This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW
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 05 13.4012 2461173.9012 11.55 01:31:14.40 +63:03:09.2
127.42338 0.52843 galactic Cas Second-epoch detections are separated by 2.3" and 6.6 pix
The object was found in VSX14" ZTF J013116.29+630314.8
Type: SR
# Max. Min./Amp. JD0 Period
16.849 g Y 0.408 g 2458522.39160 115.864605900000
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 01:31:14.40 +63:03:09.2: 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 01:31:14.40 +63:03:09.2: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 31 14.40 +63 03 09.2 11.6 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
ZTF J013116.29+630314.8,2461173.9012,11.55,0.05,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 J013116.29+630314.8 20260513.4012 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.18 01:22:33.33 +60:44:40.2
126.72693 -1.89776 galactic Cas Second-epoch detections are separated by 0.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:22:33.33 +60:44:40.2 (user input) | T | P | (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 01:22:33.33 +60:44:40.2: 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 01:22:33.33 +60:44:40.2: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 22 33.33 +60 44 40.2 11.2 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,2461173.9012,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260513.4012 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.06 02:16:03.16 +63:19:18.9
132.26194 1.99329 galactic Cas Second-epoch detections are separated by 4.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:16:03.16 +63:19:18.9 (user input) | T | P | (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 02:16:03.16 +63:19:18.9: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:03.16 +63:19:18.9: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 02 16 03.16 +63 19 18.9 11.1 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,2461173.9012,11.06,0.05,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 20260513.4012 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.86 02:03:44.67 +60:07:55.1
131.82419 -1.48548 galactic Cas Second-epoch detections are separated by 2.1" and 5.8 pix
The object was found in VSX10" Gaia DR3 507934759549565824
Type: E
# Max. Min./Amp. JD0 Period
18.000 G 18.600 G 0.426651000000
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 02:03:44.67 +60:07:55.1: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:44.67 +60:07:55.1: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 02 03 44.67 +60 07 55.1 10.9 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 507934759549565824,2461173.9012,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507934759549565824 20260513.4012 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.04 01:28:35.57 +62:13:54.9
127.24469 -0.32831 galactic Cas Second-epoch detections are separated by 2.2" 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 | target | 01:28:35.57 +62:13:54.9 (user input) | T | P | (position from user input) J-Ks=1.068+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:35.57 +62:13:54.9: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:35.57 +62:13:54.9: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 28 35.57 +62 13 54.9 11.0 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,2461173.9012,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260513.4012 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.28 01:12:01.08 +64:42:19.2
125.12907 1.92142 galactic Cas Second-epoch detections are separated by 2.7" and 5.9 pix
The object was found in VSX 2" ZTF J011201.03+644221.2
Type: RS
# Max. Min./Amp. JD0 Period
14.762 g Y 0.263 g 2458343.85900 3.018403700000
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 01:12:01.08 +64:42:19.2: 11.76 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:01.08 +64:42:19.2: 13.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 12 01.08 +64 42 19.2 11.3 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 J011201.03+644221.2,2461173.9012,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011201.03+644221.2 20260513.4012 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.04 01:52:14.57 +60:44:05.1
130.29828 -1.26440 galactic Cas Second-epoch detections are separated by 4.5" and 5.4 pix
The object was found in VSX12" Gaia DR3 508175277731318912
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.950 G 13.990 G 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 01:52:14.57 +60:44:05.1: 12.43 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:14.57 +60:44:05.1: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 52 14.57 +60 44 05.1 11.0 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 508175277731318912,2461173.9012,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508175277731318912 20260513.4012 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.05 01:04:37.02 +62:52:12.1
124.43371 0.03671 galactic Cas Second-epoch detections are separated by 3.5" and 6.0 pix
The object was not found in VSX
The object was found in ASASSN-V17" ASASSN-V J010437.17+625229.1
Type: ROT:
MeanMag 13.26 m Amp. 0.06 m Period d
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 01:04:37.02 +62:52:12.1: 11.35 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:04:37.02 +62:52:12.1: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 05 13.4012* 01 04 37.02 +62 52 12.1 11.1 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
VARIABLE_NAME,2461173.9012,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260513.4012 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.02 01:33:19.94 +62:33:19.0
127.73792 0.07510 galactic Cas Second-epoch detections are separated by 0.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512315037781955200 | 01:33:17.17 +62:33:11.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.228+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:19.94 +62:33:19.0: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:19.94 +62:33:19.0: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 33 19.94 +62 33 19.0 11.0 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 512315037781955200,2461173.9012,11.02,0.05,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 512315037781955200 20260513.4012 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.81 01:33:32.02 +60:52:20.1
128.03446 -1.58177 galactic Cas Second-epoch detections are separated by 1.9" and 6.1 pix
The object was found in VSX16" Gaia DR3 509883678286141056
Type: ROT
# Max. Min./Amp. JD0 Period
13.560 G 13.590 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 01:33:32.02 +60:52:20.1: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:32.02 +60:52:20.1: 13.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 33 32.02 +60 52 20.1 10.8 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 509883678286141056,2461173.9012,10.81,0.05,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 509883678286141056 20260513.4012 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.03 01:06:17.37 +57:53:08.9
124.91206 -4.92883 galactic Cas Second-epoch detections are separated by 0.6" 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 | ATO J016.5720+57.8855 | 01:06:17.37 +57:53:08.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.082+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:17.37 +57:53:08.9: 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 01:06:17.37 +57:53:08.9: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 06 17.37 +57 53 08.9 11.0 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 J016.5720+57.8855,2461173.9012,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J016.5720+57.8855 20260513.4012 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.98 01:09:25.30 +64:35:18.7
124.86052 1.78414 galactic Cas Second-epoch detections are separated by 3.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:09:25.30 +64:35:18.7 (user input) | T | P | (position from user input) J-Ks=0.557+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:25.30 +64:35:18.7: 12.52 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:25.30 +64:35:18.7: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 09 25.30 +64 35 18.7 11.0 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,2461173.9012,10.98,0.05,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 20260513.4012 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.01 01:07:39.26 +59:59:17.8
124.96088 -2.81957 galactic Cas Second-epoch detections are separated by 0.4" 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 | target | 01:07:39.26 +59:59:17.8 (user input) | T | P | (position from user input) J-Ks=0.895+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.26 +59:59:17.8: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.26 +59:59:17.8: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 07 39.26 +59 59 17.8 11.0 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,2461173.9012,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260513.4012 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.88 01:30:26.87 +58:02:20.9
128.09185 -4.44125 galactic Cas Second-epoch detections are separated by 1.5" 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 | target | 01:30:26.87 +58:02:20.9 (user input) | T | P | (position from user input) J-Ks=0.196+/-0.037 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:26.87 +58:02:20.9: 12.76 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:26.87 +58:02:20.9: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 30 26.87 +58 02 20.9 10.9 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
target,2461173.9012,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260513.4012 10.88CV 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 05 13.4012 2461173.9012 10.86 01:26:05.70 +59:01:14.2
127.38773 -3.55098 galactic Cas Second-epoch detections are separated by 1.2" 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 | ATO J021.5231+59.0209 | 01:26:05.70 +59:01:14.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.314+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.70 +59:01:14.2: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.70 +59:01:14.2: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 26 05.70 +59 01 14.2 10.9 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 J021.5231+59.0209,2461173.9012,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.5231+59.0209 20260513.4012 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.97 01:08:25.67 +59:48:03.0
125.06990 -3.00037 galactic Cas Second-epoch detections are separated by 0.7" 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 | target | 01:08:25.67 +59:48:03.0 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:25.67 +59:48:03.0: 12.63 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:25.67 +59:48:03.0: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 08 25.67 +59 48 03.0 11.0 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,2461173.9012,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260513.4012 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.01 01:10:43.96 +60:59:18.8
125.27036 -1.79556 galactic Cas Second-epoch detections are separated by 2.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:10:43.96 +60:59:18.8 (user input) | T | P | (position from user input) J-Ks=0.354+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:43.96 +60:59:18.8: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:43.96 +60:59:18.8: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 10 43.96 +60 59 18.8 11.0 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,2461173.9012,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260513.4012 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.57 01:56:43.25 +58:07:17.2
