (will add it to exclusion list)
00:35:43.44 +14:41:35.3 -- not an asteroid (will add it to exclusion list)
00:36:08.16 +13:40:43.3 -- not an asteroid (will add it to exclusion list)
00:52:36.32 +12:59:09.9 -- not an asteroid (will add it to exclusion list)
00:37:32.92 +15:19:52.2 -- not an asteroid (will add it to exclusion list)
00:56:17.94 +12:29:38.8 -- not an asteroid (will add it to exclusion list)
00:56:49.65 +14:31:13.5 -- not an asteroid (will add it to exclusion list)
00:37:33.03 +14:21:24.7 -- not an asteroid (will add it to exclusion list)
00:50:04.13 +13:53:09.0 -- not an asteroid (will add it to exclusion list)
00:52:24.52 +13:15:10.7 -- not an asteroid (will add it to exclusion list)
00:55:55.61 +14:25:36.4 -- not an asteroid (will add it to exclusion list)
00:36:59.45 +14:27:00.3 -- not an asteroid (will add it to exclusion list)
01:08:30.18 +13:22:39.0 -- not an asteroid (will add it to exclusion list)
00:52:23.70 +13:22:56.6 -- not an asteroid (will add it to exclusion list)
00:52:26.46 +13:20:22.7 -- not an asteroid (will add it to exclusion list)
00:36:58.85 +14:25:09.2 -- not an asteroid (will add it to exclusion list)
00:54:46.10 +14:23:31.6 -- not an asteroid (will add it to exclusion list)
00:55:51.73 +12:29:41.6 -- not an asteroid (will add it to exclusion list)
00:56:27.53 +14:45:45.4 -- not an asteroid (will add it to exclusion list)
00:36:39.76 +15:08:20.4 -- not an asteroid (will add it to exclusion list)
00:37:25.04 +13:37:23.0 -- not an asteroid (will add it to exclusion list)
00:37:47.87 +13:55:11.1 -- not an asteroid (will add it to exclusion list)
01:08:12.65 +13:16:38.7 -- not an asteroid (will add it to exclusion list)
00:38:02.16 +14:19:43.0 -- not an asteroid (will add it to exclusion list)
01:08:14.04 +13:13:02.1 -- not an asteroid (will add it to exclusion list)
00:35:28.95 +14:07:19.1 -- not an asteroid (will add it to exclusion list)
00:37:12.64 +15:07:56.7 -- not an asteroid (will add it to exclusion list)
00:50:18.01 +13:47:52.7 -- not an asteroid (will add it to exclusion list)
00:35:50.50 +14:38:19.0 -- not an asteroid (will add it to exclusion list)
00:38:15.29 +14:18:13.3 -- not an asteroid (will add it to exclusion list)
01:08:35.41 +13:20:33.6 -- not an asteroid (will add it to exclusion list)
00:35:23.86 +14:30:47.5 -- not an asteroid (will add it to exclusion list)
00:56:29.29 +14:50:04.7 -- not an asteroid (will add it to exclusion list)
00:52:13.28 +13:32:57.0 -- not an asteroid (will add it to exclusion list)
00:52:37.36 +13:29:32.5 -- not an asteroid (will add it to exclusion list)
01:08:41.22 +13:12:24.3 -- not an asteroid (will add it to exclusion list)
00:37:32.65 +15:12:16.0 -- not an asteroid (will add it to exclusion list)
00:56:31.74 +11:35:41.5 -- not an asteroid (will add it to exclusion list)
00:56:24.36 +14:40:07.6 -- not an asteroid (will add it to exclusion list)
00:36:21.65 +13:43:02.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:34:59.71 +14:40:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:23.86 +14:30:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:28.95 +14:07:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:43.44 +14:41:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:50.50 +14:38:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:08.16 +13:40:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:21.65 +13:43:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:39.76 +15:08:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:58.85 +14:25:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:59.45 +14:27:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:09.68 +14:31:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:12.64 +15:07:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:25.04 +13:37:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:32.65 +15:12:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:32.92 +15:19:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:33.03 +14:21:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:47.87 +13:55:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:02.16 +14:19:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:07.41 +14:03:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:15.29 +14:18:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:01.91 +14:37:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:04.13 +13:53:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:18.01 +13:47:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:48.29 +13:19:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:13.28 +13:32:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:23.70 +13:22:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:24.52 +13:15:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:26.46 +13:20:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:36.32 +12:59:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:37.36 +13:29:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:46.10 +14:23:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:28.78 +15:07:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:51.73 +12:29:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:55.61 +14:25:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:17.94 +12:29:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:24.36 +14:40:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:27.53 +14:45:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:29.14 +12:36:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:29.29 +14:50:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:31.74 +11:35:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:43.00 +12:12:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:49.65 +14:31:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:57:33.73 +14:43:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:18.28 +13:48:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:12.65 +13:16:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:14.04 +13:13:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:30.18 +13:22:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:35.41 +13:20:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:41.22 +13:12:24.3 -- 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)
00:34:59.71 +14:40:09.9 -- not a known variable star
00:35:23.86 +14:30:47.5 -- not a known variable star
00:35:28.95 +14:07:19.1 -- not a known variable star
00:35:43.44 +14:41:35.3 -- not a known variable star
00:35:50.50 +14:38:19.0 -- not a known variable star
00:36:08.16 +13:40:43.3 -- not a known variable star
00:36:21.65 +13:43:02.0 -- a known variable star
00:36:39.76 +15:08:20.4 -- not a known variable star
00:36:58.85 +14:25:09.2 -- not a known variable star
00:36:59.45 +14:27:00.3 -- not a known variable star
00:37:09.68 +14:31:12.6 -- not a known variable star
00:37:12.64 +15:07:56.7 -- not a known variable star
00:37:25.04 +13:37:23.0 -- not a known variable star
00:37:32.65 +15:12:16.0 -- not a known variable star
00:37:32.92 +15:19:52.2 -- not a known variable star
00:37:33.03 +14:21:24.7 -- not a known variable star
00:37:47.87 +13:55:11.1 -- not a known variable star
00:38:02.16 +14:19:43.0 -- not a known variable star
00:38:07.41 +14:03:09.1 -- not a known variable star
00:38:15.29 +14:18:13.3 -- a known variable star
