This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS
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 10.3629 2461231.8629 9.62 01:59:12.87 +03:31:10.8
153.62730 -55.26075 galactic Psc Second-epoch detections are separated by 0.3" and 6.9 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 2517883830925784704 | 01:59:12.66 +03:31:09.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0.5V 1995AJ....110.1838R GJ 1041 A
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:12.87 +03:31:10.8: 10.67 +/- 0.00 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:12.87 +03:31:10.8: 10.65 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.66 +/- 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 2517883830925784704,2461231.8629,9.62,0.05,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 2517883830925784704 20260710.3629 9.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.66 01:56:13.18 +03:03:36.2
152.81055 -56.00736 galactic Psc Second-epoch detections are separated by 1.9" and 7.0 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 2511837268591778432 | 01:56:13.21 +03:03:35.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5) J-Ks=0.296+/-0.033 (F)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:56:13.18 +03:03:36.2: 12.53 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:56:13.18 +03:03:36.2: 12.60 +/- 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
Gaia DR3 2511837268591778432,2461231.8629,11.66,0.05,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 2511837268591778432 20260710.3629 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 10.3629 2461231.8629 11.54 01:25:26.88 +02:56:21.7
139.50957 -58.83340 galactic Psc Second-epoch detections are separated by 2.5" and 6.9 pix
The object was found in VSX 0" KS Psc
Type: RS
# Max. Min./Amp. JD0 Period
12.300 R1 12.500 R1 2451456.84000 2.490000000000
The object was not found in astcheck.
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:25:26.88 +02:56:21.7: 12.63 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:25:26.88 +02:56:21.7: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 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
KS Psc,2461231.8629,11.54,0.05,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
KS Psc 20260710.3629 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 10.3629 2461231.8629 11.28 01:29:50.51 +06:51:20.6
139.61281 -54.76744 galactic Psc Second-epoch detections are separated by 0.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2565348098629495680 | 01:29:50.49 +06:51:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=0.688+/-0.035 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:29:50.51 +06:51:20.6: 12.23 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:29:50.51 +06:51:20.6: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 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 2565348098629495680,2461231.8629,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2565348098629495680 20260710.3629 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.15 01:59:30.01 +03:44:01.4
153.56800 -55.03770 galactic Psc Second-epoch detections are separated by 1.2" and 7.0 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 2517895547596560256 | 01:59:29.99 +03:44:01.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5) J-Ks=0.346+/-0.032 (G)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:30.01 +03:44:01.4: 12.20 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:30.01 +03:44:01.4: 12.16 +/- 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 2517895547596560256,2461231.8629,11.15,0.05,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 2517895547596560256 20260710.3629 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.63 02:00:00.20 +03:21:37.7
154.06262 -55.31210 galactic Psc Second-epoch detections are separated by 1.8" and 7.0 pix
The object was found in VSX 2" Gaia DR3 2517819264682332416
Type: ROT
# Max. Min./Amp. JD0 Period
12.410 G 12.440 G K
The object was not found in astcheck.
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:00:00.20 +03:21:37.7: 12.61 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:00:00.20 +03:21:37.7: 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 2517819264682332416,2461231.8629,11.63,0.05,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 2517819264682332416 20260710.3629 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.79 01:54:51.58 +02:03:52.1
153.06342 -57.05001 galactic Cet Second-epoch detections are separated by 2.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:54:51.58 +02:03:52.1 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.355+/-0.035 (G)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:54:51.58 +02:03:52.1: 12.96 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:54:51.58 +02:03:52.1: 12.93 +/- 0.02 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!
TCP 2026 07 10.3629* 01 54 51.58 +02 03 52.1 11.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8629,11.79,0.05,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
target 20260710.3629 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 10.3629 2461231.8629 11.82 02:00:10.95 +03:14:49.5
154.22452 -55.39201 galactic Psc Second-epoch detections are separated by 2.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:00:10.95 +03:14:49.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.595+/-0.033 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:00:10.95 +03:14:49.5: 12.94 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:00:10.95 +03:14:49.5: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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,2461231.8629,11.82,0.05,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 20260710.3629 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 10.3629 2461231.8629 11.12 01:25:30.34 +06:45:26.7
137.83699 -55.12538 galactic Psc Second-epoch detections are separated by 0.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2565993645099000960 | 01:25:30.29 +06:45:26.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 1986AJ.....91..144S StKM 1- 151 J-Ks=0.695+/-0.028 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:25:30.34 +06:45:26.7: 12.04 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:25:30.34 +06:45:26.7: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 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 2565993645099000960,2461231.8629,11.12,0.05,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 2565993645099000960 20260710.3629 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.53 02:00:13.53 +04:08:23.9
153.52737 -54.59361 galactic Psc Second-epoch detections are separated by 2.1" and 7.2 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 2518683824418861568 | 02:00:13.50 +04:08:25.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.262+/-0.037 (F)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:00:13.53 +04:08:23.9: 12.59 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:00:13.53 +04:08:23.9: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2518683824418861568,2461231.8629,11.53,0.05,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 2518683824418861568 20260710.3629 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 10.3629 2461231.8629 11.59 01:54:54.57 +02:13:11.3
152.95663 -56.90545 galactic Cet Second-epoch detections are separated by 1.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1903 Adzhimushkaj 37 -400 402 16.4 0 0
ATTENTION: measured mag 11.59 is 4.8 mag brighter than the predicted asteroid brightness 16.4 - the transient may be an unrelated new object!
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:54:54.57 +02:13:11.3: 12.58 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:54:54.57 +02:13:11.3: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 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!
TCP 2026 07 10.3629* 01 54 54.57 +02 13 11.3 11.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461231.8629,11.59,0.05,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
VARIABLE_NAME 20260710.3629 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.49 01:59:25.18 +02:05:20.8
154.88989 -56.50485 galactic Cet Second-epoch detections are separated by 1.9" and 7.1 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 2511437046359812224 | 01:59:25.15 +02:05:20.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.309+/-0.033 (F)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:25.18 +02:05:20.8: 12.55 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:25.18 +02:05:20.8: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 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!
TCP 2026 07 10.3629* 01 59 25.18 +02 05 20.8 11.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2511437046359812224,2461231.8629,11.49,0.05,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 2511437046359812224 20260710.3629 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.58 01:58:44.49 +03:36:55.3
153.36666 -55.22898 galactic Psc Second-epoch detections are separated by 2.5" and 7.2 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 2517888499555142144 | 01:58:44.48 +03:36:54.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.355+/-0.031 (G)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:44.49 +03:36:55.3: 12.55 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:44.49 +03:36:55.3: 12.58 +/- 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 2517888499555142144,2461231.8629,11.58,0.05,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 2517888499555142144 20260710.3629 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 10.3629 2461231.8629 11.48 01:26:03.13 +03:33:50.8
139.48481 -58.19084 galactic Psc Second-epoch detections are separated by 0.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2560098957103480448 | 01:26:03.14 +03:33:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.366+/-0.032 (G)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:26:03.13 +03:33:50.8: 12.49 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:26:03.13 +03:33:50.8: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 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 2560098957103480448,2461231.8629,11.48,0.05,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 2560098957103480448 20260710.3629 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.38 01:56:56.01 +02:43:28.1
153.36590 -56.22766 galactic Psc Second-epoch detections are separated by 1.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2511765942070452224 | 01:56:55.99 +02:43:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.287+/-0.035 (F)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:56:56.01 +02:43:28.1: 12.49 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:56:56.01 +02:43:28.1: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2511765942070452224,2461231.8629,11.38,0.05,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 2511765942070452224 20260710.3629 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 10.3629 2461231.8629 11.43 01:26:37.27 +06:57:17.8
138.22593 -54.86866 galactic Psc Second-epoch detections are separated by 1.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1572 Posnania 221 -504 550 15.3 -0 0
ATTENTION: measured mag 11.43 is 3.9 mag brighter than the predicted asteroid brightness 15.3 - the transient may be an unrelated new object!