131.48426 -3.66217 galactic Cas Second-epoch detections are separated by 0.4" 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 | target | 01:56:43.25 +58:07:17.2 (user input) | T | P | (position from user input) J-Ks=0.952+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:43.25 +58:07:17.2: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:43.25 +58:07:17.2: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 56 43.25 +58 07 17.2 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
target,2461173.9012,10.57,0.05,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
target 20260513.4012 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 05 13.4012 2461173.9012 10.72 01:13:07.66 +58:55:54.6
125.73338 -3.82189 galactic Cas Second-epoch detections are separated by 0.9" and 6.1 pix
The object was found in VSX 1" Gaia DR3 414108381479338368
Type: VAR
# Max. Min./Amp. JD0 Period
13.530 G 13.560 G 0.456759000000 B
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 01:13:07.66 +58:55:54.6: 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 01:13:07.66 +58:55:54.6: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 13 07.66 +58 55 54.6 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 414108381479338368,2461173.9012,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 414108381479338368 20260513.4012 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.68 01:26:39.14 +59:41:39.5
127.36687 -2.87387 galactic Cas Second-epoch detections are separated by 0.4" and 6.2 pix
The object was found in VSX 3" Gaia DR3 510083239641442688
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.660 G 13.680 G B
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 01:26:39.14 +59:41:39.5: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:39.14 +59:41:39.5: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 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 05 13.4012* 01 26 39.14 +59 41 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 510083239641442688,2461173.9012,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510083239641442688 20260513.4012 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.58 02:00:46.85 +57:53:48.5
132.06296 -3.74035 galactic Per Second-epoch detections are separated by 2.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J030.1940+57.8929 | 02:00:46.85 +57:53:48.5 (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 02:00:46.85 +57:53:48.5: 13.06 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:46.85 +57:53:48.5: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 05 13.4012* 02 00 46.85 +57 53 48.5 10.6 U Per 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 J030.1940+57.8929,2461173.9012,10.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J030.1940+57.8929 20260513.4012 10.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.61 01:09:09.23 +61:37:26.9
125.03562 -1.17523 galactic Cas Second-epoch detections are separated by 0.6" and 6.3 pix
The object was found in VSX 2" Gaia DR3 522536136541501952
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.570 G 13.610 G B
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 01:09:09.23 +61:37:26.9: 12.92 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:09.23 +61:37:26.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 05 13.4012* 01 09 09.23 +61 37 26.9 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 522536136541501952,2461173.9012,10.61,0.05,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 522536136541501952 20260513.4012 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 9.64 01:20:24.35 +59:10:24.1
126.64261 -3.48952 galactic Cas Second-epoch detections are separated by 0.8" 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 J020.1204+59.1623 | 01:20:25.01 +59:10:05.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.296+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:24.35 +59:10:24.1: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:24.35 +59:10:24.1: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 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 05 13.4012* 01 20 24.35 +59 10 24.1 9.6 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 J020.1204+59.1623,2461173.9012,9.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J020.1204+59.1623 20260513.4012 9.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 9.28 01:25:56.61 +59:35:11.5
127.29258 -2.99275 galactic Cas Second-epoch detections are separated by 0.3" 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 510075336901717632 | 01:25:55.70 +59:34:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1960IzKry..24..160B [B60] +59 169 J-Ks=0.194+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:56.61 +59:35:11.5: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:56.61 +59:35:11.5: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 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 05 13.4012* 01 25 56.61 +59 35 11.5 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 510075336901717632,2461173.9012,9.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510075336901717632 20260513.4012 9.28CV 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 05 13.4012 2461173.9012 10.04 01:10:34.54 +60:31:05.9
125.28632 -2.26593 galactic Cas Second-epoch detections are separated by 1.2" and 6.2 pix
The object was found in VSX 2" ZTF J011034.65+603107.8
Type: RS
# Max. Min./Amp. JD0 Period
13.515 r Y 0.105 r 2458370.91340 3.097346100000
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 01:10:34.54 +60:31:05.9: 12.47 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:34.54 +60:31:05.9: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 05 13.4012* 01 10 34.54 +60 31 05.9 10.0 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 J011034.65+603107.8,2461173.9012,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011034.65+603107.8 20260513.4012 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.55 01:07:24.47 +60:56:06.9
124.87130 -1.87635 galactic Cas Second-epoch detections are separated by 2.5" and 6.0 pix
The object was found in VSX 2" ZTF J010724.50+605605.2
Type: SR
# Max. Min./Amp. JD0 Period
15.599 g Y 0.213 g 2458370.54470 225.773534500000
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 01:07:24.47 +60:56:06.9: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:24.47 +60:56:06.9: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 07 24.47 +60 56 06.9 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
ZTF J010724.50+605605.2,2461173.9012,10.55,0.05,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 J010724.50+605605.2 20260513.4012 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.46 01:18:36.77 +58:41:37.9
126.46455 -3.99137 galactic Cas Second-epoch detections are separated by 0.7" and 6.1 pix
The object was found in VSX21" Gaia DR3 413902596701682816
Type: ROT
# Max. Min./Amp. JD0 Period
15.180 G 15.220 G 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 01:18:36.77 +58:41:37.9: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:36.77 +58:41:37.9: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 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 05 13.4012* 01 18 36.77 +58 41 37.9 10.5 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 413902596701682816,2461173.9012,10.46,0.05,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 413902596701682816 20260513.4012 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.62 01:24:45.37 +63:08:24.2
126.68490 0.51135 galactic Cas Second-epoch detections are separated by 3.1" 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 | V1319 Cas | 01:24:40.42 +63:08:29.7 (Gaia DR3) | EB (local) | 2.804870000000 (local) | Gaia3var=VARIABLE SpType: OB 1954BOTT....1i..21G [GG54] 14 J-Ks=1.109+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:45.37 +63:08:24.2: 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 01:24:45.37 +63:08:24.2: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 24 45.37 +63 08 24.2 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
V1319 Cas,2461173.9012,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1319 Cas 20260513.4012 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.78 01:10:45.41 +64:05:35.4
125.04059 1.30054 galactic Cas Second-epoch detections are separated by 3.2" 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 523447872192664448 | 01:10:43.44 +64:04:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1960IzKry..24..160B [B60] +63 52
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:45.41 +64:05:35.4: 11.23 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:45.41 +64:05:35.4: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 10 45.41 +64 05 35.4 10.8 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 523447872192664448,2461173.9012,10.78,0.05,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
Gaia DR3 523447872192664448 20260513.4012 10.78CV 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 05 13.4012 2461173.9012 10.91 01:06:55.45 +59:18:56.9
124.91017 -3.49645 galactic Cas Second-epoch detections are separated by 2.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:55.45 +59:18:56.9 (user input) | T | P | (position from user input) J-Ks=0.785+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.45 +59:18:56.9: 13.05 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.45 +59:18:56.9: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 06 55.45 +59 18 56.9 10.9 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
target,2461173.9012,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260513.4012 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.77 01:29:21.50 +61:44:12.7
127.40548 -0.80507 galactic Cas Second-epoch detections are separated by 0.1" 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 | target | 01:29:21.50 +61:44:12.7 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.037 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:21.50 +61:44:12.7: 12.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:21.50 +61:44:12.7: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 29 21.50 +61 44 12.7 10.8 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
target,2461173.9012,10.77,0.05,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 20260513.4012 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.81 01:22:11.10 +59:09:02.5
126.87213 -3.48563 galactic Cas Second-epoch detections are separated by 1.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413976852405588480 | 01:22:13.31 +59:08:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1960IzKry..24..160B [B60] +58 184
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:11.10 +59:09:02.5: 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 01:22:11.10 +59:09:02.5: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 22 11.10 +59 09 02.5 10.8 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 413976852405588480,2461173.9012,10.81,0.05,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 413976852405588480 20260513.4012 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.75 01:51:09.50 +64:52:45.9
129.21840 2.73910 galactic Cas Second-epoch detections are separated by 4.3" and 5.7 pix
The object was found in VSX 3" Gaia DR3 518229967963921664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G B
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 01:51:09.50 +64:52:45.9: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:09.50 +64:52:45.9: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 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 05 13.4012* 01 51 09.50 +64 52 45.9 10.8 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 518229967963921664,2461173.9012,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518229967963921664 20260513.4012 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.93 01:31:48.49 +64:22:26.7
