This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe
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 06 28.2761 2461219.7761 8.79 01:56:38.07 +59:15:33.8
131.18812 -2.56326 galactic Cas Second-epoch detections are separated by 0.4" and 6.2 pix
The object was found in VSX 0" X Cas
Type: M
# Max. Min./Amp. JD0 Period
9.450 V 13.200 V 2457020.00000 415.000000000000 C5,4e(N1e)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.07 +59:15:33.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.07 +59:15:33.8: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 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!
TCP 2026 06 28.2761* 01 56 38.07 +59 15 33.8 8.8 U Cas 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
X Cas,2461219.7761,8.79,0.05,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
X Cas 20260628.2761 8.79CV 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 06 28.2761 2461219.7761 10.74 01:29:41.94 +61:54:41.8
127.41953 -0.62631 galactic Cas Second-epoch detections are separated by 2.1" 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 510818331883633920 | 01:29:42.46 +61:55:01.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:41.94 +61:54:41.8: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:41.94 +61:54:41.8: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 28.2761* 01 29 41.94 +61 54 41.8 10.7 U Cas 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 510818331883633920,2461219.7761,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510818331883633920 20260628.2761 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 10.70 01:47:29.16 +61:08:58.5
129.64220 -0.98983 galactic Cas Second-epoch detections are separated by 1.0" 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 511213193996592512 | 01:47:26.76 +61:08:44.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B3 1953IzKry..10..120K [K53] 578 J-Ks=0.330+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:29.16 +61:08:58.5: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:29.16 +61:08:58.5: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 28.2761* 01 47 29.16 +61 08 58.5 10.7 U Cas 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 511213193996592512,2461219.7761,10.70,0.05,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
Gaia DR3 511213193996592512 20260628.2761 10.70CV 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 06 28.2761 2461219.7761 10.56 01:38:41.38 +58:14:18.2
129.13379 -4.06324 galactic Cas Second-epoch detections are separated by 1.0" 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 | ATO J024.6670+58.2524 | 01:38:40.23 +58:14:35.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.747+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:41.38 +58:14:18.2: 10.58 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:41.38 +58:14:18.2: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.77 +/- 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 06 28.2761* 01 38 41.38 +58 14 18.2 10.6 U Cas 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
ATO J024.6670+58.2524,2461219.7761,10.56,0.05,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
ATO J024.6670+58.2524 20260628.2761 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 10.73 01:49:15.74 +59:14:39.5
130.27511 -2.80053 galactic Cas 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 | Gaia DR3 506536352570768768 | 01:49:14.31 +59:14:50.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.811+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:15.74 +59:14:39.5: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:15.74 +59:14:39.5: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 06 28.2761* 01 49 15.74 +59 14 39.5 10.7 U Cas 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 506536352570768768,2461219.7761,10.73,0.05,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
Gaia DR3 506536352570768768 20260628.2761 10.73CV 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 06 28.2761 2461219.7761 10.57 01:41:24.55 +59:57:28.9
129.15407 -2.30865 galactic Cas Second-epoch detections are separated by 2.0" and 6.4 pix
The object was found in VSX23" Gaia DR3 509584576760542976
Type: ROT
# Max. Min./Amp. JD0 Period
17.450 G 17.580 G 19.098000000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:24.55 +59:57:28.9: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:24.55 +59:57:28.9: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 28.2761* 01 41 24.55 +59 57 28.9 10.6 U Cas 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 509584576760542976,2461219.7761,10.57,0.05,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 509584576760542976 20260628.2761 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 10.22 01:41:26.11 +60:54:33.5
128.97384 -1.37458 galactic Cas Second-epoch detections are separated by 0.6" and 6.4 pix
The object was found in VSX14" Gaia DR3 509740947930653696
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.880 G 12.920 G 0.073279700000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:26.11 +60:54:33.5: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:26.11 +60:54:33.5: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 28.2761* 01 41 26.11 +60 54 33.5 10.2 U Cas 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 509740947930653696,2461219.7761,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509740947930653696 20260628.2761 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 10.43 01:22:28.28 +61:07:37.5
126.67071 -1.51918 galactic Cas Second-epoch detections are separated by 4.2" and 5.9 pix
The object was found in VSX21" Gaia DR3 510501328936368640
Type: RS
# Max. Min./Amp. JD0 Period
13.970 G 14.040 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:28.28 +61:07:37.5: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:28.28 +61:07:37.5: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 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 06 28.2761* 01 22 28.28 +61 07 37.5 10.4 U Cas 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 510501328936368640,2461219.7761,10.43,0.05,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
Gaia DR3 510501328936368640 20260628.2761 10.43CV 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 06 28.2761 2461219.7761 10.21 01:11:31.93 +57:31:00.7
125.63873 -5.24924 galactic Cas Second-epoch detections are separated by 1.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:11:31.93 +57:31:00.7 (user input) | T | P | (position from user input) J-Ks=0.258+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:31.93 +57:31:00.7: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:31.93 +57:31:00.7: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 06 28.2761* 01 11 31.93 +57 31 00.7 10.2 U Cas 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,2461219.7761,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260628.2761 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 10.28 02:00:56.12 +59:46:32.4
131.58220 -1.92377 galactic Cas Second-epoch detections are separated by 3.6" and 6.0 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 | ZTF J020053.46+594548.7 | 02:00:54.41 +59:46:11.4 (Gaia DR3) | EW (local) | 2458347.92740 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.367+/-0.069 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:56.12 +59:46:32.4: 11.10 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:56.12 +59:46:32.4: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 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 06 28.2761* 02 00 56.12 +59 46 32.4 10.3 U Cas 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
ZTF J020053.46+594548.7,2461219.7761,10.28,0.05,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
ZTF J020053.46+594548.7 20260628.2761 10.28CV 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 06 28.2761 2461219.7761 10.20 01:08:48.96 +60:05:00.3
125.09957 -2.71517 galactic Cas Second-epoch detections are separated by 2.0" 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 426320347891252480 | 01:08:48.82 +60:05:17.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.837+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:48.96 +60:05:00.3: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:48.96 +60:05:00.3: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 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 06 28.2761* 01 08 48.96 +60 05 00.3 10.2 U Cas 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 426320347891252480,2461219.7761,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426320347891252480 20260628.2761 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 9.95 01:45:34.94 +59:18:10.4
129.80289 -2.84463 galactic Cas Second-epoch detections are separated by 2.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.3995+59.3029 | 01:45:34.94 +59:18:10.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:34.94 +59:18:10.4: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:34.94 +59:18:10.4: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 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 06 28.2761* 01 45 34.94 +59 18 10.4 9.9 U Cas 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
ATO J026.3995+59.3029,2461219.7761,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.3995+59.3029 20260628.2761 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 9.88 01:35:24.94 +60:39:17.6
128.29730 -1.75791 galactic Cas Second-epoch detections are separated by 0.3" and 6.5 pix
The object was found in VSX 6" Gaia DR3 509819081975016960
Type: S
# Max. Min./Amp. JD0 Period
17.140 G 17.450 G O
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:24.94 +60:39:17.6: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:24.94 +60:39:17.6: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 28.2761* 01 35 24.94 +60 39 17.6 9.9 U Cas 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 509819081975016960,2461219.7761,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509819081975016960 20260628.2761 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 9.79 01:23:31.52 +58:41:49.0
127.09958 -3.91491 galactic Cas Second-epoch detections are separated by 2.0" and 6.2 pix
The object was found in VSX22" Gaia DR3 413949673852809088
Type: ROT