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:26:37.27 +06:57:17.8: 12.47 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:26:37.27 +06:57:17.8: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 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
VARIABLE_NAME,2461231.8629,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3629 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.73 01:56:10.12 +02:35:31.7
153.16564 -56.43178 galactic Cet Second-epoch detections are separated by 2.1" and 6.8 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 | 01:56:10.12 +02:35:31.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.468+/-0.031 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:56:10.12 +02:35:31.7: 12.87 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:56:10.12 +02:35:31.7: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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!
TCP 2026 07 10.3629* 01 56 10.12 +02 35 31.7 11.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8629,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3629 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.38 01:59:09.56 +02:57:57.1
154.05350 -55.75940 galactic Psc Second-epoch detections are separated by 1.7" and 7.2 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 2511797243792123904 | 01:59:08.67 +02:57:19.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.781+/-0.044 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:09.56 +02:57:57.1: 12.43 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:09.56 +02:57:57.1: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 2511797243792123904,2461231.8629,11.38,0.05,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 2511797243792123904 20260710.3629 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 10.3629 2461231.8629 11.37 01:57:58.16 +03:00:41.5
153.54619 -55.85463 galactic Psc Second-epoch detections are separated by 0.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2511824383690354560 | 01:57:58.11 +03:00:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.635+/-0.031 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:57:58.16 +03:00:41.5: 12.42 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:57:58.16 +03:00:41.5: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 2511824383690354560,2461231.8629,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2511824383690354560 20260710.3629 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.80 01:59:18.06 +04:12:53.9
153.11373 -54.63074 galactic Psc Second-epoch detections are separated by 1.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:59:18.06 +04:12:53.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.465+/-0.041 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:18.06 +04:12:53.9: 12.85 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:18.06 +04:12:53.9: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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,2461231.8629,11.80,0.05,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
target 20260710.3629 11.80CV 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 10.3629 2461231.8629 11.38 01:24:55.60 +05:47:52.2
137.98229 -56.09222 galactic Psc Second-epoch detections are separated by 1.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1317 Silvretta 139 316 345 15.2 -0 -0
ATTENTION: measured mag 11.38 is 3.8 mag brighter than the predicted asteroid brightness 15.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:24:55.60 +05:47:52.2: 12.42 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:24:55.60 +05:47:52.2: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 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
VARIABLE_NAME,2461231.8629,11.38,0.05,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
VARIABLE_NAME 20260710.3629 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 10.3629 2461231.8629 11.79 01:58:19.56 +02:13:57.9
154.33054 -56.50568 galactic Cet Second-epoch detections are separated by 2.6" and 6.8 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 | 01:58:19.56 +02:13:57.9 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.316+/-0.034 (F)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:19.56 +02:13:57.9: 12.81 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:19.56 +02:13:57.9: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 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!
TCP 2026 07 10.3629* 01 58 19.56 +02 13 57.9 11.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8629,11.79,0.05,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
target 20260710.3629 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 10.3629 2461231.8629 11.39 01:55:14.83 +01:45:35.5
153.47557 -57.27852 galactic Cet Second-epoch detections are separated by 0.4" and 6.9 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 | Large-amplitude variable Gaia DR2 2511038099732098304 | 01:55:14.92 +01:45:35.5 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G3 (LAMOST DR5) J-Ks=0.354+/-0.033 (G)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:55:14.83 +01:45:35.5: 12.35 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:55:14.83 +01:45:35.5: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 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!
TCP 2026 07 10.3629* 01 55 14.83 +01 45 35.5 11.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2511038099732098304,2461231.8629,11.39,0.05,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
Large-amplitude variable Gaia DR2 2511038099732098304 20260710.3629 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 10.3629 2461231.8629 11.29 02:00:38.76 +04:22:02.6
153.51038 -54.34339 galactic Psc Second-epoch detections are separated by 2.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2518785086863406208 | 02:00:38.77 +04:22:03.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.560+/-0.034 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:00:38.76 +04:22:02.6: 12.35 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:00:38.76 +04:22:02.6: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 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 2518785086863406208,2461231.8629,11.29,0.05,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 2518785086863406208 20260710.3629 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.70 01:58:28.70 +03:02:19.4
153.72555 -55.77259 galactic Psc Second-epoch detections are separated by 0.6" and 6.9 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 | 01:58:28.70 +03:02:19.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.567+/-0.032 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:28.70 +03:02:19.4: 12.75 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:28.70 +03:02:19.4: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 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,2461231.8629,11.70,0.05,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 20260710.3629 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.70 01:58:31.75 +02:53:47.9
153.86130 -55.89315 galactic Psc Second-epoch detections are separated by 1.2" and 6.8 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 | 01:58:31.75 +02:53:47.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.400+/-0.035 (G)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:31.75 +02:53:47.9: 12.73 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:31.75 +02:53:47.9: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 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,2461231.8629,11.70,0.05,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 20260710.3629 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.60 01:56:49.35 +02:57:20.8
153.13479 -56.03354 galactic Psc Second-epoch detections are separated by 2.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:56:49.35 +02:57:20.8 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.352+/-0.035 (G)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:56:49.35 +02:57:20.8: 12.74 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:56:49.35 +02:57:20.8: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 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,2461231.8629,11.60,0.05,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 20260710.3629 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.65 01:57:52.60 +02:54:02.2
153.59929 -55.96395 galactic Psc Second-epoch detections are separated by 1.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2511776318711434752 | 01:57:52.67 +02:54:01.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.618+/-0.033 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:57:52.60 +02:54:02.2: 12.70 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:57:52.60 +02:54:02.2: 12.67 +/- 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 2511776318711434752,2461231.8629,11.65,0.05,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 2511776318711434752 20260710.3629 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 10.3629 2461231.8629 11.39 01:58:51.29 +03:30:12.8
153.49975 -55.31588 galactic Psc Second-epoch detections are separated by 0.1" and 6.9 pix
The object was found in VSX 0" Gaia DR3 2517882520960666880
Type: ROT
# Max. Min./Amp. JD0 Period
12.070 G 12.100 G K
The object was not found in astcheck.
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:51.29 +03:30:12.8: 12.32 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:51.29 +03:30:12.8: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 2517882520960666880,2461231.8629,11.39,0.05,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 2517882520960666880 20260710.3629 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 10.3629 2461231.8629 11.35 01:26:31.80 +05:35:11.8
138.76800 -56.20237 galactic Psc Second-epoch detections are separated by 0.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2565099501626965888 | 01:26:31.77 +05:35:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.809+/-0.031 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:26:31.80 +05:35:11.8: 12.33 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:26:31.80 +05:35:11.8: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 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 2565099501626965888,2461231.8629,11.35,0.05,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 2565099501626965888 20260710.3629 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 10.3629 2461231.8629 11.64 01:59:52.71 +03:25:43.8
153.95880 -55.26575 galactic Psc Second-epoch detections are separated by 2.7" and 7.3 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 | 01:59:52.71 +03:25:43.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.364+/-0.033 (G)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:52.71 +03:25:43.8: 12.70 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:52.71 +03:25:43.8: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 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,2461231.8629,11.64,0.05,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 20260710.3629 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.84 01:59:53.29 +04:13:51.9
153.32683 -54.55046 galactic Psc Second-epoch detections are separated by 0.8" and 6.8 pix
The object was found in VSX 2" Gaia DR3 2518688535998371584
Type: ROT
# Max. Min./Amp. JD0 Period
12.740 G 12.760 G K
The object was not found in astcheck.