127.28077 1.84374 galactic Cas Second-epoch detections are separated by 0.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:31:48.49 +64:22:26.7 (user input) | T | P | (position from user input) J-Ks=0.844+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.49 +64:22:26.7: 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 01:31:48.49 +64:22:26.7: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 31 48.49 +64 22 26.7 10.9 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
target,2461173.9012,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260513.4012 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.99 01:31:48.42 +64:21:55.1
127.28202 1.83505 galactic Cas Second-epoch detections are separated by 2.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:31:48.42 +64:21:55.1 (user input) | T | P | (position from user input) J-Ks=0.974+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.42 +64:21:55.1: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.42 +64:21:55.1: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 31 48.42 +64 21 55.1 11.0 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,2461173.9012,10.99,0.05,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 20260513.4012 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.85 01:32:40.27 +61:07:38.4
127.89018 -1.34684 galactic Cas Second-epoch detections are separated by 3.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:32:40.27 +61:07:38.4 (user input) | T | P | (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 01:32:40.27 +61:07:38.4: 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 01:32:40.27 +61:07:38.4: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 32 40.27 +61 07 38.4 10.8 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
target,2461173.9012,10.85,0.05,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 20260513.4012 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.87 01:48:29.74 +60:27:35.5
129.91243 -1.63627 galactic Cas Second-epoch detections are separated by 3.5" 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 | target | 01:48:29.74 +60:27:35.5 (user input) | T | P | (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 01:48:29.74 +60:27:35.5: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:29.74 +60:27:35.5: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 48 29.74 +60 27 35.5 10.9 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
target,2461173.9012,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260513.4012 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.08 01:07:29.17 +63:11:00.7
124.74075 0.36816 galactic Cas Second-epoch detections are separated by 4.4" 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 | target | 01:07:29.17 +63:11:00.7 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:29.17 +63:11:00.7: 11.37 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:29.17 +63:11:00.7: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 07 29.17 +63 11 00.7 11.1 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,2461173.9012,11.08,0.05,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 20260513.4012 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.94 01:15:06.86 +60:09:19.2
125.87661 -2.58098 galactic Cas Second-epoch detections are separated by 0.5" 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 | ATO J018.7740+60.1555 | 01:15:06.86 +60:09:19.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: B8V 1992AJ....103.1596B Cl* NGC 433 BCN 42 J-Ks=0.413+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:06.86 +60:09:19.2: 12.82 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:06.86 +60:09:19.2: 14.10 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 15 06.86 +60 09 19.2 10.9 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 J018.7740+60.1555,2461173.9012,10.94,0.05,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 J018.7740+60.1555 20260513.4012 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.05 01:38:11.84 +65:32:59.7
127.74965 3.11649 galactic Cas Second-epoch detections are separated by 1.1" and 6.3 pix
The object was found in VSX 3" ASASSN-V J013812.08+653302.3
Type: L
# Max. Min./Amp. JD0 Period
14.260 V 14.420 V
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 01:38:11.84 +65:32:59.7: 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 01:38:11.84 +65:32:59.7: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 38 11.84 +65 32 59.7 11.1 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
ASASSN-V J013812.08+653302.3,2461173.9012,11.05,0.05,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
ASASSN-V J013812.08+653302.3 20260513.4012 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.00 01:36:50.86 +59:55:48.0
128.59736 -2.44130 galactic Cas Second-epoch detections are separated by 1.1" and 6.1 pix
The object was found in VSX 1" Gaia DR3 509760361181182976
Type: ROT
# Max. Min./Amp. JD0 Period
13.870 G 13.910 G 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 01:36:50.86 +59:55:48.0: 12.80 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:50.86 +59:55:48.0: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 36 50.86 +59 55 48.0 11.0 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 509760361181182976,2461173.9012,11.00,0.05,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 509760361181182976 20260513.4012 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.98 01:38:05.75 +61:04:12.5
128.54598 -1.29201 galactic Cas Second-epoch detections are separated by 2.0" 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 | target | 01:38:05.75 +61:04:12.5 (user input) | T | P | (position from user input) J-Ks=0.901+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:05.75 +61:04:12.5: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:05.75 +61:04:12.5: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 38 05.75 +61 04 12.5 11.0 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,2461173.9012,10.98,0.05,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 20260513.4012 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.05 01:08:36.96 +60:44:52.3
125.03030 -2.05388 galactic Cas Second-epoch detections are separated by 3.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 426363744241527552 | 01:08:34.66 +60:44:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8: 1935BSD...C01....0S BSD 8-1144
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:36.96 +60:44:52.3: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:36.96 +60:44:52.3: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 08 36.96 +60 44 52.3 11.1 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 426363744241527552,2461173.9012,11.05,0.05,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 426363744241527552 20260513.4012 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.99 01:50:39.74 +62:00:54.3
129.81903 -0.06214 galactic Cas Second-epoch detections are separated by 1.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511356332360621440 | 01:50:34.89 +62:00:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1955ApJS....2..123F LF 5 +61 158
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:39.74 +62:00:54.3: 13.21 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:39.74 +62:00:54.3: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 50 39.74 +62 00 54.3 11.0 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 511356332360621440,2461173.9012,10.99,0.05,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 511356332360621440 20260513.4012 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.21 01:29:39.20 +63:18:45.5
127.20725 0.75856 galactic Cas Second-epoch detections are separated by 2.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512422794227736704 | 01:29:32.93 +63:18:37.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8Ib 1987ApJS...64..241S NGC 559 14
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:39.20 +63:18:45.5: 12.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:39.20 +63:18:45.5: 14.12 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 05 13.4012* 01 29 39.20 +63 18 45.5 11.2 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 512422794227736704,2461173.9012,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512422794227736704 20260513.4012 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.84 02:00:32.94 +59:40:06.7
131.56365 -2.03998 galactic Cas Second-epoch detections are separated by 2.3" and 6.5 pix
The object was found in VSX 2" ZTF J020033.07+594008.7
Type: SR
# Max. Min./Amp. JD0 Period
13.621 r Y 0.477 r 2458342.93970 344.838134100000 C
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 02:00:32.94 +59:40:06.7: 11.54 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.94 +59:40:06.7: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 02 00 32.94 +59 40 06.7 10.8 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
ZTF J020033.07+594008.7,2461173.9012,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J020033.07+594008.7 20260513.4012 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.10 01:51:53.56 +63:26:20.2
129.62903 1.35600 galactic Cas Second-epoch detections are separated by 0.9" and 6.3 pix
The object was found in VSX10" ZTF J015152.31+632614.6
Type: EB:
# Max. Min./Amp. JD0 Period
15.451 r Y 0.389 r 2458367.82620 5.408679200000
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 01:51:53.56 +63:26:20.2: 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 01:51:53.56 +63:26:20.2: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 51 53.56 +63 26 20.2 11.1 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 J015152.31+632614.6,2461173.9012,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J015152.31+632614.6 20260513.4012 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.99 02:01:03.88 +64:43:33.7
130.27905 2.85213 galactic Cas Second-epoch detections are separated by 0.3" 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 | target | 02:01:03.88 +64:43:33.7 (user input) | T | P | (position from user input) J-Ks=0.437+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:03.88 +64:43:33.7: 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 02:01:03.88 +64:43:33.7: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 02 01 03.88 +64 43 33.7 11.0 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,2461173.9012,10.99,0.05,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 20260513.4012 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.35 01:22:13.51 +59:52:26.5
126.79077 -2.76685 galactic Cas Second-epoch detections are separated by 2.7" 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 | target | 01:22:13.51 +59:52:26.5 (user input) | T | P | (position from user input) J-Ks=1.005+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:13.51 +59:52:26.5: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:13.51 +59:52:26.5: 14.33 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 22 13.51 +59 52 26.5 11.3 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
target,2461173.9012,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260513.4012 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.21 01:33:30.76 +58:02:21.1