# Max. Min./Amp. JD0 Period
16.410 G 16.550 G 1.041480000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:31.52 +58:41:49.0: 12.17 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:31.52 +58:41:49.0: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 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 06 28.2761* 01 23 31.52 +58 41 49.0 9.8 U Cas 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 413949673852809088,2461219.7761,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413949673852809088 20260628.2761 9.79CV 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 06 28.2761 2461219.7761 9.35 01:48:51.20 +59:35:50.3
130.14601 -2.46784 galactic Cas Second-epoch detections are separated by 4.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506595038995541376 | 01:48:49.64 +59:36:01.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:51.20 +59:35:50.3: 12.60 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:51.20 +59:35:50.3: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 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 06 28.2761* 01 48 51.20 +59 35 50.3 9.3 U Cas 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 506595038995541376,2461219.7761,9.35,0.05,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 506595038995541376 20260628.2761 9.35CV 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 06 28.2761 2461219.7761 8.44 01:19:35.37 +60:03:33.4
126.44159 -2.62049 galactic Cas Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510326059911501184 | 01:19:36.00 +60:03:49.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1935BSD...C01....0S BSD 8- 783 J-Ks=0.314+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:35.37 +60:03:33.4: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:35.37 +60:03:33.4: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 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!
TCP 2026 06 28.2761* 01 19 35.37 +60 03 33.4 8.4 U Cas 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 510326059911501184,2461219.7761,8.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510326059911501184 20260628.2761 8.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 8.32 01:33:24.29 +60:39:45.6
128.05298 -1.79113 galactic Cas Second-epoch detections are separated by 0.7" and 6.3 pix
The object was found in VSX 1" NSV 543
Type:
# Max. Min./Amp. JD0 Period
11.480 V B2Ve
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:24.29 +60:39:45.6: 10.72 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:24.29 +60:39:45.6: 11.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.18 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 28.2761* 01 33 24.29 +60 39 45.6 8.3 U Cas 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
NSV 543,2461219.7761,8.32,0.05,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
NSV 543 20260628.2761 8.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 8.78 01:46:02.35 +61:13:14.6
129.45669 -0.95742 galactic Cas Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | V0978 Cas | 01:46:04.90 +61:13:41.8 (Gaia DR3) | BE (local) | B0/1Ve (local) | Gaia3var=NOT_AVAILABLE SpType: OB 1928MeUpp..37....1S BD+60 333 J-Ks=0.236+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:02.35 +61:13:14.6: 11.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:02.35 +61:13:14.6: 11.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 28.2761* 01 46 02.35 +61 13 14.6 8.8 U Cas 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
V0978 Cas,2461219.7761,8.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0978 Cas 20260628.2761 8.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 10.26 01:07:56.92 +63:37:30.6
124.76452 0.81218 galactic Cas Second-epoch detections are separated by 3.9" and 6.3 pix
The object was found in VSX23" V1064 Cas
Type: EW
# Max. Min./Amp. JD0 Period
11.300 R1 11.800 R1 2451349.91900 0.457606000000 B2
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:56.92 +63:37:30.6: 10.68 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:56.92 +63:37:30.6: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 28.2761* 01 07 56.92 +63 37 30.6 10.3 U Cas 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
V1064 Cas,2461219.7761,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1064 Cas 20260628.2761 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 10.17 01:57:04.43 +58:53:28.0
131.33532 -2.90560 galactic Cas Second-epoch detections are separated by 1.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506288893734057856 | 01:57:03.38 +58:53:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.729+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:04.43 +58:53:28.0: 13.13 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:04.43 +58:53:28.0: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 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 06 28.2761* 01 57 04.43 +58 53 28.0 10.2 U Cas 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 506288893734057856,2461219.7761,10.17,0.05,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 506288893734057856 20260628.2761 10.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 10.44 01:09:29.74 +61:47:05.0
125.06490 -1.01222 galactic Cas Second-epoch detections are separated by 4.7" and 5.7 pix
The object was found in VSX 2" ZTF J010929.80+614703.2
Type: RS
# Max. Min./Amp. JD0 Period
13.138 r Y 0.060 r 2458523.67140 4.708071800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:29.74 +61:47:05.0: 10.23 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:29.74 +61:47:05.0: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.43 +/- 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 06 28.2761* 01 09 29.74 +61 47 05.0 10.4 U Cas 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
ZTF J010929.80+614703.2,2461219.7761,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J010929.80+614703.2 20260628.2761 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 28.2761 2461219.7761 10.71 02:02:42.47 +60:04:29.3
131.71561 -1.57590 galactic Cas Second-epoch detections are separated by 2.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 507936511903779840 | 02:02:37.17 +60:04:47.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB 1928MeUpp..37....1S BD+59 387 J-Ks=0.223+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:42.47 +60:04:29.3: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:42.47 +60:04:29.3: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 28.2761* 02 02 42.47 +60 04 29.3 10.7 U Cas 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 507936511903779840,2461219.7761,10.71,0.05,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 507936511903779840 20260628.2761 10.71CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461219.77640855 28.06.2026 06:37:51.699 /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
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: 6 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): 23591
Objects passed selection criteria: 23398
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 14748.5
Average stars matched: 13849.5 (93.9045 %)
Memory usage VmPeak: 128528 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sat Jun 27 15:05:05 CDT 2026
VaST build number 1.0rc89-110-ga10a059d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-27)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 28 03:35:41 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: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461219.77640855 28.06.2026 06:37:51.699 /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 122
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
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: 60 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): 176413
Objects passed selection criteria: 175909
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 118828
Average stars matched: 110508 (92.9981 %)
Memory usage VmPeak: 1935072 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sat Jun 27 15:05:05 CDT 2026
VaST build number 1.0rc89-110-ga10a059d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-27)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 28 03:42:30 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/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.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: 2461219.77579468
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_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits'
wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.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: 01:42:55.038 +61:58:24.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:55.038 +61:58:24.83
Angular distance between the image centers 0.0528 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.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: 01:42:56.263 +61:59:01.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:56.263 +61:59:01.09
Angular distance between the image centers 0.0540 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 01:42:55.038 +61:58:24.83
Second-epoch second image center 01:42:56.263 +61:59:01.09
Angular distance between the image centers 0.01035 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.4jtTEKBcya
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.TdjdGCrdJ0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits &> /tmp/tmp.UzShf3mzl7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits &> /tmp/tmp.TQpSGHIaj3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat' -> 'wcsmag.cat'
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 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 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 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): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929150
a=0.000000 b=1.000000 c=22.929150
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 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 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 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): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=5.8)
Read 31681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.0659 to 45.7628 deg, Dec +55.3336 to +67.4023 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 7.0659 to 45.7628 deg, Dec 55.3336 to 67.4023 deg
Loaded 26179 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): 14497 out of 16269 total matches.