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:53.29 +04:13:51.9: 12.99 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:53.29 +04:13:51.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 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 2518688535998371584,2461231.8629,11.84,0.05,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
Gaia DR3 2518688535998371584 20260710.3629 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 10.3629 2461231.8629 11.71 01:58:25.22 +02:02:04.8
154.53583 -56.67004 galactic Cet Second-epoch detections are separated by 1.4" and 7.1 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 2511438558188301184 | 01:58:25.24 +02:02:04.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.625+/-0.030 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:25.22 +02:02:04.8: 12.67 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:25.22 +02:02:04.8: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 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!
TCP 2026 07 10.3629* 01 58 25.22 +02 02 04.8 11.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2511438558188301184,2461231.8629,11.71,0.05,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
Gaia DR3 2511438558188301184 20260710.3629 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 10.3629 2461231.8629 11.71 01:59:47.45 +03:48:02.0
153.62756 -54.94520 galactic Psc Second-epoch detections are separated by 1.5" and 6.9 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 | 01:59:47.45 +03:48:02.0 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:47.45 +03:48:02.0: 12.96 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:47.45 +03:48:02.0: 13.02 +/- 0.02 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,2461231.8629,11.71,0.05,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 20260710.3629 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 10.3629 2461231.8629 11.30 01:25:33.85 +03:44:56.9
139.17353 -58.04242 galactic Psc Second-epoch detections are separated by 0.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2560117103340980992 | 01:25:33.82 +03:44:56.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.767+/-0.035 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:25:33.85 +03:44:56.9: 12.25 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:25:33.85 +03:44:56.9: 12.28 +/- 0.01 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 2560117103340980992,2461231.8629,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2560117103340980992 20260710.3629 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3629 2461231.8629 11.65 01:59:45.78 +02:00:15.7
155.09955 -56.53898 galactic Cet Second-epoch detections are separated by 2.3" and 6.8 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 2511388603423763456 | 01:59:45.72 +02:00:14.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.625+/-0.033 (K)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:45.78 +02:00:15.7: 12.65 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:45.78 +02:00:15.7: 12.64 +/- 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!
TCP 2026 07 10.3629* 01 59 45.78 +02 00 15.7 11.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2511388603423763456,2461231.8629,11.65,0.05,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 2511388603423763456 20260710.3629 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.63853609 09.01.2026 03:19:19.518 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
First image: 2461049.63853609 09.01.2026 03:19:19.518 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Last image: 2461231.86328623 10.07.2026 08:42:57.930 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4926
Objects passed selection criteria: 4896
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: 2755
Average stars matched: 2643.5 (95.9528 %)
Memory usage VmPeak: 111612 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 06:37:59 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: 2461049.63853609 09.01.2026 03:19:19.518 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
First image: 2461049.63853609 09.01.2026 03:19:19.518 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Last image: 2461231.86328623 10.07.2026 08:42:57.930 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 51
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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: 12 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): 27193
Objects passed selection criteria: 27078
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: 15719.2
Average stars matched: 14914 (94.8773 %)
Memory usage VmPeak: 132100 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 06:40:01 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
SExtractor catalog cache: saved Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat to cache
SExtractor catalog cache: saved Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.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: 2461231.86250455
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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits exists and is non-empty
Saving wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits to local_wcs_cache/
'wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits' -> 'local_wcs_cache/wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits'
wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits exists and is non-empty
Saving wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits to local_wcs_cache/
'wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits' -> 'local_wcs_cache/wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits'
wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits exists and is non-empty
Saving wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits to local_wcs_cache/
'wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits' -> 'local_wcs_cache/wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits'
wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits exists and is non-empty
Saving wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits to local_wcs_cache/
'wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits' -> 'local_wcs_cache/wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits (1st reference image)
verification OK: wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Image size: 941.4'x627.0' 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: 01:42:52.021 +05:59:59.08 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-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits (1st new image)
verification OK: wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
Image size: 938.7'x624.3' 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: 01:42:40.205 +05:59:18.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:52.021 +05:59:59.08
Second-epoch image center 01:42:40.205 +05:59:18.70
Angular distance between the image centers 0.0502 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits (2nd new image)
verification OK: wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
Image size: 938.6'x624.3' 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: 01:42:38.255 +05:58:52.80 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:52.021 +05:59:59.08
Second-epoch image center 01:42:38.255 +05:58:52.80
Angular distance between the image centers 0.0599 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 01:42:40.205 +05:59:18.70
Second-epoch second image center 01:42:38.255 +05:58:52.80
Angular distance between the image centers 0.01082 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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits &> /tmp/tmp.21hKs4QKZ6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits &> /tmp/tmp.1LEjC1GcVJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits &> /tmp/tmp.2j3gvaxCpv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits &> /tmp/tmp.SIxmSRoCa4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits and wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits and wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
Found non-empty wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits and wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
The reference image (wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits) and catalog (wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat) found
'wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat' -> 'wcsmag.cat'
Read 6596 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7260 to 33.6942 deg, Dec +0.7094 to +11.2856 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 17.7260 to 33.6942 deg, Dec 0.7094 to 11.2856 deg
Loaded 4459 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): 3597 out of 3790 total matches.
Matched with Tycho-2 3790 out of 6596 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.907900
a=0.000000 b=1.000000 c=22.907900
From vast_summary.log: estimated ref. image limiting mag.: -7.62
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 6596 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7260 to 33.6942 deg, Dec +0.7094 to +11.2856 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 17.7260 to 33.6942 deg, Dec 0.7094 to 11.2856 deg
Loaded 4459 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): 3597 out of 3790 total matches.
Matched with Tycho-2 3790 out of 6596 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits:
Forced-photometry filter: calibrated wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits -> calib.txt_param_ref_wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits (aperture=5.9)
Read 6518 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7262 to 33.6942 deg, Dec +0.6961 to +11.2761 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 17.7262 to 33.6942 deg, Dec 0.6961 to 11.2761 deg
Loaded 4458 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): 3575 out of 3779 total matches.
Matched with Tycho-2 3779 out of 6518 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits:
Forced-photometry filter: calibrated wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits -> calib.txt_param_ref_wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
2.0 pix Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
2.7 pix fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
2.7 pix fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
2.0 pix wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
2.0 pix wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Limiting magnitude estimates:
15.3 mag. Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
15.3 mag. Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
11.4 mag. fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
11.6 mag. fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
All-image limiting magnitude estimate: 11.4 (SNR ) 9.6 (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.21hKs4QKZ6 (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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits' -> 'wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS_IMAGE_NAME=wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS-calibrated image found: wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Checking if the catalog wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat corresponding to the image wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat corresponding to the image wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS catalog name: wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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=487, bad_region=1477, passed=6596
Got 6596 stars (including 4742 good ones) from the SExtractor catalog wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
util/solve_plate_with_UCAC5 got 6596 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 453 to 508 (Dec 0.7 to 11.3)
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(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5196 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 453 to 508 (Dec 0.7 to 11.3)
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(), 5196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits N_match=961 sigma_overall_arcsec=0.287 sigma_q1_arcsec=0.374 sigma_q2_arcsec=0.270 sigma_q3_arcsec=0.259 sigma_q4_arcsec=0.242 n_q1=295 n_q2=175 n_q3=310 n_q4=181 worst_quadrant_to_overall_ratio=1.301
The image catalog is written to wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits -region wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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.1LEjC1GcVJ (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-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits' -> 'wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS_IMAGE_NAME=wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS-calibrated image found: wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Checking if the catalog wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat corresponding to the image wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat corresponding to the image wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS catalog name: wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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=500, bad_region=1471, passed=6518
Got 6518 stars (including 4655 good ones) from the SExtractor catalog wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat
util/solve_plate_with_UCAC5 got 6518 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 453 to 508 (Dec 0.7 to 11.3)
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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5125 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 453 to 508 (Dec 0.7 to 11.3)
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(), 5125 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5125 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits N_match=961 sigma_overall_arcsec=0.306 sigma_q1_arcsec=0.375 sigma_q2_arcsec=0.295 sigma_q3_arcsec=0.281 sigma_q4_arcsec=0.258 n_q1=287 n_q2=183 n_q3=312 n_q4=179 worst_quadrant_to_overall_ratio=1.224
The image catalog is written to wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits -region wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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.2j3gvaxCpv (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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
Checking if the catalog wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
WCS catalog name: wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.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=38, bad_region=235, passed=719
Got 719 stars (including 457 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat
util/solve_plate_with_UCAC5 got 719 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 453 to 508 (Dec 0.6 to 11.2)
Done reading UCAC5 zone files...