128.49357 -4.37749 galactic Cas Second-epoch detections are separated by 1.7" 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 J023.3712+58.0394 | 01:33:30.76 +58:02:21.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.820+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:30.76 +58:02:21.1: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:30.76 +58:02:21.1: 14.25 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 33 30.76 +58 02 21.1 11.2 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
ATO J023.3712+58.0394,2461173.9012,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J023.3712+58.0394 20260513.4012 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.12 01:56:57.30 +63:00:31.7
130.28634 1.07636 galactic Cas Second-epoch detections are separated by 0.7" 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 | target | 01:56:57.30 +63:00:31.7 (user input) | T | P | (position from user input) J-Ks=0.837+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:57.30 +63:00:31.7: 13.18 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:57.30 +63:00:31.7: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 56 57.30 +63 00 31.7 11.1 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,2461173.9012,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260513.4012 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.57 01:20:52.42 +61:07:03.7
126.48017 -1.55110 galactic Cas Second-epoch detections are separated by 0.3" 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 510497996044470784 | 01:20:51.51 +61:06:37.6 (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 01:20:52.42 +61:07:03.7: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:52.42 +61:07:03.7: 14.35 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 20 52.42 +61 07 03.7 11.6 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 510497996044470784,2461173.9012,11.57,0.05,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 510497996044470784 20260513.4012 11.57CV 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 05 13.4012 2461173.9012 11.52 01:21:55.89 +63:45:22.2
126.29552 1.08374 galactic Cas Second-epoch detections are separated by 0.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:21:55.89 +63:45:22.2 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:55.89 +63:45:22.2: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:55.89 +63:45:22.2: 14.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 01 21 55.89 +63 45 22.2 11.5 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,2461173.9012,11.52,0.05,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 20260513.4012 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 11.71 01:29:47.82 +60:57:24.3
127.57256 -1.56890 galactic Cas Second-epoch detections are separated by 1.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510636289686368512 | 01:29:49.30 +60:57:59.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.216+/-0.051 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:47.82 +60:57:24.3: 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 01:29:47.82 +60:57:24.3: 14.72 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 05 13.4012* 01 29 47.82 +60 57 24.3 11.7 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 510636289686368512,2461173.9012,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510636289686368512 20260513.4012 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.49 02:13:30.59 +65:36:57.6
131.27340 4.08216 galactic Cas Second-epoch detections are separated by 3.5" and 5.7 pix
The object was found in VSX 2" NSVS J0213310+653658
Type: L:
# Max. Min./Amp. JD0 Period
11.668 R1 Y 0.601 R1 73.000000000000
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 02:13:30.59 +65:36:57.6: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:30.59 +65:36:57.6: 14.33 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 02 13 30.59 +65 36 57.6 10.5 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
NSVS J0213310+653658,2461173.9012,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0213310+653658 20260513.4012 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.89 02:12:37.60 +61:35:06.5
132.43319 0.22021 galactic Cas Second-epoch detections are separated by 2.8" and 5.8 pix
The object was found in VSX 2" ZTF J021237.80+613507.4
Type: SR
# Max. Min./Amp. JD0 Period
17.093 g Y 0.595 g 2458334.80460 120.561840400000
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 02:12:37.60 +61:35:06.5: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:12:37.60 +61:35:06.5: 14.78 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 05 13.4012* 02 12 37.60 +61 35 06.5 10.9 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
ZTF J021237.80+613507.4,2461173.9012,10.89,0.05,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 J021237.80+613507.4 20260513.4012 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 8.82 02:15:23.55 +65:01:37.4
131.64682 3.58553 galactic Cas Second-epoch detections are separated by 0.4" and 6.1 pix
The object was found in VSX 3" V0931 Cas
Type: SR
# Max. Min./Amp. JD0 Period
12.800 V 13.500 V 2451453.00000 138.000000000000
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 02:15:23.55 +65:01:37.4: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:23.55 +65:01:37.4: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 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 05 13.4012* 02 15 23.55 +65 01 37.4 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
V0931 Cas,2461173.9012,8.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0931 Cas 20260513.4012 8.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.06 02:13:47.45 +63:11:25.1
132.06227 1.78776 galactic Cas Second-epoch detections are separated by 2.3" and 5.9 pix
The object was found in VSX 2" Gaia DR3 514702769014676224
Type: L
# Max. Min./Amp. JD0 Period
18.400 G 18.590 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 02:13:47.45 +63:11:25.1: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:47.45 +63:11:25.1: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 02 13 47.45 +63 11 25.1 10.1 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 514702769014676224,2461173.9012,10.06,0.05,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 514702769014676224 20260513.4012 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 13.4012 2461173.9012 10.91 02:10:17.67 +60:58:57.3
132.34982 -0.43903 galactic Cas Second-epoch detections are separated by 3.9" and 6.0 pix
The object was found in VSX 1" NSVS J0210179+605902
Type: SR
# Max. Min./Amp. JD0 Period
14.153 r Y 0.631 r 2458450.25450 296.241215300000 C
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 02:10:17.67 +60:58:57.3: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:17.67 +60:58:57.3: 14.74 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 13.4012* 02 10 17.67 +60 58 57.3 10.9 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
NSVS J0210179+605902,2461173.9012,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0210179+605902 20260513.4012 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461173.90144541 13.05.2026 09:37:54.883 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
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: 12 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): 26129
Objects passed selection criteria: 26002
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 18750
Average stars matched: 17100.5 (91.2027 %)
Memory usage VmPeak: 128284 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 10 15:05:05 CDT 2026
VaST build number 1.0rc89-44-gd532a530
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed May 13 06:40:48 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: 2461173.90144541 13.05.2026 09:37:54.883 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 194
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: 117 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): 189983
Objects passed selection criteria: 189502
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 139835
Average stars matched: 127469 (91.1569 %)
Memory usage VmPeak: 1940824 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 10 15:05:05 CDT 2026
VaST build number 1.0rc89-44-gd532a530
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed May 13 06:47:49 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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: 2461173.90097382
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
Entering WCS image calibration mode.
Entering WCS image calibration mode.
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
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
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
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits was not set. Trying to guess...
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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits was not set. Trying to guess...
The guess is 605 arcmin.
The guess is 605 arcmin.
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
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits was not set. Trying to guess...
The guess is 570 arcmin.
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits .... Determining astrometry method...
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.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.cat 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.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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/workdir/vast_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/lib/make_outxyls_for_astrometric_calibration found 16209 high-SNR stars for plate solving
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Generating wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat from image00001.cat
'/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
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits was not set. Trying to guess...
The guess is 569 arcmin.
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.cat 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.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits was not found.
verification OK: /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/vast_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/lib/make_outxyls_for_astrometric_calibration found 16165 high-SNR stars for plate solving
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Generating wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat from image00002.cat
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits created.
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out2922571.xyls"...
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits created.
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out2922574.xyls"...
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:54.565 +61:59:40.70 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 31559 stars ###
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/correct_sextractor_wcs_catalog_usingxy2sky2922987.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
### Converted positions of 31681 stars ###
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
Reading file "./out2922571.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Reading file "./out2922574.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/correct_sextractor_wcs_catalog_usingxy2sky2923070.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
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
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
log-odds ratio 55.9043 (1.90078e+24), 15 match, 0 conflict, 42 distractors, 88 index.
RA,Dec = (25.6228,62.0738), pixel scale 5.92067 arcsec/pix.
Hit/miss: Hit/miss: ----+----+--+---++--++--+---+---+---+---+---+-------+---+(best)-----------+-----------+-----------+---+---
log-odds ratio 55.1077 (8.57021e+23), 15 match, 0 conflict, 42 distractors, 88 index.