Matched with Tycho-2 16269 out of 31681 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
13.5 mag. fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
13.5 mag. fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.8 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.4jtTEKBcya (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/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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=3786, bad_region=8115, passed=31559
Got 31559 stars (including 20507 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
util/solve_plate_with_UCAC5 got 31559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 272 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 181 matched stars entering correct_measured_positions(), 127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 166 matched stars entering correct_measured_positions(), 5658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.17"
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 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 329 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 253 matched stars entering correct_measured_positions(), 5719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.16"
Accuracy estimation diagnostic: 250 matched stars entering correct_measured_positions(), 8204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.77"
Excluding outliers - 250 stars left (next iteration limit 182)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=250 sigma_overall_arcsec=18.752 sigma_q1_arcsec=37.068 sigma_q2_arcsec=15.069 sigma_q3_arcsec=23.291 sigma_q4_arcsec=16.683 n_q1=21 n_q2=98 n_q3=46 n_q4=85 worst_quadrant_to_overall_ratio=1.977
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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.TdjdGCrdJ0 (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/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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=3692, bad_region=8179, passed=31681
Got 31681 stars (including 20613 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat
util/solve_plate_with_UCAC5 got 31681 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 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 23244 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 23245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 23245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=975 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.464 sigma_q2_arcsec=0.388 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.289 n_q1=173 n_q2=179 n_q3=388 n_q4=235 worst_quadrant_to_overall_ratio=1.235
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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.UzShf3mzl7 (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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.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=688, bad_region=1641, passed=7784
Got 7784 stars (including 5600 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat
util/solve_plate_with_UCAC5 got 7784 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 728 to 788 (Dec 55.8 to 67.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 6297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 728 to 788 (Dec 55.8 to 67.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 969 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits N_match=969 sigma_overall_arcsec=0.615 sigma_q1_arcsec=0.566 sigma_q2_arcsec=0.482 sigma_q3_arcsec=0.810 sigma_q4_arcsec=0.710 n_q1=335 n_q2=248 n_q3=270 n_q4=116 worst_quadrant_to_overall_ratio=1.317
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.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.TQpSGHIaj3 (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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.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=680, bad_region=1664, passed=7878
Got 7878 stars (including 5692 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat
util/solve_plate_with_UCAC5 got 7878 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 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 6407 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6406 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6406 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 969 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits N_match=969 sigma_overall_arcsec=0.602 sigma_q1_arcsec=0.599 sigma_q2_arcsec=0.476 sigma_q3_arcsec=0.752 sigma_q4_arcsec=0.768 n_q1=332 n_q2=252 n_q3=266 n_q4=119 worst_quadrant_to_overall_ratio=1.276
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.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=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=18.752 worst_q_ratio=1.977
ref2=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=0.376 worst_q_ratio=1.235
new1=fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits sigma_overall=0.615 worst_q_ratio=1.317
new2=fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits sigma_overall=0.602 worst_q_ratio=1.276
reference average sigma_overall=9.564 worst_q_ratio=1.606
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018_astrometric_residuals.png (250 matched stars from wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 8.01 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019_astrometric_residuals.png (975 matched stars from wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234_astrometric_residuals.png (969 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.57 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235_astrometric_residuals.png (969 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.57 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.07 +59:15:33.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.07 +59:15:33.8: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter KEPT candidate at 01:56:38.07 +59:15:33.8: ref_mag=9.75 +/- 0.00 new_mean_mag=8.7898 delta=0.96 (need > 0.90)
Adding exclusion_list_local.txt__out20109.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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 52510_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 52510_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:19:46.48 +58:12:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20109_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 20109_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Cas-03-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 ####
01:56:38.07 +59:15:33.8
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/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.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_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.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: 01:42:55.038 +61:58:24.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:55.038 +61:58:24.83
Angular distance between the image centers 0.0528 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.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: 01:42:56.263 +61:59:01.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:56.263 +61:59:01.09
Angular distance between the image centers 0.0540 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 01:42:55.038 +61:58:24.83
Second-epoch second image center 01:42:56.263 +61:59:01.09
Angular distance between the image centers 0.01035 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.5wB8jJP04a
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.xrg3pexYqo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits &> /tmp/tmp.HHvAlyYc7S
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits &> /tmp/tmp.lkGon99UgI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat' -> 'wcsmag.cat'
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 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 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 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): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.035150
a=0.000000 b=1.000000 c=20.035150
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 12.76
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 12.76
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 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 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 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): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=4.4)
Read 218998 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9707 to 45.8168 deg, Dec +55.3262 to +67.4140 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 6.9707 to 45.8168 deg, Dec 55.3262 to 67.4140 deg
Loaded 26295 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): 10859 out of 16691 total matches.