Matched 430 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 430 matched stars entering correct_measured_positions(), 379 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 430 matched stars entering correct_measured_positions(), 435 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 453 to 508 (Dec 0.6 to 11.2)
Done reading UCAC5 zone files...
Matched 430 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 430 matched stars entering correct_measured_positions(), 436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 430 matched stars entering correct_measured_positions(), 436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 430 stars left (next iteration limit 473)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits N_match=430 sigma_overall_arcsec=0.514 sigma_q1_arcsec=0.472 sigma_q2_arcsec=0.487 sigma_q3_arcsec=0.505 sigma_q4_arcsec=0.617 n_q1=154 n_q2=107 n_q3=137 n_q4=32 worst_quadrant_to_overall_ratio=1.201
The image catalog is written to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits -region wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.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.SIxmSRoCa4 (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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
Checking if the catalog wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
WCS catalog name: wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.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=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=46, bad_region=211, passed=646
Got 646 stars (including 399 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits.wcscat
util/solve_plate_with_UCAC5 got 646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (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 0.010429 (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 453 to 508 (Dec 0.6 to 11.2)
Done reading UCAC5 zone files...
Matched 376 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 376 matched stars entering correct_measured_positions(), 329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 376 matched stars entering correct_measured_positions(), 394 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 453 to 508 (Dec 0.6 to 11.2)
Done reading UCAC5 zone files...
Matched 376 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 376 matched stars entering correct_measured_positions(), 391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 376 matched stars entering correct_measured_positions(), 391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 376 stars left (next iteration limit 413)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits N_match=376 sigma_overall_arcsec=0.479 sigma_q1_arcsec=0.500 sigma_q2_arcsec=0.566 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.577 n_q1=125 n_q2=86 n_q3=134 n_q4=31 worst_quadrant_to_overall_ratio=1.204
The image catalog is written to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits -region wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits sigma_overall=0.287 worst_q_ratio=1.301
ref2=Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits sigma_overall=0.306 worst_q_ratio=1.224
new1=fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits sigma_overall=0.514 worst_q_ratio=1.201
new2=fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits sigma_overall=0.479 worst_q_ratio=1.204
reference average sigma_overall=0.2965 worst_q_ratio=1.2625
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_astrometric_residuals.png (961 matched stars from wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_astrometric_residuals.png (961 matched stars from wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362_astrometric_residuals.png (430 matched stars from wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363_astrometric_residuals.png (376 matched stars from wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.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-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits'
Saving fully-calibrated image wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits'
Preparing the HTML report for the field Psc-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:12.87 +03:31:10.8: 10.67 +/- 0.00 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:12.87 +03:31:10.8: 10.65 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.66 +/- 0.00
Forced photometry filter KEPT candidate at 01:59:12.87 +03:31:10.8: ref_mag=10.66 +/- 0.00 new_mean_mag=9.6229 delta=1.04 (need > 0.90)
Adding exclusion_list_local.txt__out04840.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 04840_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 04840_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 18s
Prepared the HTML report for the field Psc-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:59:12.87 +03:31:10.8
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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
SExtractor catalog cache: saved Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat to cache
SExtractor catalog cache: saved Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Creating symlink local_wcs_cache/wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits exists and is non-empty
wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits exists and is non-empty
wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits exists and is non-empty
wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits (1st reference image)
verification OK: wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Image size: 941.4'x627.0' 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: 01:42:52.021 +05:59:59.08 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-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits (1st new image)
verification OK: wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
Image size: 938.7'x624.3' 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: 01:42:40.205 +05:59:18.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:52.021 +05:59:59.08
Second-epoch image center 01:42:40.205 +05:59:18.70
Angular distance between the image centers 0.0502 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits (2nd new image)
verification OK: wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
Image size: 938.6'x624.3' 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: 01:42:38.255 +05:58:52.80 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:52.021 +05:59:59.08
Second-epoch image center 01:42:38.255 +05:58:52.80
Angular distance between the image centers 0.0599 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 01:42:40.205 +05:59:18.70
Second-epoch second image center 01:42:38.255 +05:58:52.80
Angular distance between the image centers 0.01082 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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits &> /tmp/tmp.We14Ev50Zg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits &> /tmp/tmp.YS614r5c0A
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits &> /tmp/tmp.CdbJaXyNv0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits &> /tmp/tmp.uO7eFzxBPI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits and wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits and wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
Found non-empty wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits and wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
The reference image (wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits) and catalog (wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat) found
'wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat' -> 'wcsmag.cat'
Read 34861 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7260 to 33.6942 deg, Dec +0.7059 to +11.2869 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 17.7260 to 33.6942 deg, Dec 0.7059 to 11.2869 deg
Loaded 4462 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): 3480 out of 3876 total matches.
Matched with Tycho-2 3876 out of 34861 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.802450
a=0.000000 b=1.000000 c=22.802450
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 34861 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7260 to 33.6942 deg, Dec +0.7059 to +11.2869 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 17.7260 to 33.6942 deg, Dec 0.7059 to 11.2869 deg
Loaded 4462 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): 3480 out of 3876 total matches.
Matched with Tycho-2 3876 out of 34861 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits:
Forced-photometry filter: calibrated wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits -> calib.txt_param_ref_wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits (aperture=4.7)
Read 35044 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7262 to 33.7121 deg, Dec +0.6960 to +11.2774 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 17.7262 to 33.7121 deg, Dec 0.6960 to 11.2774 deg
Loaded 4462 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): 3477 out of 3877 total matches.