RA,Dec = (25.6267,62.0838), pixel scale 5.92056 arcsec/pix.
Hit/miss: Hit/miss: ----+----+--+---++--++--+---+---+---+---+---+-------+---+(best)-----------+-----------+-----------+---+---
Field 1: solved with index index-4114.fits.
Field 1 solved: writing to file ./out2922574.solved to indicate this.
Field 1: solved with index index-4114.fits.
Field 1 solved: writing to file ./out2922571.solved to indicate this.
Field: out2922574.xyls
Field center: (RA,Dec) = (25.697629, 62.076591) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:42:47.431, +62:04:35.729).
Field size: 15.7441 x 10.5363 degrees
Field rotation angle: up is -2.31022 degrees E of N
Field parity: neg
Field: out2922571.xyls
Field center: (RA,Dec) = (25.693672, 62.066474) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:42:46.481, +62:03:59.307).
Field size: 15.7443 x 10.5363 degrees
Field rotation angle: up is -2.31434 degrees E of N
Field parity: neg
Inserting WCS header...
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits' -> 'fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits'
'/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits' -> 'fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits'
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 13 06:40 fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
-rw-r--r-- 1 apache apache 12K May 13 06:40 out2922571.wcs
WCS keywords have been successfully stripped from all HDUs in the file.
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits for reading... done!
Creating new image file (wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits)... done!
-rw-r--r-- 1 apache apache 117M May 13 06:40 fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
-rw-r--r-- 1 apache apache 12K May 13 06:40 out2922574.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits for reading... done!
Creating new image file (wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits)... done!
done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits (fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits (fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out2922571.xyls"...
Reading input file 1 of 1: "out2922574.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2922571.axy"...
Only searching for solutions within 15.68 degrees of RA,Dec (25.6954,62.0673)
log-odds ratio 143.641 (2.41277e+62), 19 match, 0 conflict, 26 distractors, 27 index.
RA,Dec = (25.6956,62.0665), pixel scale 5.96108 arcsec/pix.
Hit/miss: Hit/miss: -+++---+++----+++-++------+-++--+++------+--+(best)-------------------------------------------------------
Reading file "./out2922574.axy"...
Only searching for solutions within 15.68 degrees of RA,Dec (25.6993,62.0774)
log-odds ratio 141.483 (2.78724e+61), 19 match, 0 conflict, 27 distractors, 27 index.
RA,Dec = (25.6997,62.0766), pixel scale 5.96113 arcsec/pix.
Hit/miss: Hit/miss: -+-++--+++----++--+-++----+-+-++--++--------++(best)------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2922571.solved to indicate this.
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2922574.solved to indicate this.
Field: out2922571.xyls
Field center: (RA,Dec) = (25.694737, 62.065360) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:42:46.737, +62:03:55.298).
Field size: 15.7203 x 10.5358 degrees
Field rotation angle: up is -2.34227 degrees E of N
Field parity: neg
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 13 06:40 fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
-rw-r--r-- 1 apache apache 12K May 13 06:40 out2922571.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits for reading... done!
Creating new image file (wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
Field: out2922574.xyls
Field center: (RA,Dec) = (25.698767, 62.075480) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:42:47.704, +62:04:31.727).
Field size: 15.7203 x 10.536 degrees
Field rotation angle: up is -2.33824 degrees E of N
Field parity: neg
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 13 06:40 fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
-rw-r--r-- 1 apache apache 12K May 13 06:41 out2922574.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits for reading... done!
Creating new image file (wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 76623 sources.
Solving...
Reading file "./wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.axy"...
Verifying WCS using indices with quads of size [63.5143, 952.117] arcmin
Verifying WCS with index 39 of 61 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 40 of 61 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 43.01 (4.77542e+18), 22 match, 0 conflict, 375 distractors, 27 index.
RA,Dec = (25.693,62.0645), pixel scale 5.96565 arcsec/pix.
Hit/miss: Hit/miss: -----------------+++--------------------++---+-----------------------------------+------------------
--> log-odds 43.01
Verifying WCS with index 41 of 61 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 199.921 (6.67386e+86), 38 match, 0 conflict, 359 distractors, 49 index.
RA,Dec = (25.693,62.0645), pixel scale 5.96565 arcsec/pix.
Hit/miss: Hit/miss: -------+------++++++------++------------++---+------+-------------+--------------++-----------------
--> log-odds 199.921
Verifying WCS with index 42 of 61 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 526.776 (5.97204e+228), 72 match, 0 conflict, 362 distractors, 91 index.
RA,Dec = (25.693,62.0645), pixel scale 5.96565 arcsec/pix.
Hit/miss: Hit/miss: -------+----++++++++---++-++--+-----+---++---+----+++---+---------++------++-----++---------------+-
--> log-odds 526.776
Verifying WCS with index 43 of 61 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 1268.88 (inf), 158 match, 0 conflict, 467 distractors, 190 index.
RA,Dec = (25.693,62.0645), pixel scale 5.96565 arcsec/pix.
Hit/miss: Hit/miss: ----+-+++--++++++++++-+++-++-+++-+-++-+-++---+++--+++-+-+---+-----++----+-++-----++++---+--+------+-
--> log-odds 1268.88
Verifying WCS with index 44 of 61 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 2439.49 (inf), 301 match, 0 conflict, 538 distractors, 384 index.
RA,Dec = (25.693,62.0645), pixel scale 5.96565 arcsec/pix.
Hit/miss: Hit/miss: +--++-+++--++++++++++-+++-++-+++++-++--+++-+-+++-++++++-+--++++++-+++++++-++-+---++++---+--++++-++++
--> log-odds 2439.49
Verifying WCS with index 45 of 61 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 4336.2 (inf), 570 match, 0 conflict, 892 distractors, 728 index.
RA,Dec = (25.693,62.0645), pixel scale 5.96565 arcsec/pix.
Hit/miss: Hit/miss: +--++-+++--+++++++++++++++++++++++-+++-+++-+-+++++++++++++-++++++-++++++++++++--+++++++++--+++++++++
simplexy: found 81315 sources.
--> log-odds 4336.2
Verifying WCS with index 46 of 61 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 7672.92 (inf), 1091 match, 0 conflict, 1515 distractors, 1444 index.
RA,Dec = (25.693,62.0645), pixel scale 5.96565 arcsec/pix.
Hit/miss: Hit/miss: +--++-+++--+++++++++++++++++++++++++++-+++++++++++++++++++-++++++-+++++++++++++-+++++++++--+++++++++
--> log-odds 7672.92
Got 7 solutions.
Field: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Field center: (RA,Dec) = (25.694727, 62.065490) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:42:46.735, +62:03:55.763).
Field size: 15.7256 x 10.5369 degrees
Field rotation angle: up is -2.3197 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.new"...
renamed 'wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.new' -> 'wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits'
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Generating wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat from image00003.cat
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits created.
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Image size: 938.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:47.141 +62:03:58.86 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 17117 stars ###
'wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/correct_sextractor_wcs_catalog_usingxy2sky2995017.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Solving...
Reading file "./wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.axy"...
Verifying WCS using indices with quads of size [63.5147, 952.125] arcmin
Verifying WCS with index 39 of 61 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 40 of 61 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 47.0166 (2.62448e+20), 23 match, 0 conflict, 422 distractors, 27 index.
RA,Dec = (25.6971,62.0746), pixel scale 5.96569 arcsec/pix.
Hit/miss: Hit/miss: -+-------+-----------------+---------+------+-----------+-------------------------------------------
--> log-odds 47.0166
Verifying WCS with index 41 of 61 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 158.657 (8.01319e+68), 37 match, 0 conflict, 408 distractors, 49 index.
RA,Dec = (25.6971,62.0746), pixel scale 5.96569 arcsec/pix.
Hit/miss: Hit/miss: -+-----+-+----+---------+--+---------+------+-----+-----++-+----------------+-----+-----------------
--> log-odds 158.657
Verifying WCS with index 42 of 61 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 498.225 (2.37916e+216), 72 match, 0 conflict, 409 distractors, 91 index.