Matched with Tycho-2 16691 out of 218998 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 109 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.0 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.1 pix fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
2.1 pix fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
2.0 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.0 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
12.8 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
12.7 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
11.0 mag. fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
11.0 mag. fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
All-image limiting magnitude estimate: 11.0 (SNR ) 10.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5wB8jJP04a (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/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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=34, blended=35398, bad_region=42270, passed=222522
Got 222522 stars (including 150930 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
util/solve_plate_with_UCAC5 got 222522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 285 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 185 matched stars entering correct_measured_positions(), 120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 176 matched stars entering correct_measured_positions(), 35458 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.87"
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 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 352 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 272 matched stars entering correct_measured_positions(), 35503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.85"
Accuracy estimation diagnostic: 260 matched stars entering correct_measured_positions(), 43928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.93"
Excluding outliers - 260 stars left (next iteration limit 193)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=260 sigma_overall_arcsec=16.759 sigma_q1_arcsec=27.822 sigma_q2_arcsec=16.292 sigma_q3_arcsec=29.616 sigma_q4_arcsec=15.932 n_q1=22 n_q2=122 n_q3=34 n_q4=82 worst_quadrant_to_overall_ratio=1.767
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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.xrg3pexYqo (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/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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=24, blended=35098, bad_region=41592, passed=218974
Got 218974 stars (including 148361 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat
util/solve_plate_with_UCAC5 got 218974 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 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 178822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 178823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 178820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=978 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.369 sigma_q2_arcsec=0.317 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.279 n_q1=197 n_q2=181 n_q3=381 n_q4=219 worst_quadrant_to_overall_ratio=1.028
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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.HHvAlyYc7S (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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=4173, bad_region=9332, passed=69674
Got 69674 stars (including 56618 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat
util/solve_plate_with_UCAC5 got 69674 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 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 61179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 61179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 61179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits N_match=970 sigma_overall_arcsec=0.540 sigma_q1_arcsec=0.541 sigma_q2_arcsec=0.453 sigma_q3_arcsec=0.738 sigma_q4_arcsec=0.545 n_q1=335 n_q2=267 n_q3=246 n_q4=122 worst_quadrant_to_overall_ratio=1.367
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.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.lkGon99UgI (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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.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=1, no_mag_err=0, low_SNR=11, blended=4128, bad_region=9356, passed=69190
Got 69190 stars (including 56151 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat
util/solve_plate_with_UCAC5 got 69190 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 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 61083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 61081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 61081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits N_match=969 sigma_overall_arcsec=0.571 sigma_q1_arcsec=0.588 sigma_q2_arcsec=0.468 sigma_q3_arcsec=0.720 sigma_q4_arcsec=0.573 n_q1=325 n_q2=272 n_q3=242 n_q4=130 worst_quadrant_to_overall_ratio=1.260
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.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_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-36-58_20.00sec_5.00C_LIGHT_0234.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.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_2026-06-28_CI_Cas-03-Q2b1x1_014309_TTUQ2b1x1_3573170_F1JexyBe/wcs_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235.fits
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:41.38 +58:14:18.2: 10.58 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:41.94 +61:54:41.8: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:29.16 +61:08:58.5: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:24.55 +59:57:28.9: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:15.74 +59:14:39.5: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:28.28 +61:07:37.5: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:26.11 +60:54:33.5: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:56.12 +59:46:32.4: 11.10 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:31.93 +57:31:00.7: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:41.38 +58:14:18.2: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:15.74 +59:14:39.5: 13.20 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:24.55 +59:57:28.9: 13.16 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:29.16 +61:08:58.5: 13.29 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:41.94 +61:54:41.8: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.02
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Forced photometry filter KEPT candidate at 01:38:41.38 +58:14:18.2: ref_mag=11.77 +/- 0.02 new_mean_mag=10.5300 delta=1.24 (need > 0.90)
Forced photometry filter KEPT candidate at 01:41:24.55 +59:57:28.9: ref_mag=13.16 +/- 0.03 new_mean_mag=10.5740 delta=2.59 (need > 0.90)
Forced photometry filter KEPT candidate at 01:49:15.74 +59:14:39.5: ref_mag=13.20 +/- 0.02 new_mean_mag=10.7137 delta=2.48 (need > 0.90)
Forced photometry filter KEPT candidate at 01:29:41.94 +61:54:41.8: ref_mag=13.44 +/- 0.03 new_mean_mag=10.7365 delta=2.71 (need > 0.90)
Forced photometry filter KEPT candidate at 01:47:29.16 +61:08:58.5: ref_mag=13.29 +/- 0.03 new_mean_mag=10.6736 delta=2.62 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:56.12 +59:46:32.4: 12.83 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:28.28 +61:07:37.5: 13.25 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:26.11 +60:54:33.5: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry filter KEPT candidate at 01:22:28.28 +61:07:37.5: ref_mag=13.25 +/- 0.02 new_mean_mag=10.3903 delta=2.86 (need > 0.90)
Forced photometry filter KEPT candidate at 02:00:56.12 +59:46:32.4: ref_mag=12.65 +/- 0.02 new_mean_mag=10.2743 delta=2.38 (need > 0.90)