Matched with Tycho-2 3877 out of 35044 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits:
Forced-photometry filter: calibrated wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits -> calib.txt_param_ref_wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 36 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
1.9 pix Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
2.5 pix fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
2.3 pix fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
1.9 pix wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
1.9 pix wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Limiting magnitude estimates:
15.5 mag. Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
15.5 mag. Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
11.8 mag. fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
12.0 mag. fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
All-image limiting magnitude estimate: 11.8 (SNR ) 11.7 (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.We14Ev50Zg (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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits' -> 'wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS_IMAGE_NAME=wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS-calibrated image found: wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Checking if the catalog wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat corresponding to the image wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat corresponding to the image wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS catalog name: wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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=9, blended=1454, bad_region=6606, passed=34852
Got 34852 stars (including 27089 good ones) from the SExtractor catalog wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
util/solve_plate_with_UCAC5 got 34852 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 453 to 508 (Dec 0.7 to 11.3)
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(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 28684 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
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(), 28684 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 28683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits N_match=960 sigma_overall_arcsec=0.299 sigma_q1_arcsec=0.387 sigma_q2_arcsec=0.274 sigma_q3_arcsec=0.258 sigma_q4_arcsec=0.269 n_q1=299 n_q2=171 n_q3=307 n_q4=183 worst_quadrant_to_overall_ratio=1.293
The image catalog is written to wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits -region wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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.YS614r5c0A (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-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits' -> 'wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS_IMAGE_NAME=wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS-calibrated image found: wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Checking if the catalog wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat corresponding to the image wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat corresponding to the image wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS catalog name: wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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=11, blended=1474, bad_region=6618, passed=35033
Got 35033 stars (including 27216 good ones) from the SExtractor catalog wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat
util/solve_plate_with_UCAC5 got 35033 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 453 to 508 (Dec 0.7 to 11.3)
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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 28906 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 453 to 508 (Dec 0.7 to 11.3)
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(), 28906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 28907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits N_match=960 sigma_overall_arcsec=0.307 sigma_q1_arcsec=0.378 sigma_q2_arcsec=0.302 sigma_q3_arcsec=0.285 sigma_q4_arcsec=0.275 n_q1=286 n_q2=175 n_q3=316 n_q4=183 worst_quadrant_to_overall_ratio=1.232
The image catalog is written to wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits -region wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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.CdbJaXyNv0 (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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
Checking if the catalog wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
WCS catalog name: wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.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=148, bad_region=1118, passed=4409
Got 4409 stars (including 3221 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat
util/solve_plate_with_UCAC5 got 4409 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 3376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 3378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 3378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits N_match=946 sigma_overall_arcsec=0.558 sigma_q1_arcsec=0.525 sigma_q2_arcsec=0.528 sigma_q3_arcsec=0.569 sigma_q4_arcsec=0.713 n_q1=320 n_q2=234 n_q3=310 n_q4=82 worst_quadrant_to_overall_ratio=1.276
The image catalog is written to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits -region wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.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.uO7eFzxBPI (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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
Checking if the catalog wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
WCS catalog name: wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.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=148, bad_region=987, passed=4272
Got 4272 stars (including 3208 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits.wcscat
util/solve_plate_with_UCAC5 got 4272 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (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 0.010429 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 3335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 3335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 3335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits N_match=941 sigma_overall_arcsec=0.482 sigma_q1_arcsec=0.448 sigma_q2_arcsec=0.514 sigma_q3_arcsec=0.489 sigma_q4_arcsec=0.592 n_q1=318 n_q2=194 n_q3=335 n_q4=94 worst_quadrant_to_overall_ratio=1.227
The image catalog is written to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits -region wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.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-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-41-50_20.00sec_5.00C_LIGHT_0362.fits
Saving fully-calibrated image wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.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-06-Q2b1x1_041904_TTUQ2b1x1_320122_4UzXjVQS/wcs_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363.fits
Preparing the HTML report for the field Psc-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:25:30.34 +06:45:26.7: 12.04 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:25:26.88 +02:56:21.7: 12.63 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:54:51.58 +02:03:52.1: 12.96 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:29:50.51 +06:51:20.6: 12.23 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:00:10.95 +03:14:49.5: 12.94 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:00:00.20 +03:21:37.7: 12.61 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:56:13.18 +03:03:36.2: 12.53 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:30.01 +03:44:01.4: 12.20 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:00:13.53 +04:08:23.9: 12.59 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:54:54.57 +02:13:11.3: 12.58 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:25:30.34 +06:45:26.7: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry filter KEPT candidate at 01:25:30.34 +06:45:26.7: ref_mag=12.07 +/- 0.01 new_mean_mag=11.0701 delta=1.00 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:00:10.95 +03:14:49.5: 12.86 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:29:50.51 +06:51:20.6: 12.21 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:54:51.58 +02:03:52.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:56:13.18 +03:03:36.2: 12.60 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:00:00.20 +03:21:37.7: 12.64 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:30.01 +03:44:01.4: 12.16 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:25:26.88 +02:56:21.7: 12.67 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:00:13.53 +04:08:23.9: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter KEPT candidate at 01:29:50.51 +06:51:20.6: ref_mag=12.22 +/- 0.01 new_mean_mag=11.2587 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 02:00:10.95 +03:14:49.5: ref_mag=12.90 +/- 0.01 new_mean_mag=11.8170 delta=1.08 (need > 0.90)