RA,Dec = (25.6971,62.0746), pixel scale 5.96569 arcsec/pix.
Hit/miss: Hit/miss: -+--++-+-++---++------+-+--++---+----+------+-----+-+---++-+-------+------+-+---+-+-------+---------
--> log-odds 498.225
Verifying WCS with index 43 of 61 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 1125.57 (inf), 144 match, 0 conflict, 459 distractors, 189 index.
RA,Dec = (25.6971,62.0746), pixel scale 5.96569 arcsec/pix.
Hit/miss: Hit/miss: ++-+++++-++++-++----+-+-+--++++++-+--+----+-+-+---+-+-+-++-+-+-----++---+-+-+---+-+-------++----+--+
--> log-odds 1125.57
Verifying WCS with index 44 of 61 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 2240.52 (inf), 280 match, 0 conflict, 449 distractors, 383 index.
RA,Dec = (25.6971,62.0746), pixel scale 5.96569 arcsec/pix.
Hit/miss: Hit/miss: ++-++++++++++-+++-+-+-+-+--+++++++++-+-++-+-+++-+-+-+++-++++-++++--++++++-+++-+++-+-++-+--++++--+--+
--> log-odds 2240.52
Verifying WCS with index 45 of 61 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 4011.8 (inf), 527 match, 0 conflict, 705 distractors, 726 index.
RA,Dec = (25.6971,62.0746), pixel scale 5.96569 arcsec/pix.
Hit/miss: Hit/miss: +++++++++++++++++-+-+++++--+-+++++++++-++-+-+++++-+-++++++++-+++++-++++++-+++++++-+++++++-++++--+--+
--> log-odds 4011.8
Verifying WCS with index 46 of 61 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 7173.79 (inf), 1033 match, 0 conflict, 1519 distractors, 1443 index.
RA,Dec = (25.6971,62.0746), pixel scale 5.96569 arcsec/pix.
Hit/miss: Hit/miss: +++++++++++++++++-+-+++++--+-+++++++++-++-+++++++-+-+++++++++++++++++++++++++++++-+++++++-+++++-+--+
--> log-odds 7173.79
Got 7 solutions.
Field: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
Field center: (RA,Dec) = (25.698740, 62.075605) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:42:47.698, +62:04:32.177).
Field size: 15.7254 x 10.5368 degrees
Field rotation angle: up is -2.31559 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.new"...
renamed 'wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.new' -> 'wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits'
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
Generating wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat from image00004.cat
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits created.
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
Image size: 938.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:48.104 +62:04:35.27 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 16942 stars ###
'wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/correct_sextractor_wcs_catalog_usingxy2sky3013645.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
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_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Image size: 938.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:47.141 +62:03:58.86 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 01:42:47.141 +62:03:58.86
Angular distance between the image centers 0.0888 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
Image size: 938.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:48.104 +62:04:35.27 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 01:42:48.104 +62:04:35.27
Angular distance between the image centers 0.0989 deg.
###################################
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=N/A worst_q_ratio=N/A
ref2=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=N/A worst_q_ratio=N/A
new1=wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits sigma_overall=N/A worst_q_ratio=N/A
new2=wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits sigma_overall=N/A worst_q_ratio=N/A
reference average sigma_overall=N/A worst_q_ratio=N/A
warn-on-ratio threshold: 2.0x reference
###################################
INFO: WCS quality sigma_overall_arcsec not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality sigma_overall_arcsec not available for comparison (2nd new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (2nd new image new=N/A ref_avg=N/A)
###################################
# 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 01:42:47.141 +62:03:58.86
Second-epoch second image center 01:42:48.104 +62:04:35.27
Angular distance between the image centers 0.01029 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.capEhnLwe4
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.FmZTXZhL3g
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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits &> /tmp/tmp.lNZWQTo2ZR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits &> /tmp/tmp.Hfc9iGMzGM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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.cat
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.cat
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.cat
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.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> '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 3 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
2.5 pix fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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
14.4 mag. fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
14.4 mag. fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.capEhnLwe4 (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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/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.cat 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.cat 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.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, passed=31559
Got 31559 stars (including 27744 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
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 364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 280 matched stars entering correct_measured_positions(), 228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 266 matched stars entering correct_measured_positions(), 9996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
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 403 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 337 matched stars entering correct_measured_positions(), 10041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.88"
Excluding outliers - 331 stars left (next iteration limit 292)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=331 sigma_overall_arcsec=7.729 sigma_q1_arcsec=31.346 sigma_q2_arcsec=12.794 sigma_q3_arcsec=22.422 sigma_q4_arcsec=4.202 n_q1=16 n_q2=97 n_q3=37 n_q4=181 worst_quadrant_to_overall_ratio=4.055
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.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.cat.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.cat.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.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FmZTXZhL3g (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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/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.cat 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.cat 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.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, passed=31681
Got 31681 stars (including 27947 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=973 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.346 n_q1=119 n_q2=244 n_q3=303 n_q4=307 worst_quadrant_to_overall_ratio=1.316
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.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.cat.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.cat.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.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.lNZWQTo2ZR (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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.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_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1163, passed=17117
Got 17117 stars (including 15940 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat
util/solve_plate_with_UCAC5 got 17117 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 16808 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 16809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 16809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
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_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits N_match=969 sigma_overall_arcsec=0.675 sigma_q1_arcsec=0.630 sigma_q2_arcsec=0.707 sigma_q3_arcsec=0.619 sigma_q4_arcsec=0.798 n_q1=281 n_q2=322 n_q3=205 n_q4=161 worst_quadrant_to_overall_ratio=1.181
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Hfc9iGMzGM (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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1229, passed=16942
Got 16942 stars (including 15694 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat
util/solve_plate_with_UCAC5 got 16942 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 16624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 16626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 16626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits N_match=968 sigma_overall_arcsec=0.695 sigma_q1_arcsec=0.615 sigma_q2_arcsec=0.737 sigma_q3_arcsec=0.660 sigma_q4_arcsec=0.770 n_q1=278 n_q2=326 n_q3=201 n_q4=163 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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 01:33:24.37 +60:39:44.9: 12.74 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:24.37 +60:39:44.9: 11.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.01
Forced photometry filter REJECTED candidate at 01:33:24.37 +60:39:44.9: ref_mag=11.22 +/- 0.01 new_mean_mag=10.9859 delta=0.24 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52834_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 52834_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:19:46.43 +58:12:25.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53370_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 53370_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 08339_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:20:32.50 +62:32:00.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
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 ####
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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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
Entering WCS image calibration mode.
Entering WCS image calibration mode.
Entering WCS image calibration mode.
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
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
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
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
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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
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 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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits was not set. Trying to guess...
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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits was not set. Trying to guess...
The guess is 605 arcmin.
The guess is 605 arcmin.
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits was not found.
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
It's a known telescope with plate solutions that are supposed to be good.
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits was not found.
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...
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...
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
'/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
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits was not set. Trying to guess...
'/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
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits was not set. Trying to guess...
The guess is 570 arcmin.
The guess is 569 arcmin.
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.cat 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.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits was not found.
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.cat 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.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits was not found.
verification OK: /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_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Generating wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat from image00001.cat
Generating wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat from image00003.cat
Generating wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat from image00004.cat
Generating wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat from image00002.cat
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits created.
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits created.
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
Image size: 938.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:47.141 +62:03:58.86 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 938.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:48.104 +62:04:35.27 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits created.
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits created.
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:54.565 +61:59:40.70 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 112144 stars ###
'wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/correct_sextractor_wcs_catalog_usingxy2sky3824426.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
### Converted positions of 118720 stars ###
'wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/correct_sextractor_wcs_catalog_usingxy2sky3824436.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
### Converted positions of 222556 stars ###
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/correct_sextractor_wcs_catalog_usingxy2sky3824857.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
### Converted positions of 218998 stars ###
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
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/correct_sextractor_wcs_catalog_usingxy2sky3824860.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
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
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_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Image size: 938.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:47.141 +62:03:58.86 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 01:42:47.141 +62:03:58.86
Angular distance between the image centers 0.0888 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
Image size: 938.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:48.104 +62:04:35.27 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 01:42:48.104 +62:04:35.27
Angular distance between the image centers 0.0989 deg.