00:49:01.91 +14:37:14.4 -- a known variable star
00:50:04.13 +13:53:09.0 -- not a known variable star
00:50:18.01 +13:47:52.7 -- not a known variable star
00:51:48.29 +13:19:26.9 -- a known variable star
00:52:13.28 +13:32:57.0 -- not a known variable star
00:52:23.70 +13:22:56.6 -- not a known variable star
00:52:24.52 +13:15:10.7 -- not a known variable star
00:52:26.46 +13:20:22.7 -- not a known variable star
00:52:36.32 +12:59:09.9 -- not a known variable star
00:52:37.36 +13:29:32.5 -- not a known variable star
00:54:46.10 +14:23:31.6 -- not a known variable star
00:55:28.78 +15:07:53.5 -- not a known variable star
00:55:51.73 +12:29:41.6 -- not a known variable star
00:55:55.61 +14:25:36.4 -- not a known variable star
00:56:17.94 +12:29:38.8 -- not a known variable star
00:56:24.36 +14:40:07.6 -- a known variable star
00:56:27.53 +14:45:45.4 -- not a known variable star
00:56:29.14 +12:36:09.8 -- not a known variable star
00:56:29.29 +14:50:04.7 -- not a known variable star
00:56:31.74 +11:35:41.5 -- not a known variable star
00:56:43.00 +12:12:36.1 -- not a known variable star
00:56:49.65 +14:31:13.5 -- not a known variable star
00:57:33.73 +14:43:29.7 -- not a known variable star
01:01:18.28 +13:48:00.6 -- not a known variable star
01:08:12.65 +13:16:38.7 -- not a known variable star
01:08:14.04 +13:13:02.1 -- not a known variable star
01:08:30.18 +13:22:39.0 -- not a known variable star
01:08:35.41 +13:20:33.6 -- not a known variable star
01:08:41.22 +13:12:24.3 -- not a known variable star
Found 44 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
49 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 49 (excluding asteroids and hot pixels, 44 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)2461231.84346693 -observatory V36
07:32:17.84 +17:08:02.3 Mercury (5.1mag)
10:11:36.96 +12:41:11.0 Venus (-4.1mag)
04:24:09.05 +21:25:09.0 Mars (1.3mag)
08:16:40.17 +20:11:30.2 Jupiter (-1.8mag)
00:55:50.86 +03:20:28.7 Saturn (0.7mag)
04:07:13.95 +20:45:03.2 Uranus (5.8mag)
00:17:01.50 +00:20:41.2 Neptune (7.8mag)
20:30:54.98 -23:18:00.4 Pluto (14.4mag)
03:11:18.20 +22:18:16.9 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 361 Jul 10 06:26 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461231.84346693:
08:16:46.80 +20:11:07.2 Io (6.1mag)
08:16:42.90 +20:11:21.8 Europa (6.3mag)
08:16:57.23 +20:10:28.6 Ganymede (5.6mag)
08:17:08.17 +20:09:46.8 Callisto (6.8mag)
08:15:11.68 +19:55:39.6 Himalia (15.7mag)
08:16:39.25 +20:11:34.6 Thebe (16.6mag)
08:14:33.02 +20:00:09.3 Elara (17.6mag)
08:20:12.38 +20:05:40.6 Pasiphae (17.8mag)
08:21:38.05 +20:16:35.2 Carme (19.0mag)
00:55:40.71 +03:20:19.6 Titan (8.5mag)
00:55:45.62 +03:20:31.8 Rhea (9.8mag)
00:55:20.16 +03:19:37.6 Iapetus (11.2mag)
00:56:00.12 +03:20:47.7 Hyperion (14.5mag)
00:55:51.60 +03:17:42.5 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 06:26 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.84346693:
17:46:08.36 -32:59:32.0 JWST
16:13:48.93 +48:50:50.7 Chandra
02:51:46.64 +61:52:17.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 06:26 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.84346693 -observatory V36
02:36:15.48 +14:25:38.3 17.9mag P/1996 R2 (Lagerkvist)
18:17:56.75 -34:21:44.6 13.7mag P/2010 H2 (Vales)
06:25:39.99 -68:08:22.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:48.20 +32:26:48.6 17.6mag C/2017 K2 (PANSTARRS)
17:03:07.10 +16:02:54.6 18.0mag C/2021 G2 (ATLAS)
01:47:45.56 +08:12:16.4 15.4mag P/2021 N1 (ZTF)
22:59:32.17 +32:17:08.1 17.3mag C/2022 E2 (ATLAS)
06:12:23.41 +26:55:34.9 16.7mag C/2022 N2 (PANSTARRS)
09:55:30.48 +29:46:52.5 16.8mag C/2022 QE78 (ATLAS)
09:09:43.79 +04:59:56.6 17.8mag C/2022 R6 (PANSTARRS)