Forced photometry filter KEPT candidate at 01:56:13.18 +03:03:36.2: ref_mag=12.56 +/- 0.01 new_mean_mag=11.6070 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 01:54:51.58 +02:03:52.1: ref_mag=12.94 +/- 0.02 new_mean_mag=11.7925 delta=1.15 (need > 0.90)
Forced photometry filter KEPT candidate at 02:00:00.20 +03:21:37.7: ref_mag=12.62 +/- 0.01 new_mean_mag=11.5999 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 01:59:30.01 +03:44:01.4: ref_mag=12.18 +/- 0.01 new_mean_mag=11.1487 delta=1.03 (need > 0.90)
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 01:25:26.88 +02:56:21.7: ref_mag=12.65 +/- 0.01 new_mean_mag=11.5285 delta=1.12 (need > 0.90)
Forced photometry filter KEPT candidate at 02:00:13.53 +04:08:23.9: ref_mag=12.59 +/- 0.01 new_mean_mag=11.5157 delta=1.08 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:54:54.57 +02:13:11.3: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter KEPT candidate at 01:54:54.57 +02:13:11.3: ref_mag=12.60 +/- 0.01 new_mean_mag=11.5857 delta=1.02 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:25.18 +02:05:20.8: 12.55 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:25.18 +02:05:20.8: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 01:59:25.18 +02:05:20.8: ref_mag=12.52 +/- 0.01 new_mean_mag=11.4874 delta=1.04 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:44.49 +03:36:55.3: 12.55 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:26:03.13 +03:33:50.8: 12.49 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:44.49 +03:36:55.3: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 01:58:44.49 +03:36:55.3: ref_mag=12.57 +/- 0.01 new_mean_mag=11.5730 delta=0.99 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:26:03.13 +03:33:50.8: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter KEPT candidate at 01:26:03.13 +03:33:50.8: ref_mag=12.50 +/- 0.01 new_mean_mag=11.4853 delta=1.01 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:56:56.01 +02:43:28.1: 12.49 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:56:56.01 +02:43:28.1: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter KEPT candidate at 01:56:56.01 +02:43:28.1: ref_mag=12.47 +/- 0.01 new_mean_mag=11.3823 delta=1.09 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:26:37.27 +06:57:17.8: 12.47 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:56:10.12 +02:35:31.7: 12.87 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:26:37.27 +06:57:17.8: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter KEPT candidate at 01:26:37.27 +06:57:17.8: ref_mag=12.49 +/- 0.01 new_mean_mag=11.4269 delta=1.06 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:56:10.12 +02:35:31.7: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 01:56:10.12 +02:35:31.7: ref_mag=12.86 +/- 0.01 new_mean_mag=11.7402 delta=1.12 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:09.56 +02:57:57.1: 12.43 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:09.56 +02:57:57.1: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter KEPT candidate at 01:59:09.56 +02:57:57.1: ref_mag=12.42 +/- 0.01 new_mean_mag=11.3820 delta=1.04 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:57:58.16 +03:00:41.5: 12.42 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:18.06 +04:12:53.9: 12.85 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:24:55.60 +05:47:52.2: 12.42 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:18.06 +04:12:53.9: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:24:55.60 +05:47:52.2: 12.39 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:57:58.16 +03:00:41.5: 12.43 +/- 0.01 detection
Forced photometry filter KEPT candidate at 01:59:18.06 +04:12:53.9: ref_mag=12.83 +/- 0.01 new_mean_mag=11.7773 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter KEPT candidate at 01:24:55.60 +05:47:52.2: ref_mag=12.40 +/- 0.01 new_mean_mag=11.3690 delta=1.03 (need > 0.90)
Forced photometry filter KEPT candidate at 01:57:58.16 +03:00:41.5: ref_mag=12.42 +/- 0.01 new_mean_mag=11.3642 delta=1.06 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:19.56 +02:13:57.9: 12.81 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:55:14.83 +01:45:35.5: 12.35 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:19.56 +02:13:57.9: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter KEPT candidate at 01:58:19.56 +02:13:57.9: ref_mag=12.79 +/- 0.01 new_mean_mag=11.7783 delta=1.02 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:55:14.83 +01:45:35.5: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 01:55:14.83 +01:45:35.5: ref_mag=12.36 +/- 0.01 new_mean_mag=11.3890 delta=0.97 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:00:38.76 +04:22:02.6: 12.35 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:28.70 +03:02:19.4: 12.75 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:31.75 +02:53:47.9: 12.73 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:00:38.76 +04:22:02.6: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 02:00:38.76 +04:22:02.6: ref_mag=12.33 +/- 0.01 new_mean_mag=11.2868 delta=1.05 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:28.70 +03:02:19.4: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 01:58:28.70 +03:02:19.4: ref_mag=12.75 +/- 0.01 new_mean_mag=11.6978 delta=1.05 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:31.75 +02:53:47.9: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 01:58:31.75 +02:53:47.9: ref_mag=12.72 +/- 0.01 new_mean_mag=11.6939 delta=1.02 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:56:49.35 +02:57:20.8: 12.74 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:56:49.35 +02:57:20.8: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 01:56:49.35 +02:57:20.8: ref_mag=12.76 +/- 0.01 new_mean_mag=11.5876 delta=1.18 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:57:52.60 +02:54:02.2: 12.70 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:57:52.60 +02:54:02.2: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 01:57:52.60 +02:54:02.2: ref_mag=12.68 +/- 0.01 new_mean_mag=11.6286 delta=1.06 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:51.29 +03:30:12.8: 12.32 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:51.29 +03:30:12.8: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 01:58:51.29 +03:30:12.8: ref_mag=12.35 +/- 0.01 new_mean_mag=11.3968 delta=0.95 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:26:31.80 +05:35:11.8: 12.33 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:26:31.80 +05:35:11.8: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:52.71 +03:25:43.8: 12.70 +/- 0.02 detection
Forced photometry filter KEPT candidate at 01:26:31.80 +05:35:11.8: ref_mag=12.29 +/- 0.01 new_mean_mag=11.3464 delta=0.94 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:52.71 +03:25:43.8: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 01:59:52.71 +03:25:43.8: ref_mag=12.69 +/- 0.01 new_mean_mag=11.6434 delta=1.04 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:53.29 +04:13:51.9: 12.99 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:53.29 +04:13:51.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter KEPT candidate at 01:59:53.29 +04:13:51.9: ref_mag=12.98 +/- 0.02 new_mean_mag=11.7894 delta=1.19 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:25.22 +02:02:04.8: 12.67 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:25.22 +02:02:04.8: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 01:58:25.22 +02:02:04.8: ref_mag=12.69 +/- 0.01 new_mean_mag=11.7044 delta=0.98 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:47.45 +03:48:02.0: 12.96 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:25:33.85 +03:44:56.9: 12.25 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:47.45 +03:48:02.0: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 01:59:47.45 +03:48:02.0: ref_mag=12.99 +/- 0.02 new_mean_mag=11.7153 delta=1.28 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:25:33.85 +03:44:56.9: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 01:25:33.85 +03:44:56.9: ref_mag=12.26 +/- 0.01 new_mean_mag=11.2804 delta=0.98 (need > 0.90)
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:59:45.78 +02:00:15.7: 12.65 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q2b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:59:45.78 +02:00:15.7: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 01:59:45.78 +02:00:15.7: ref_mag=12.64 +/- 0.01 new_mean_mag=11.6391 delta=1.00 (need > 0.90)
Adding exclusion_list_local.txt__out14576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34678.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 46s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 16s
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Considering the candidate 52437_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
The candidate 52437_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363 did not pass the final checks