###################################
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=N/A worst_q_ratio=N/A
ref2=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=N/A worst_q_ratio=N/A
new1=wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits sigma_overall=N/A worst_q_ratio=N/A
new2=wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits sigma_overall=N/A worst_q_ratio=N/A
reference average sigma_overall=N/A worst_q_ratio=N/A
warn-on-ratio threshold: 2.0x reference
###################################
INFO: WCS quality sigma_overall_arcsec not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality sigma_overall_arcsec not available for comparison (2nd new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (2nd new image new=N/A ref_avg=N/A)
###################################
# 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 01:42:47.141 +62:03:58.86
Second-epoch second image center 01:42:48.104 +62:04:35.27
Angular distance between the image centers 0.01029 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.8UwbJcQOBz
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.UZCq6ge7Y0
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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits &> /tmp/tmp.u6he1s94wh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits &> /tmp/tmp.ti9avGhc7X
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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.cat
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.cat
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.cat
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.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> '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 173 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
2.5 pix fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
2.3 pix fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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
11.7 mag. fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
11.8 mag. fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
All-image limiting magnitude estimate: 11.7 (SNR ) 11.2 (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.8UwbJcQOBz (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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/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.cat 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.cat 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.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=35398, passed=222522
Got 222522 stars (including 186791 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
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 368 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 275 matched stars entering correct_measured_positions(), 212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.82"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 264 matched stars entering correct_measured_positions(), 49591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
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 434 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 49636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
Accuracy estimation diagnostic: 344 matched stars entering correct_measured_positions(), 64908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.78"
Excluding outliers - 344 stars left (next iteration limit 290)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=344 sigma_overall_arcsec=7.924 sigma_q1_arcsec=24.049 sigma_q2_arcsec=13.165 sigma_q3_arcsec=21.493 sigma_q4_arcsec=4.815 n_q1=16 n_q2=127 n_q3=29 n_q4=172 worst_quadrant_to_overall_ratio=3.035
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.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.cat.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.cat.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.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.UZCq6ge7Y0 (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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/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.cat 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.cat 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.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=35098, passed=218974
Got 218974 stars (including 183551 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=974 sigma_overall_arcsec=0.370 sigma_q1_arcsec=0.448 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.374 sigma_q4_arcsec=0.313 n_q1=145 n_q2=246 n_q3=288 n_q4=295 worst_quadrant_to_overall_ratio=1.210
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.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.cat.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.cat.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.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.u6he1s94wh (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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.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_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=11431, passed=112128
Got 112128 stars (including 100573 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat
util/solve_plate_with_UCAC5 got 112128 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.4)
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(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 110740 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 67.4)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 110742 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 110742 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_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits N_match=969 sigma_overall_arcsec=0.687 sigma_q1_arcsec=0.660 sigma_q2_arcsec=0.693 sigma_q3_arcsec=0.555 sigma_q4_arcsec=0.839 n_q1=274 n_q2=291 n_q3=227 n_q4=177 worst_quadrant_to_overall_ratio=1.222
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ti9avGhc7X (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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=12271, passed=118705
Got 118705 stars (including 106304 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat
util/solve_plate_with_UCAC5 got 118705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.4)
Done reading UCAC5 zone files...
Matched 970 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(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 117158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 67.4)
Done reading UCAC5 zone files...
Matched 970 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(), 117158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 117158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
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_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits N_match=969 sigma_overall_arcsec=0.706 sigma_q1_arcsec=0.675 sigma_q2_arcsec=0.756 sigma_q3_arcsec=0.679 sigma_q4_arcsec=0.692 n_q1=276 n_q2=293 n_q3=225 n_q4=175 worst_quadrant_to_overall_ratio=1.072
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-14_20.00sec_-4.90C_LIGHT_0416.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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_2026-05-13_CI_Cas-03-Q2b1x1_063351_TTUQ2b1x1_2766800_AhEftGsW/wcs_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417.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 01:31:14.40 +63:03:09.2: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:04:37.02 +62:52:12.1: 11.35 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:44.67 +60:07:55.1: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:33.33 +60:44:40.2: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:01.08 +64:42:19.2: 11.76 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:03.16 +63:19:18.9: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:35.57 +62:13:54.9: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:14.57 +60:44:05.1: 12.43 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:14.40 +63:03:09.2: 14.18 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:44.67 +60:07:55.1: 13.84 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:04:37.02 +62:52:12.1: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.07
Forced photometry filter KEPT candidate at 01:31:14.40 +63:03:09.2: ref_mag=14.18 +/- 0.07 new_mean_mag=11.5557 delta=2.63 (need > 0.90)
Forced photometry reference-image weighted average: 13.84 +/- 0.06
Forced photometry reference-image weighted average: 13.01 +/- 0.03
Forced photometry filter KEPT candidate at 01:04:37.02 +62:52:12.1: ref_mag=13.01 +/- 0.03 new_mean_mag=11.0083 delta=2.00 (need > 0.90)
Forced photometry filter KEPT candidate at 02:03:44.67 +60:07:55.1: ref_mag=13.84 +/- 0.06 new_mean_mag=10.7884 delta=3.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:01.08 +64:42:19.2: 13.86 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:33.33 +60:44:40.2: 14.03 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:35.57 +62:13:54.9: 13.65 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:14.57 +60:44:05.1: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:03.16 +63:19:18.9: 14.03 +/- 0.06 detection
Forced photometry filter KEPT candidate at 01:12:01.08 +64:42:19.2: ref_mag=13.34 +/- 0.04 new_mean_mag=11.2757 delta=2.06 (need > 0.90)
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter KEPT candidate at 01:22:33.33 +60:44:40.2: ref_mag=14.03 +/- 0.06 new_mean_mag=11.1627 delta=2.87 (need > 0.90)
Forced photometry filter KEPT candidate at 01:28:35.57 +62:13:54.9: ref_mag=13.65 +/- 0.04 new_mean_mag=11.0204 delta=2.63 (need > 0.90)
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:19.94 +62:33:19.0: 13.09 +/- 99.00 upperlimit
Forced photometry filter KEPT candidate at 01:52:14.57 +60:44:05.1: ref_mag=13.51 +/- 0.03 new_mean_mag=11.0278 delta=2.49 (need > 0.90)
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Forced photometry filter KEPT candidate at 02:16:03.16 +63:19:18.9: ref_mag=14.03 +/- 0.06 new_mean_mag=11.0585 delta=2.97 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:32.02 +60:52:20.1: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:19.94 +62:33:19.0: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter KEPT candidate at 01:33:19.94 +62:33:19.0: ref_mag=13.76 +/- 0.04 new_mean_mag=11.0149 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:32.02 +60:52:20.1: 13.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter KEPT candidate at 01:33:32.02 +60:52:20.1: ref_mag=13.60 +/- 0.03 new_mean_mag=10.7669 delta=2.83 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:17.37 +57:53:08.9: 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 01:09:25.30 +64:35:18.7: 12.52 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:17.37 +57:53:08.9: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.05