Forced photometry filter KEPT candidate at 01:41:26.11 +60:54:33.5: ref_mag=12.88 +/- 0.02 new_mean_mag=10.1993 delta=2.68 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:31.93 +57:31:00.7: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 01:11:31.93 +57:31:00.7: ref_mag=13.00 +/- 0.02 new_mean_mag=10.2061 delta=2.79 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:48.96 +60:05:00.3: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:48.96 +60:05:00.3: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Forced photometry filter KEPT candidate at 01:08:48.96 +60:05:00.3: ref_mag=12.74 +/- 0.02 new_mean_mag=10.1465 delta=2.59 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:34.94 +59:18:10.4: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:34.94 +59:18:10.4: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Forced photometry filter KEPT candidate at 01:45:34.94 +59:18:10.4: ref_mag=12.64 +/- 0.02 new_mean_mag=9.9448 delta=2.70 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:24.94 +60:39:17.6: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:24.94 +60:39:17.6: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Forced photometry filter KEPT candidate at 01:35:24.94 +60:39:17.6: ref_mag=12.70 +/- 0.02 new_mean_mag=9.8754 delta=2.82 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:31.52 +58:41:49.0: 12.17 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:31.52 +58:41:49.0: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter KEPT candidate at 01:23:31.52 +58:41:49.0: ref_mag=12.55 +/- 0.01 new_mean_mag=9.7886 delta=2.76 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:51.20 +59:35:50.3: 12.60 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:51.20 +59:35:50.3: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry filter KEPT candidate at 01:48:51.20 +59:35:50.3: ref_mag=11.93 +/- 0.01 new_mean_mag=9.3099 delta=2.62 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:35.37 +60:03:33.4: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:35.37 +60:03:33.4: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Forced photometry filter KEPT candidate at 01:19:35.37 +60:03:33.4: ref_mag=11.02 +/- 0.00 new_mean_mag=8.4302 delta=2.59 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:24.29 +60:39:45.6: 10.72 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:24.29 +60:39:45.6: 11.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.18 +/- 0.03
Forced photometry filter KEPT candidate at 01:33:24.29 +60:39:45.6: ref_mag=11.18 +/- 0.03 new_mean_mag=8.3263 delta=2.85 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:02.35 +61:13:14.6: 11.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:02.35 +61:13:14.6: 11.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.02
Forced photometry filter KEPT candidate at 01:46:02.35 +61:13:14.6: ref_mag=11.59 +/- 0.02 new_mean_mag=8.7767 delta=2.81 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:56.92 +63:37:30.6: 10.68 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:56.92 +63:37:30.6: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.02
Forced photometry filter KEPT candidate at 01:07:56.92 +63:37:30.6: ref_mag=12.31 +/- 0.02 new_mean_mag=10.2118 delta=2.09 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:04.43 +58:53:28.0: 13.13 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:29.74 +61:47:05.0: 10.23 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:04.43 +58:53:28.0: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry filter KEPT candidate at 01:57:04.43 +58:53:28.0: ref_mag=12.81 +/- 0.02 new_mean_mag=10.1653 delta=2.64 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:29.74 +61:47:05.0: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.02
Forced photometry filter KEPT candidate at 01:09:29.74 +61:47:05.0: ref_mag=11.43 +/- 0.02 new_mean_mag=10.3727 delta=1.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:36.53 +61:11:12.5: 9.88 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:42.47 +60:04:29.3: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:36.53 +61:11:12.5: 13.54 +/- 0.10 detection
Forced photometry reference-image weighted average: 10.01 +/- 0.02
Forced photometry filter REJECTED candidate at 01:46:36.53 +61:11:12.5: ref_mag=10.01 +/- 0.02 new_mean_mag=10.6013 delta=-0.59 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:42.47 +60:04:29.3: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Forced photometry filter KEPT candidate at 02:02:42.47 +60:04:29.3: ref_mag=13.44 +/- 0.04 new_mean_mag=10.6721 delta=2.77 (need > 0.90)
Adding exclusion_list_local.txt__out247630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out261005.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 38s
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: 14s
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Considering the candidate 247630_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247630_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247633_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247633_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247642_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247642_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247651_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247651_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247653_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247653_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:07:34.93 +57:33:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247659_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247659_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247667_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247667_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:10:37.51 +57:22:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247668_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247668_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 02:01:30.75 +65:05:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247674_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247674_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 247677_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247677_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:14:45.30 +60:30:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247678_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247678_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:40:31.46 +60:31:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247679_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247679_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247681_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247681_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247685_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247685_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247686_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247686_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247690_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247690_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:39:04.28 +61:53:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247691_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247691_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:42:49.54 +60:21:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247697_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247697_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247698_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247698_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:07:07.96 +57:44:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247699_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247699_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:43:51.69 +61:54:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247704_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247704_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247706_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247706_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:55:14.60 +59:32:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247707_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247707_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:15:16.88 +57:28:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247708_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247708_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247710_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247710_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:34:26.90 +60:30:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247711_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247711_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247712_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247712_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:15:55.92 +58:23:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247713_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247713_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:43:59.15 +61:55:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247714_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247714_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:16:20.59 +62:42:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247717_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247717_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:20:24.36 +59:10:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247721_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247721_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247722_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247722_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:19:48.74 +61:38:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247727_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247727_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:25:56.64 +59:35:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247729_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247729_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:44:58.40 +57:57:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247731_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247731_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 02:13:07.15 +58:04:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247732_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247732_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:16:01.00 +62:41:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247734_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 247734_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 247736_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 247736_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:47:13.10 +57:44:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249424_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 249424_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 250070_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 250070_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:46:19.57 +61:15:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250258_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 250258_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
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Considering the candidate 251377_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 251377_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:46:08.61 +61:12:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251455_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 251455_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:44:02.34 +61:53:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252018_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 252018_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:19:11.12 +58:20:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252088_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 252088_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:38:00.45 +57:56:45.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252354_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 252354_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:33:20.56 +60:37:47.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252805_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 252805_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:17:59.09 +57:47:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252995_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 252995_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:46:30.15 +61:13:00.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253417_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 253417_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:40:01.55 +60:52:32.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253476_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 253476_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:38:05.56 +58:00:20.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253767_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 253767_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:28:15.33 +58:44:13.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253848_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 253848_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:24:27.42 +58:44:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253996_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 253996_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:26:46.65 +57:46:54.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254432_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 254432_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:25:31.76 +57:37:39.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254981_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 254981_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:42:49.31 +61:25:57.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255054_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 255054_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:26:41.12 +60:46:47.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255153_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 255153_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:58:16.27 +59:39:00.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255273_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 255273_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 02:05:03.48 +64:21:52.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255593_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 255593_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:45:49.72 +57:50:10.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255798_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 255798_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:08:42.34 +58:17:00.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256053_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 256053_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:29:32.70 +61:46:27.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256195_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 256195_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:16:08.51 +58:49:39.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256463_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 256463_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:18:14.19 +61:44:37.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256743_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 256743_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:33:59.34 +58:28:33.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256791_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 256791_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:59:37.38 +62:54:30.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257011_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 257011_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:44:17.72 +61:53:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257024_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 257024_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:43:53.24 +61:53:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257119_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 257119_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257180_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 257180_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:21:28.01 +57:48:03.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257211_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 257211_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:18:19.21 +57:42:24.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257245_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 257245_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:31:37.06 +58:38:07.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257635_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 257635_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:51:02.37 +64:49:52.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257691_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 257691_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 02:00:51.83 +58:31:26.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257798_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 257798_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 02:16:36.19 +64:57:47.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257802_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 257802_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:23:56.10 +60:54:50.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257815_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 257815_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:20:10.98 +58:12:08.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257970_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 257970_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258196_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 258196_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 02:15:58.99 +63:12:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258239_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 258239_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 02:11:23.05 +61:21:06.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258241_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 258241_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:19:22.22 +58:19:19.