**** FOUND 01:56:00.02 +01:51:00.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 33952_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 33952_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 29479_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 29479_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 14861_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 14861_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 32086_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 32086_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 30933_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 30933_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 26475_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 26475_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 30586_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 30586_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 15239_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 15239_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 32549_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 32549_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 27018_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 27018_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 26612_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 26612_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 31738_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 31738_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 30973_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 30973_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 28766_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 28766_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 14576_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 14576_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 28257_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 28257_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 29625_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 29625_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 29741_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 29741_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 33696_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 33696_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 18652_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 18652_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
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Considering the candidate 27030_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 27030_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25431_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 25431_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34251_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 34251_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29871_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 29871_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29365_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 29365_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29601_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 29601_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29353_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 29353_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31426_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 31426_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19393_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 19393_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31082_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 31082_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33851_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 33851_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34678_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 34678_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32204_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 32204_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32397_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 32397_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29060_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
Preparing report for the candidate 29060_fd_Psc-06-Q2b1x1_2026-07-10_03-42-57_20.00sec_5.00C_LIGHT_0363
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 65s
Prepared the HTML report for the field Psc-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:59:12.87 +03:31:10.8
01:26:37.27 +06:57:17.8
01:29:50.51 +06:51:20.6
01:25:30.34 +06:45:26.7
01:24:55.60 +05:47:52.2
01:26:31.80 +05:35:11.8
01:55:14.83 +01:45:35.5
01:54:51.58 +02:03:52.1
01:59:25.18 +02:05:20.8
01:54:54.57 +02:13:11.3
01:58:19.56 +02:13:57.9
01:56:10.12 +02:35:31.7
01:56:56.01 +02:43:28.1
01:59:45.78 +02:00:15.7
01:57:52.60 +02:54:02.2
01:58:31.75 +02:53:47.9
01:25:26.88 +02:56:21.7
01:56:49.35 +02:57:20.8
01:59:09.56 +02:57:57.1
01:57:58.16 +03:00:41.5
01:58:28.70 +03:02:19.4
02:00:10.95 +03:14:49.5
02:00:00.20 +03:21:37.7
01:26:03.13 +03:33:50.8
01:59:52.71 +03:25:43.8
01:58:51.29 +03:30:12.8
01:58:44.49 +03:36:55.3
01:59:30.01 +03:44:01.4
01:59:47.45 +03:48:02.0
01:25:33.85 +03:44:56.9
02:00:13.53 +04:08:23.9
01:59:18.06 +04:12:53.9
01:59:53.29 +04:13:51.9
01:56:13.18 +03:03:36.2
02:00:38.76 +04:22:02.6
01:58:25.22 +02:02:04.8
########### Completed Psc-06-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:59:12.87 +03:31:10.8
01:56:13.18 +03:03:36.2
01:25:26.88 +02:56:21.7
01:29:50.51 +06:51:20.6
01:59:30.01 +03:44:01.4
02:00:00.20 +03:21:37.7
01:54:51.58 +02:03:52.1
02:00:10.95 +03:14:49.5
01:25:30.34 +06:45:26.7
02:00:13.53 +04:08:23.9
01:54:54.57 +02:13:11.3
01:59:25.18 +02:05:20.8
01:58:44.49 +03:36:55.3
01:26:03.13 +03:33:50.8
01:56:56.01 +02:43:28.1
01:26:37.27 +06:57:17.8
01:56:10.12 +02:35:31.7
01:59:09.56 +02:57:57.1
01:57:58.16 +03:00:41.5
01:59:18.06 +04:12:53.9
01:24:55.60 +05:47:52.2
01:58:19.56 +02:13:57.9
01:55:14.83 +01:45:35.5
02:00:38.76 +04:22:02.6
01:58:28.70 +03:02:19.4
01:58:31.75 +02:53:47.9
01:56:49.35 +02:57:20.8
01:57:52.60 +02:54:02.2
01:58:51.29 +03:30:12.8
01:26:31.80 +05:35:11.8
01:59:52.71 +03:25:43.8
01:59:53.29 +04:13:51.9
01:58:25.22 +02:02:04.8
01:59:47.45 +03:48:02.0
01:25:33.85 +03:44:56.9
01:59:45.78 +02:00:15.7
###################################################################################
01:59:12.87 +03:31:10.8 -- not an asteroid (will add it to exclusion list)
01:56:13.18 +03:03:36.2 -- not an asteroid (will add it to exclusion list)
01:25:26.88 +02:56:21.7 -- not an asteroid (will add it to exclusion list)
01:29:50.51 +06:51:20.6 -- not an asteroid (will add it to exclusion list)
01:59:30.01 +03:44:01.4 -- not an asteroid (will add it to exclusion list)
02:00:00.20 +03:21:37.7 -- not an asteroid (will add it to exclusion list)
01:54:51.58 +02:03:52.1 -- not an asteroid (will add it to exclusion list)
02:00:10.95 +03:14:49.5 -- not an asteroid (will add it to exclusion list)
01:25:30.34 +06:45:26.7 -- not an asteroid (will add it to exclusion list)
02:00:13.53 +04:08:23.9 -- not an asteroid (will add it to exclusion list)
01:54:54.57 +02:13:11.3 -- asteroid (will NOT add it to exclusion list)
01:59:25.18 +02:05:20.8 -- not an asteroid (will add it to exclusion list)
01:58:44.49 +03:36:55.3 -- not an asteroid (will add it to exclusion list)
01:26:03.13 +03:33:50.8 -- not an asteroid (will add it to exclusion list)
01:56:56.01 +02:43:28.1 -- not an asteroid (will add it to exclusion list)
01:26:37.27 +06:57:17.8 -- asteroid (will NOT add it to exclusion list)
01:56:10.12 +02:35:31.7 -- not an asteroid (will add it to exclusion list)
01:59:09.56 +02:57:57.1 -- not an asteroid (will add it to exclusion list)
01:57:58.16 +03:00:41.5 -- not an asteroid (will add it to exclusion list)
01:59:18.06 +04:12:53.9 -- not an asteroid (will add it to exclusion list)
01:24:55.60 +05:47:52.2 -- asteroid (will NOT add it to exclusion list)
01:58:19.56 +02:13:57.9 -- not an asteroid (will add it to exclusion list)
01:55:14.83 +01:45:35.5 -- not an asteroid (will add it to exclusion list)
02:00:38.76 +04:22:02.6 -- not an asteroid (will add it to exclusion list)
01:58:28.70 +03:02:19.4 -- not an asteroid (will add it to exclusion list)
01:58:31.75 +02:53:47.9 -- not an asteroid (will add it to exclusion list)
01:56:49.35 +02:57:20.8 -- not an asteroid (will add it to exclusion list)
01:57:52.60 +02:54:02.2 -- not an asteroid (will add it to exclusion list)
01:58:51.29 +03:30:12.8 -- not an asteroid (will add it to exclusion list)
01:26:31.80 +05:35:11.8 -- not an asteroid (will add it to exclusion list)
01:59:52.71 +03:25:43.8 -- not an asteroid (will add it to exclusion list)
01:59:53.29 +04:13:51.9 -- not an asteroid (will add it to exclusion list)
01:58:25.22 +02:02:04.8 -- not an asteroid (will add it to exclusion list)
01:59:47.45 +03:48:02.0 -- not an asteroid (will add it to exclusion list)
01:25:33.85 +03:44:56.9 -- not an asteroid (will add it to exclusion list)