18:07:13.38 +21:17:39.0 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:35.28 -11:23:15.3 17.7mag P/2023 B1 (PANSTARRS)
21:49:14.68 +67:37:16.9 17.8mag C/2023 H5 (Lemmon)
16:30:54.11 -10:04:38.5 13.9mag C/2023 R1 (PANSTARRS)
08:00:38.17 +65:42:28.7 17.9mag C/2024 A1 (ATLAS)
07:32:48.22 +30:00:10.5 14.6mag C/2024 E1 (Wierzchos)
15:16:19.81 +15:19:41.3 17.5mag C/2024 G6 (ATLAS)
19:41:19.22 +39:23:29.1 13.8mag C/2024 J3 (ATLAS)
21:47:35.48 +46:00:07.2 17.8mag C/2024 R4 (PANSTARRS)
04:49:37.88 -13:47:46.6 15.7mag C/2024 T5 (ATLAS)
06:34:33.97 +29:04:16.5 18.0mag C/2025 J1 (Borisov)
07:14:20.00 -12:53:20.1 16.5mag C/2025 R3 (PANSTARRS)
09:56:04.92 +22:26:14.0 17.6mag C/2025 V2 (Rankin)
12:44:36.85 +03:56:17.4 17.1mag C/2025 Y1 (ATLAS)
16:51:58.65 +79:07:12.5 17.4mag C/2026 A2 (Bok)
02:46:16.01 +45:14:22.1 16.7mag C/2026 B2 (Sun-Gao)
11:25:30.35 +04:32:33.4 16.9mag A/2026 E1
21:19:01.43 -15:04:24.3 7.3mag 10P/Tempel
11:13:27.06 -01:53:12.6 16.1mag 29P/Schwassmann-Wachmann
04:00:09.59 +29:33:08.0 17.8mag 47P/Ashbrook-Jackson
10:08:03.50 +14:00:51.1 17.0mag 63P/Wild
00:48:21.52 -05:05:35.7 15.5mag 65P/Gunn
08:26:55.55 +34:13:09.3 17.9mag 76P/West-Kohoutek-Ikemura
04:27:22.62 +20:10:41.9 13.7mag 78P/Gehrels
02:22:19.20 +10:36:29.9 16.2mag 88P/Howell
06:35:30.26 +30:32:07.0 15.7mag 93P/Lovas
04:20:58.25 +31:07:21.4 16.9mag 114P/Wiseman-Skiff
08:08:40.37 +30:42:16.1 15.3mag 123P/West-Hartley
10:48:06.89 +01:11:25.8 16.8mag 124P/Mrkos
04:51:42.84 +20:48:45.8 16.2mag 128P/Shoemaker-Holt
05:36:14.33 +19:42:50.8 17.8mag 131P/Mueller
00:01:32.58 +02:56:05.6 17.9mag 139P/Vaisala-Oterma
07:13:31.75 +17:01:21.4 15.5mag 141P-D/Machholz
03:16:50.72 -21:06:23.9 15.5mag 161P/Hartley-IRAS
05:33:01.90 +33:56:48.1 15.3mag 162P/SidingSpring
19:04:29.73 +15:04:37.9 14.7mag 169P/NEAT
01:41:00.55 +07:35:51.5 17.7mag 220P/McNaught
16:35:58.21 -08:23:06.1 17.0mag 235P/LINEAR
08:45:16.01 +33:18:00.9 17.9mag 240P/NEAT
20:42:10.73 -49:34:07.2 17.8mag 259P/Garradd
01:59:16.90 +12:05:26.3 15.7mag 260P/McNaught
05:37:11.96 +36:50:31.9 17.4mag 295P/LINEAR
15:06:36.82 +06:03:27.7 17.6mag 391P/Kowalski
08:34:35.74 +19:40:37.7 17.9mag 450P/LONEOS
07:51:45.15 +39:13:00.9 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 06:26 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 06:26 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 06:26 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:03:23.326 +12:49:15.53 AT 2026sqk 2026-07-06.95 17.816
02:23:45.306 -56:30:54.13 AT 2026sqj 2026-07-07.14 18.706
20:05:32.749 -40:04:20.18 AT 2026sqi 2026-07-07.00 19.025
13:27:09.068 +62:50:19.22 AT 2026sqh 2026-07-06.32 19.347
10:36:21.258 +13:42:31.91 AT 2026sqg 2026-07-06.96 17.376
10:38:47.961 +53:30:34.10 SN 2026sqf 2026-07-08.25 12.9
13:40:20.447 +40:38:15.61 AT 2026sqe 2026-07-03.20 20.3209
20:26:11.475 -21:05:59.62 AT 2026sqd 2026-07-07.33 20.2909
20:38:05.960 -15:39:19.94 AT 2026sqc 2026-07-07.33 22.2834
21:50:20.218 -14:25:11.02 AT 2026sqb 2026-07-07.39 21.5547
20:32:17.644 -16:37:51.49 AT 2026sqa 2026-07-07.33 21.6569
20:38:02.144 -16:39:15.94 AT 2026spz 2026-07-07.33 22.7762
20:36:24.191 -15:13:43.37 AT 2026spy 2026-07-07.33 22.1739
20:41:10.988 -25:49:45.49 AT 2026spx 2026-07-07.33 22.8645
21:17:15.336 -23:31:53.39 AT 2026spw 2026-07-07.32 21.9459
20:27:45.431 -19:59:58.81 AT 2026spv 2026-07-07.33 21.6485
21:55:34.604 -14:11:57.66 AT 2026spu 2026-07-07.39 23.0585
21:10:34.181 -22:59:24.76 AT 2026spt 2026-07-07.32 22.3526
21:05:55.405 -19:04:02.26 AT 2026sps 2026-07-07.32 21.4424
20:59:14.423 -27:33:25.12 AT 2026spr 2026-07-07.32 23.4151
-rw-r--r-- 1 apache apache 30K Jul 10 06:26 tns_transients_list.txt