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258308_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 258308_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258481_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 258481_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:38:33.11 +60:48:02.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258596_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 258596_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:18:39.89 +58:25:51.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258922_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 258922_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:43:03.22 +58:08:04.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259296_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 259296_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:39:56.69 +60:52:15.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259475_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 259475_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:44:32.42 +58:45:36.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259817_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 259817_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 02:00:36.76 +58:30:22.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259824_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 259824_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:33:32.53 +60:40:05.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260110_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 260110_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:07:40.43 +63:30:15.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260198_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 260198_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:37:44.66 +64:45:52.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260271_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 260271_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:16:05.25 +58:49:40.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260586_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 260586_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 02:04:26.46 +65:05:53.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260761_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 260761_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:35:50.52 +61:27:35.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260862_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 260862_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260902_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 260902_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:44:27.93 +60:41:23.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261005_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
Preparing report for the candidate 261005_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261562_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 261562_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:47:19.27 +63:38:11.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261643_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 261643_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 02:02:54.11 +60:15:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261912_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 261912_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:38:33.87 +60:47:23.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262166_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 262166_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:41:51.01 +61:02:08.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262331_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 262331_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:55:53.09 +64:15:24.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262475_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 262475_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:42:28.25 +58:17:49.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263229_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 263229_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:58:04.82 +59:36:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263330_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 263330_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:39:24.06 +58:23:06.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263683_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 263683_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:38:12.07 +61:01:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 70271_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 02:20:32.49 +62:32:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 72532_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:45:35.71 +63:07:05.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156692_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 156692_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:56:38.08 +59:15:34.0 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235
The candidate 39378_fd_Cas-03-Q2b1x1_2026-06-28_01-37-51_20.00sec_4.90C_LIGHT_0235 did not pass the final checks
**** FOUND 01:47:55.75 +64:32:55.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 54s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:56:38.07 +59:15:33.8
01:29:41.94 +61:54:41.8
01:47:29.16 +61:08:58.5
01:38:41.38 +58:14:18.2
01:49:15.74 +59:14:39.5
01:41:24.55 +59:57:28.9
01:41:26.11 +60:54:33.5
01:22:28.28 +61:07:37.5
01:11:31.93 +57:31:00.7
02:00:56.12 +59:46:32.4
01:08:48.96 +60:05:00.3
01:45:34.94 +59:18:10.4
01:35:24.94 +60:39:17.6
01:23:31.52 +58:41:49.0
01:48:51.20 +59:35:50.3
01:19:35.37 +60:03:33.4
01:33:24.29 +60:39:45.6
01:46:02.35 +61:13:14.6
01:07:56.92 +63:37:30.6
01:57:04.43 +58:53:28.0
01:09:29.74 +61:47:05.0
02:02:42.47 +60:04:29.3
########### Completed Cas-03-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 ####
01:56:38.07 +59:15:33.8
01:29:41.94 +61:54:41.8
01:47:29.16 +61:08:58.5
01:38:41.38 +58:14:18.2
01:49:15.74 +59:14:39.5
01:41:24.55 +59:57:28.9
01:41:26.11 +60:54:33.5
01:22:28.28 +61:07:37.5
01:11:31.93 +57:31:00.7
02:00:56.12 +59:46:32.4
01:08:48.96 +60:05:00.3
01:45:34.94 +59:18:10.4
01:35:24.94 +60:39:17.6
01:23:31.52 +58:41:49.0
01:48:51.20 +59:35:50.3
01:19:35.37 +60:03:33.4
01:33:24.29 +60:39:45.6
01:46:02.35 +61:13:14.6
01:07:56.92 +63:37:30.6
01:57:04.43 +58:53:28.0
01:09:29.74 +61:47:05.0
02:02:42.47 +60:04:29.3
###################################################################################
01:56:38.07 +59:15:33.8 -- not an asteroid (will add it to exclusion list)
01:29:41.94 +61:54:41.8 -- not an asteroid (will add it to exclusion list)
01:47:29.16 +61:08:58.5 -- not an asteroid (will add it to exclusion list)
01:38:41.38 +58:14:18.2 -- not an asteroid (will add it to exclusion list)
01:49:15.74 +59:14:39.5 -- not an asteroid (will add it to exclusion list)
01:41:24.55 +59:57:28.9 -- not an asteroid (will add it to exclusion list)
01:41:26.11 +60:54:33.5 -- not an asteroid (will add it to exclusion list)
01:22:28.28 +61:07:37.5 -- not an asteroid (will add it to exclusion list)
01:11:31.93 +57:31:00.7 -- not an asteroid (will add it to exclusion list)
02:00:56.12 +59:46:32.4 -- not an asteroid (will add it to exclusion list)
01:08:48.96 +60:05:00.3 -- not an asteroid (will add it to exclusion list)
01:45:34.94 +59:18:10.4 -- not an asteroid (will add it to exclusion list)
01:35:24.94 +60:39:17.6 -- not an asteroid (will add it to exclusion list)
01:23:31.52 +58:41:49.0 -- not an asteroid (will add it to exclusion list)
01:48:51.20 +59:35:50.3 -- not an asteroid (will add it to exclusion list)
01:19:35.37 +60:03:33.4 -- not an asteroid (will add it to exclusion list)
01:33:24.29 +60:39:45.6 -- not an asteroid (will add it to exclusion list)
01:46:02.35 +61:13:14.6 -- not an asteroid (will add it to exclusion list)
01:07:56.92 +63:37:30.6 -- not an asteroid (will add it to exclusion list)
01:57:04.43 +58:53:28.0 -- not an asteroid (will add it to exclusion list)
01:09:29.74 +61:47:05.0 -- not an asteroid (will add it to exclusion list)