01:59:45.78 +02:00:15.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:25:26.88 +02:56:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:30.34 +06:45:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:33.85 +03:44:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:03.13 +03:33:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:31.80 +05:35:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:50.51 +06:51:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:51.58 +02:03:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:14.83 +01:45:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:10.12 +02:35:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:13.18 +03:03:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:49.35 +02:57:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:56.01 +02:43:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:52.60 +02:54:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:58.16 +03:00:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:19.56 +02:13:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:25.22 +02:02:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:28.70 +03:02:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:31.75 +02:53:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:44.49 +03:36:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:51.29 +03:30:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:09.56 +02:57:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:12.87 +03:31:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:18.06 +04:12:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:25.18 +02:05:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:30.01 +03:44:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:45.78 +02:00:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:47.45 +03:48:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:52.71 +03:25:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:53.29 +04:13:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:00.20 +03:21:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:10.95 +03:14:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:13.53 +04:08:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:38.76 +04:22:02.6 -- 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)
01:25:26.88 +02:56:21.7 -- a known variable star
01:25:30.34 +06:45:26.7 -- not a known variable star
01:25:33.85 +03:44:56.9 -- not a known variable star
01:26:03.13 +03:33:50.8 -- not a known variable star
01:26:31.80 +05:35:11.8 -- not a known variable star
01:29:50.51 +06:51:20.6 -- not a known variable star
01:54:51.58 +02:03:52.1 -- not a known variable star
01:55:14.83 +01:45:35.5 -- not a known variable star
01:56:10.12 +02:35:31.7 -- not a known variable star
01:56:13.18 +03:03:36.2 -- not a known variable star
01:56:49.35 +02:57:20.8 -- not a known variable star
01:56:56.01 +02:43:28.1 -- not a known variable star
01:57:52.60 +02:54:02.2 -- not a known variable star
01:57:58.16 +03:00:41.5 -- not a known variable star
01:58:19.56 +02:13:57.9 -- not a known variable star
01:58:25.22 +02:02:04.8 -- not a known variable star
01:58:28.70 +03:02:19.4 -- not a known variable star
01:58:31.75 +02:53:47.9 -- not a known variable star
01:58:44.49 +03:36:55.3 -- not a known variable star
01:58:51.29 +03:30:12.8 -- a known variable star
01:59:09.56 +02:57:57.1 -- not a known variable star
01:59:12.87 +03:31:10.8 -- not a known variable star
01:59:18.06 +04:12:53.9 -- not a known variable star
01:59:25.18 +02:05:20.8 -- not a known variable star
01:59:30.01 +03:44:01.4 -- not a known variable star
01:59:45.78 +02:00:15.7 -- not a known variable star
01:59:47.45 +03:48:02.0 -- not a known variable star
01:59:52.71 +03:25:43.8 -- not a known variable star
01:59:53.29 +04:13:51.9 -- a known variable star
02:00:00.20 +03:21:37.7 -- a known variable star
02:00:10.95 +03:14:49.5 -- not a known variable star
02:00:13.53 +04:08:23.9 -- not a known variable star
02:00:38.76 +04:22:02.6 -- not a known variable star
Found 29 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
33 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
01:25:26.88 +02:56:21.7
01:25:30.34 +06:45:26.7
01:25:33.85 +03:44:56.9
01:26:03.13 +03:33:50.8
01:26:31.80 +05:35:11.8
01:29:50.51 +06:51:20.6
01:54:51.58 +02:03:52.1
01:55:14.83 +01:45:35.5
01:56:10.12 +02:35:31.7
01:56:13.18 +03:03:36.2
01:56:49.35 +02:57:20.8
01:56:56.01 +02:43:28.1
01:57:52.60 +02:54:02.2
01:57:58.16 +03:00:41.5
01:58:19.56 +02:13:57.9
01:58:25.22 +02:02:04.8
01:58:28.70 +03:02:19.4
01:58:31.75 +02:53:47.9
01:58:44.49 +03:36:55.3
01:58:51.29 +03:30:12.8
01:59:09.56 +02:57:57.1
01:59:12.87 +03:31:10.8
01:59:18.06 +04:12:53.9
01:59:25.18 +02:05:20.8
01:59:30.01 +03:44:01.4
01:59:45.78 +02:00:15.7
01:59:47.45 +03:48:02.0
01:59:52.71 +03:25:43.8
01:59:53.29 +04:13:51.9
02:00:00.20 +03:21:37.7
02:00:10.95 +03:14:49.5
02:00:13.53 +04:08:23.9
02:00:38.76 +04:22:02.6
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461231.86250455 -observatory V36
07:32:14.91 +17:07:59.6 Mercury (5.1mag)
10:11:41.81 +12:40:41.0 Venus (-4.1mag)
04:24:12.46 +21:25:17.7 Mars (1.3mag)
08:16:41.22 +20:11:26.9 Jupiter (-1.8mag)
00:55:50.99 +03:20:29.1 Saturn (0.7mag)
04:07:14.18 +20:45:03.8 Uranus (5.8mag)
00:17:01.49 +00:20:41.1 Neptune (7.8mag)
20:30:54.88 -23:18:01.0 Pluto (14.4mag)
03:12:30.38 +22:25:12.8 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 361 Jul 10 06:38 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461231.86250455:
08:16:48.08 +20:11:03.0 Io (6.1mag)
08:16:44.29 +20:11:17.3 Europa (6.3mag)
08:16:58.34 +20:10:25.0 Ganymede (5.6mag)
08:17:09.15 +20:09:43.7 Callisto (6.8mag)
08:15:12.68 +19:55:36.9 Himalia (15.7mag)
08:16:40.77 +20:11:29.5 Thebe (16.6mag)
08:14:34.01 +20:00:06.2 Elara (17.6mag)
08:20:13.46 +20:05:36.7 Pasiphae (17.8mag)
08:21:39.03 +20:16:32.1 Carme (19.0mag)
00:55:40.88 +03:20:19.8 Titan (8.5mag)
00:55:45.74 +03:20:31.9 Rhea (9.8mag)
00:55:20.26 +03:19:37.9 Iapetus (11.2mag)
00:56:00.18 +03:20:48.3 Hyperion (14.5mag)
00:55:51.69 +03:17:42.8 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 06:38 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.86250455:
17:46:05.39 -32:58:48.3 JWST
16:16:35.67 +48:18:27.7 Chandra
03:56:45.19 +57:09:43.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 06:38 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.86250455 -observatory V36
02:36:17.11 +14:25:46.6 17.9mag P/1996 R2 (Lagerkvist)
18:17:55.85 -34:21:46.5 13.7mag P/2010 H2 (Vales)
06:25:41.14 -68:08:23.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:48.60 +32:26:49.7 17.6mag C/2017 K2 (PANSTARRS)
17:03:06.77 +16:02:54.2 18.0mag C/2021 G2 (ATLAS)
01:47:52.09 +08:14:35.4 15.4mag P/2021 N1 (ZTF)
22:59:31.49 +32:17:08.1 17.3mag C/2022 E2 (ATLAS)
06:12:24.73 +26:55:34.4 16.7mag C/2022 N2 (PANSTARRS)
09:55:31.48 +29:46:49.5 16.8mag C/2022 QE78 (ATLAS)
09:09:44.54 +04:59:58.0 17.8mag C/2022 R6 (PANSTARRS)
18:07:12.68 +21:17:36.5 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:35.16 -11:23:16.8 17.7mag P/2023 B1 (PANSTARRS)
21:49:13.29 +67:37:16.6 17.8mag C/2023 H5 (Lemmon)
16:30:51.83 -10:04:45.6 13.9mag C/2023 R1 (PANSTARRS)
08:00:40.16 +65:42:32.4 17.9mag C/2024 A1 (ATLAS)
07:32:49.74 +30:00:14.0 14.6mag C/2024 E1 (Wierzchos)
15:16:19.25 +15:19:43.1 17.5mag C/2024 G6 (ATLAS)
19:41:17.75 +39:23:42.7 13.8mag C/2024 J3 (ATLAS)
21:47:34.30 +46:00:17.7 17.8mag C/2024 R4 (PANSTARRS)
04:49:38.97 -13:47:43.5 15.7mag C/2024 T5 (ATLAS)
06:34:34.93 +29:04:05.1 18.0mag C/2025 J1 (Borisov)
07:14:20.83 -12:53:26.1 16.5mag C/2025 R3 (PANSTARRS)
09:56:06.25 +22:26:11.1 17.6mag C/2025 V2 (Rankin)
12:44:37.23 +03:56:14.5 17.1mag C/2025 Y1 (ATLAS)
16:51:55.33 +79:07:13.9 17.4mag C/2026 A2 (Bok)
02:46:17.24 +45:14:25.3 16.7mag C/2026 B2 (Sun-Gao)
11:25:31.08 +04:32:45.8 16.9mag A/2026 E1
21:19:03.11 -15:04:48.5 7.3mag 10P/Tempel
11:13:27.60 -01:53:15.5 16.1mag 29P/Schwassmann-Wachmann
04:00:11.25 +29:33:15.6 17.8mag 47P/Ashbrook-Jackson
10:08:05.91 +14:00:29.2 17.0mag 63P/Wild
00:48:22.02 -05:05:34.8 15.5mag 65P/Gunn
08:26:59.15 +34:13:06.1 17.9mag 76P/West-Kohoutek-Ikemura
04:27:25.40 +20:10:45.7 13.7mag 78P/Gehrels
02:22:21.07 +10:36:39.6 16.2mag 88P/Howell
06:35:33.69 +30:32:03.3 15.7mag 93P/Lovas
04:21:01.96 +31:07:24.7 16.9mag 114P/Wiseman-Skiff
08:08:43.19 +30:42:08.6 15.2mag 123P/West-Hartley
10:48:09.04 +01:10:57.8 16.8mag 124P/Mrkos
04:51:44.69 +20:48:47.9 16.2mag 128P/Shoemaker-Holt
05:36:16.51 +19:42:50.4 17.8mag 131P/Mueller
00:01:32.89 +02:56:08.4 17.9mag 139P/Vaisala-Oterma
07:13:36.03 +17:01:06.7 15.5mag 141P-D/Machholz
03:16:51.22 -21:06:18.3 15.5mag 161P/Hartley-IRAS
05:33:06.03 +33:57:03.3 15.3mag 162P/SidingSpring
19:04:26.78 +15:05:19.0 14.7mag 169P/NEAT
01:41:03.28 +07:35:59.5 17.7mag 220P/McNaught
16:35:58.02 -08:23:08.7 17.0mag 235P/LINEAR
08:45:18.45 +33:17:54.7 17.9mag 240P/NEAT
20:42:10.17 -49:34:22.6 17.8mag 259P/Garradd
01:59:20.09 +12:05:58.5 15.7mag 260P/McNaught
05:37:15.43 +36:50:37.7 17.4mag 295P/LINEAR
15:06:36.75 +06:03:21.6 17.6mag 391P/Kowalski
08:34:36.77 +19:40:34.9 17.9mag 450P/LONEOS
07:51:46.97 +39:12:55.2 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 06:38 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 06:37 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 06:37 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 06:37 tns_transients_list.txt