02:02:42.47 +60:04:29.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:07:56.92 +63:37:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:48.96 +60:05:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:29.74 +61:47:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:31.93 +57:31:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:35.37 +60:03:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:28.28 +61:07:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:31.52 +58:41:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:41.94 +61:54:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:24.29 +60:39:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:24.94 +60:39:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:41.38 +58:14:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:24.55 +59:57:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:26.11 +60:54:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:34.94 +59:18:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:02.35 +61:13:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:29.16 +61:08:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:51.20 +59:35:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:15.74 +59:14:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:38.07 +59:15:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:04.43 +58:53:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:56.12 +59:46:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:42.47 +60:04:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:07:56.92 +63:37:30.6 -- a known variable star
01:08:48.96 +60:05:00.3 -- not a known variable star
01:09:29.74 +61:47:05.0 -- a known variable star
01:11:31.93 +57:31:00.7 -- not a known variable star
01:19:35.37 +60:03:33.4 -- not a known variable star
01:22:28.28 +61:07:37.5 -- a known variable star
01:23:31.52 +58:41:49.0 -- a known variable star
01:29:41.94 +61:54:41.8 -- not a known variable star
01:33:24.29 +60:39:45.6 -- a known variable star
01:35:24.94 +60:39:17.6 -- a known variable star
01:38:41.38 +58:14:18.2 -- not a known variable star
01:41:24.55 +59:57:28.9 -- a known variable star
01:41:26.11 +60:54:33.5 -- a known variable star
01:45:34.94 +59:18:10.4 -- not a known variable star
01:46:02.35 +61:13:14.6 -- not a known variable star
01:47:29.16 +61:08:58.5 -- not a known variable star
01:48:51.20 +59:35:50.3 -- not a known variable star
01:49:15.74 +59:14:39.5 -- not a known variable star
01:56:38.07 +59:15:33.8 -- a known variable star
01:57:04.43 +58:53:28.0 -- not a known variable star
02:00:56.12 +59:46:32.4 -- not a known variable star
02:02:42.47 +60:04:29.3 -- not a known variable star
Found 13 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
22 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 ####
01:07:56.92 +63:37:30.6
01:08:48.96 +60:05:00.3
01:09:29.74 +61:47:05.0
01:11:31.93 +57:31:00.7
01:19:35.37 +60:03:33.4
01:22:28.28 +61:07:37.5
01:23:31.52 +58:41:49.0
01:29:41.94 +61:54:41.8
01:33:24.29 +60:39:45.6
01:35:24.94 +60:39:17.6
01:38:41.38 +58:14:18.2
01:41:24.55 +59:57:28.9
01:41:26.11 +60:54:33.5
01:45:34.94 +59:18:10.4
01:46:02.35 +61:13:14.6
01:47:29.16 +61:08:58.5
01:48:51.20 +59:35:50.3
01:49:15.74 +59:14:39.5
01:56:38.07 +59:15:33.8
01:57:04.43 +58:53:28.0
02:00:56.12 +59:46:32.4
02:02:42.47 +60:04:29.3
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461219.77579468 -observatory V36
07:49:44.59 +19:13:34.3 Mercury (1.7mag)
09:19:02.44 +17:35:12.1 Venus (-4.0mag)
03:48:26.70 +19:39:37.6 Mars (1.3mag)
08:05:48.34 +20:44:23.5 Jupiter (-1.8mag)
00:54:05.11 +03:12:58.1 Saturn (0.8mag)
04:04:46.64 +20:38:20.7 Uranus (5.8mag)
00:16:55.99 +00:20:47.4 Neptune (7.8mag)
20:31:57.92 -23:12:43.5 Pluto (14.5mag)
17:02:18.34 -28:27:35.7 Moon (-12.2mag)
-rw-r--r-- 1 apache apache 362 Jun 28 03:35 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461219.77579468:
08:05:55.16 +20:43:59.8 Io (6.1mag)
08:05:41.89 +20:44:45.5 Europa (6.3mag)
08:05:46.59 +20:44:25.6 Ganymede (5.6mag)
08:05:33.40 +20:45:09.7 Callisto (6.9mag)
08:04:56.32 +20:24:17.9 Himalia (15.7mag)
08:05:49.67 +20:44:19.7 Thebe (16.6mag)
08:04:25.84 +20:32:03.3 Elara (17.6mag)
08:08:54.60 +20:45:06.3 Pasiphae (17.8mag)
08:11:25.63 +20:47:56.9 Carme (18.9mag)
00:54:11.64 +03:12:31.4 Titan (8.6mag)
00:54:07.69 +03:12:46.1 Rhea (9.9mag)
00:53:59.32 +03:14:25.3 Iapetus (11.3mag)
00:53:55.99 +03:12:39.2 Hyperion (14.6mag)
00:54:21.84 +03:11:58.4 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jun 28 03:35 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461219.77579468:
17:33:46.23 -34:55:56.1 JWST
18:33:45.05 +24:15:24.1 Chandra
20:38:29.70 +36:03:44.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 28 03:35 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461219.77579468 -observatory V36
02:18:33.89 +12:53:39.5 18.0mag P/1996 R2 (Lagerkvist)
18:27:45.75 -33:53:48.0 13.7mag P/2010 H2 (Vales)
06:13:31.85 -68:00:50.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:56:28.80 +32:15:08.9 17.6mag C/2017 K2 (PANSTARRS)
17:07:00.06 +15:59:44.4 17.9mag C/2021 G2 (ATLAS)
00:25:59.46 -18:26:31.2 15.5mag P/2021 N1 (ZTF)
23:05:51.95 +32:10:34.2 17.2mag C/2022 E2 (ATLAS)
05:58:19.20 +26:59:56.7 16.6mag C/2022 N2 (PANSTARRS)
09:45:17.07 +30:18:16.8 16.8mag C/2022 QE78 (ATLAS)
09:02:08.20 +04:42:14.5 17.8mag C/2022 R6 (PANSTARRS)
18:14:54.85 +21:37:25.2 17.9mag C/2023 A3 (Tsuchinshan-ATLAS)
15:13:31.38 -11:09:55.7 17.7mag P/2023 B1 (PANSTARRS)
22:01:58.72 +67:28:09.4 17.8mag C/2023 H5 (Lemmon)
16:57:06.44 -08:47:23.4 13.8mag C/2023 R1 (PANSTARRS)
13:21:20.83 +78:12:02.1 18.0mag C/2023 X2 (Lemmon)
07:40:31.69 +65:06:32.3 17.8mag C/2024 A1 (ATLAS)
07:16:28.83 +29:19:37.3 14.3mag C/2024 E1 (Wierzchos)
15:23:02.48 +14:52:41.0 17.5mag C/2024 G6 (ATLAS)
19:55:30.78 +36:41:12.4 13.8mag C/2024 J3 (ATLAS)
21:58:23.93 +44:01:46.8 17.9mag C/2024 R4 (PANSTARRS)
04:37:59.65 -14:26:54.0 15.8mag C/2024 T5 (ATLAS)
06:24:12.53 +31:04:53.9 18.0mag C/2025 J1 (Borisov)
07:05:02.16 -11:57:34.5 15.7mag C/2025 R3 (PANSTARRS)
09:42:51.22 +22:53:05.4 17.8mag C/2025 V2 (Rankin)
12:41:26.38 +04:21:55.4 17.1mag C/2025 Y1 (ATLAS)
17:27:15.23 +78:22:35.6 17.6mag C/2026 A2 (Bok)
02:31:39.39 +44:39:20.0 16.5mag C/2026 B2 (Sun-Gao)
11:18:37.90 +02:04:03.3 16.8mag A/2026 E1
20:59:07.28 -11:31:52.4 7.7mag 10P/Tempel
11:08:17.84 -01:26:13.8 16.1mag 29P/Schwassmann-Wachmann
03:42:22.56 +28:10:43.4 17.8mag 47P/Ashbrook-Jackson
09:42:41.08 +17:47:46.5 17.0mag 63P/Wild
00:41:53.96 -05:22:29.9 15.6mag 65P/Gunn
07:48:35.42 +34:28:33.0 17.5mag 76P/West-Kohoutek-Ikemura
03:58:01.23 +19:20:58.2 13.7mag 78P/Gehrels
02:01:15.41 +08:44:27.3 16.0mag 88P/Howell
05:58:35.62 +30:56:40.9 15.5mag 93P/Lovas
03:42:37.36 +30:15:25.1 17.1mag 114P/Wiseman-Skiff
07:39:08.87 +31:51:32.4 15.4mag 123P/West-Hartley
10:25:55.06 +06:09:32.1 16.7mag 124P/Mrkos
04:32:06.31 +20:22:04.6 16.3mag 128P/Shoemaker-Holt
05:13:05.92 +19:40:34.2 17.8mag 131P/Mueller
07:16:05.77 +15:33:08.8 17.1mag 141P/Machholz
07:15:27.01 +15:36:38.6 17.1mag 141P-A/Machholz
06:25:21.61 +19:22:40.9 14.0mag 141P-D/Machholz
03:10:42.03 -22:15:06.5 16.0mag 161P/Hartley-IRAS
04:50:00.25 +30:50:25.7 15.1mag 162P/SidingSpring
19:25:31.75 +08:53:42.2 15.6mag 169P/NEAT
01:11:06.55 +05:59:09.6 17.7mag 220P/McNaught
16:39:34.34 -08:05:29.3 16.8mag 235P/LINEAR
08:19:20.63 +34:18:27.0 17.8mag 240P/NEAT
20:44:01.50 -46:33:45.8 17.9mag 259P/Garradd
01:25:58.90 +06:28:01.0 15.9mag 260P/McNaught
05:01:07.76 +35:35:11.9 17.4mag 295P/LINEAR
15:08:20.35 +07:01:24.9 17.5mag 391P/Kowalski
08:23:55.53 +20:07:59.0 17.9mag 450P/LONEOS
07:32:33.14 +40:11:31.3 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Jun 28 03:35 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
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
15:03:05.18 +22:02:03.40 AT2026lxf 2026-05-8.07 13.94
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
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
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
14:47:21.56 -40:15:51.30 2026-06-23.03 14.62
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
14:47:21.56 -40:15:51.30 2026-06-23.03 14.62
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
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
-rw-r--r-- 1 apache apache 5.6K Jun 28 03:35 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 Jun 28 03:35 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:54:11.879 +44:04:32.53 AT 2026pwp 2026-06-21.90 19.972
11:51:13.242 +46:13:17.21 AT 2026pwo 2026-06-15.28 19.447
17:21:30.031 +58:03:12.13 AT 2026pwn 2026-06-21.48 18.862
11:47:04.003 +73:27:42.99 AT 2026pwm 2026-06-21.90 19.015
13:30:13.578 +62:30:34.06 SN 2026pwl 2026-06-21.97 19.359
17:43:17.310 +64:32:16.40 AT 2026pwk 2026-06-09.43 20.8004
17:29:11.285 +73:29:30.02 AT 2026pwj 2026-06-14.20 20.4641
11:43:37.251 -11:20:23.59 AT 2026pwi 2026-06-13.89 19.358
20:53:50.297 +14:31:52.13 AT 2026pwh 2026-06-21.09 19.201
18:33:16.188 +62:56:34.08 AT 2026pwg 2026-06-21.51 19.203
19:50:18.283 -16:34:54.78 AT 2026pwf 2026-06-14.40 20.7828
14:04:46.460 +33:05:14.33 AT 2026pwe 2026-06-16.20 20.0234
09:09:55.625 +23:29:33.75 AT 2026pwd 2026-06-16.17 19.333
13:11:20.569 +79:19:36.02 AT 2026pwc 2026-06-06.30 20.2375
14:25:15.992 +45:05:38.69 AT 2026pwb 2026-06-11.20 20.9128
13:20:25.454 +58:33:31.90 AT 2026pwa 2026-06-18.30 20.0089
13:43:58.451 +39:20:16.74 AT 2026pvz 2026-06-17.20 20.6601
14:09:02.575 +39:37:43.12 AT 2026pvy 2026-06-15.27 20.8145
16:35:02.714 +51:28:05.49 AT 2026pvx 2026-06-21.91 20.13
19:09:47.096 +13:24:41.21 AT 2026pvw 2026-06-14.39 17.01
-rw-r--r-- 1 apache apache 30K Jun 28 03:35 tns_transients_list.txt