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.26 +59:59:17.8: 13.37 +/- 99.00 upperlimit
Forced photometry filter KEPT candidate at 01:06:17.37 +57:53:08.9: ref_mag=13.83 +/- 0.05 new_mean_mag=11.0305 delta=2.80 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:26.87 +58:02:20.9: 12.76 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:25.30 +64:35:18.7: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry filter KEPT candidate at 01:09:25.30 +64:35:18.7: ref_mag=13.82 +/- 0.05 new_mean_mag=10.9650 delta=2.85 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.26 +59:59:17.8: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry filter KEPT candidate at 01:07:39.26 +59:59:17.8: ref_mag=13.73 +/- 0.04 new_mean_mag=11.0071 delta=2.72 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:26.87 +58:02:20.9: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Forced photometry filter KEPT candidate at 01:30:26.87 +58:02:20.9: ref_mag=13.86 +/- 0.05 new_mean_mag=10.8769 delta=2.99 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.70 +59:01:14.2: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:25.67 +59:48:03.0: 12.63 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.70 +59:01:14.2: 13.91 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:25.67 +59:48:03.0: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.06
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry filter KEPT candidate at 01:26:05.70 +59:01:14.2: ref_mag=13.91 +/- 0.06 new_mean_mag=10.8585 delta=3.05 (need > 0.90)
Forced photometry filter KEPT candidate at 01:08:25.67 +59:48:03.0: ref_mag=13.73 +/- 0.04 new_mean_mag=10.9671 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 01:10:43.96 +60:59:18.8: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:43.96 +60:59:18.8: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Forced photometry filter KEPT candidate at 01:10:43.96 +60:59:18.8: ref_mag=13.70 +/- 0.04 new_mean_mag=10.9978 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 01:56:43.25 +58:07:17.2: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:07.66 +58:55:54.6: 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 01:56:43.25 +58:07:17.2: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter KEPT candidate at 01:56:43.25 +58:07:17.2: ref_mag=13.33 +/- 0.03 new_mean_mag=10.5753 delta=2.75 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:07.66 +58:55:54.6: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 01:13:07.66 +58:55:54.6: ref_mag=13.45 +/- 0.03 new_mean_mag=10.7145 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:39.14 +59:41:39.5: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:39.14 +59:41:39.5: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Forced photometry filter KEPT candidate at 01:26:39.14 +59:41:39.5: ref_mag=13.51 +/- 0.04 new_mean_mag=10.6721 delta=2.84 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:46.85 +57:53:48.5: 13.06 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:09.23 +61:37:26.9: 12.92 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:46.85 +57:53:48.5: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter KEPT candidate at 02:00:46.85 +57:53:48.5: ref_mag=13.40 +/- 0.03 new_mean_mag=10.5492 delta=2.85 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:09.23 +61:37:26.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 01:09:09.23 +61:37:26.9: ref_mag=13.35 +/- 0.03 new_mean_mag=10.6058 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:24.35 +59:10:24.1: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:24.35 +59:10:24.1: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry filter KEPT candidate at 01:20:24.35 +59:10:24.1: ref_mag=12.28 +/- 0.01 new_mean_mag=9.6369 delta=2.64 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:56.61 +59:35:11.5: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:56.61 +59:35:11.5: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Forced photometry filter KEPT candidate at 01:25:56.61 +59:35:11.5: ref_mag=11.97 +/- 0.01 new_mean_mag=9.2795 delta=2.69 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:34.54 +60:31:05.9: 12.47 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:34.54 +60:31:05.9: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Forced photometry filter KEPT candidate at 01:10:34.54 +60:31:05.9: ref_mag=13.11 +/- 0.03 new_mean_mag=10.0392 delta=3.07 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:24.47 +60:56:06.9: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:36.77 +58:41:37.9: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:24.47 +60:56:06.9: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Forced photometry filter KEPT candidate at 01:07:24.47 +60:56:06.9: ref_mag=13.70 +/- 0.04 new_mean_mag=10.5519 delta=3.15 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:36.77 +58:41:37.9: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Forced photometry filter KEPT candidate at 01:18:36.77 +58:41:37.9: ref_mag=13.50 +/- 0.04 new_mean_mag=10.4528 delta=3.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:27.32 +60:30:01.7: 8.46 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:27.32 +60:30:01.7: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 8.54 +/- 0.01
Forced photometry filter REJECTED candidate at 01:10:27.32 +60:30:01.7: ref_mag=8.54 +/- 0.01 new_mean_mag=10.6079 delta=-2.07 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:45.37 +63:08:24.2: 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 01:24:45.37 +63:08:24.2: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry filter KEPT candidate at 01:24:45.37 +63:08:24.2: ref_mag=13.48 +/- 0.03 new_mean_mag=10.6200 delta=2.86 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:45.41 +64:05:35.4: 11.23 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:45.41 +64:05:35.4: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.04
Forced photometry filter KEPT candidate at 01:10:45.41 +64:05:35.4: ref_mag=12.70 +/- 0.04 new_mean_mag=10.7738 delta=1.92 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.45 +59:18:56.9: 13.05 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.45 +59:18:56.9: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry filter KEPT candidate at 01:06:55.45 +59:18:56.9: ref_mag=13.82 +/- 0.05 new_mean_mag=10.8890 delta=2.93 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:21.50 +61:44:12.7: 12.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:21.50 +61:44:12.7: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Forced photometry filter KEPT candidate at 01:29:21.50 +61:44:12.7: ref_mag=13.63 +/- 0.04 new_mean_mag=10.7607 delta=2.87 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:11.10 +59:09:02.5: 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 01:22:11.10 +59:09:02.5: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Forced photometry filter KEPT candidate at 01:22:11.10 +59:09:02.5: ref_mag=13.71 +/- 0.04 new_mean_mag=10.8102 delta=2.90 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:09.50 +64:52:45.9: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:09.50 +64:52:45.9: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.04
Forced photometry filter KEPT candidate at 01:51:09.50 +64:52:45.9: ref_mag=13.52 +/- 0.04 new_mean_mag=10.7476 delta=2.77 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.49 +64:22:26.7: 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 01:31:48.49 +64:22:26.7: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Forced photometry filter KEPT candidate at 01:31:48.49 +64:22:26.7: ref_mag=13.99 +/- 0.06 new_mean_mag=10.9184 delta=3.07 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.42 +64:21:55.1: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:40.27 +61:07:38.4: 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 01:48:29.74 +60:27:35.5: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.42 +64:21:55.1: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Forced photometry filter KEPT candidate at 01:31:48.42 +64:21:55.1: ref_mag=13.80 +/- 0.05 new_mean_mag=10.9829 delta=2.82 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:40.27 +61:07:38.4: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.06
Forced photometry filter KEPT candidate at 01:32:40.27 +61:07:38.4: ref_mag=13.75 +/- 0.06 new_mean_mag=10.8475 delta=2.90 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:29.74 +60:27:35.5: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Forced photometry filter KEPT candidate at 01:48:29.74 +60:27:35.5: ref_mag=13.79 +/- 0.05 new_mean_mag=10.8532 delta=2.94 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:29.17 +63:11:00.7: 11.37 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:06.86 +60:09:19.2: 12.82 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:29.17 +63:11:00.7: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.05
Forced photometry filter KEPT candidate at 01:07:29.17 +63:11:00.7: ref_mag=12.76 +/- 0.05 new_mean_mag=11.0811 delta=1.68 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:06.86 +60:09:19.2: 14.10 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.09
Forced photometry filter KEPT candidate at 01:15:06.86 +60:09:19.2: ref_mag=13.98 +/- 0.09 new_mean_mag=10.9261 delta=3.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:11.84 +65:32:59.7: 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 01:38:11.84 +65:32:59.7: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.06
Forced photometry filter KEPT candidate at 01:38:11.84 +65:32:59.7: ref_mag=13.85 +/- 0.06 new_mean_mag=11.0503 delta=2.80 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:50.86 +59:55:48.0: 12.80 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:50.86 +59:55:48.0: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.06
Forced photometry filter KEPT candidate at 01:36:50.86 +59:55:48.0: ref_mag=13.95 +/- 0.06 new_mean_mag=11.0002 delta=2.95 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:05.75 +61:04:12.5: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:05.75 +61:04:12.5: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.06
Forced photometry filter KEPT candidate at 01:38:05.75 +61:04:12.5: ref_mag=13.88 +/- 0.06 new_mean_mag=10.9759 delta=2.90 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:36.96 +60:44:52.3: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:36.96 +60:44:52.3: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Forced photometry filter KEPT candidate at 01:08:36.96 +60:44:52.3: ref_mag=13.79 +/- 0.05 new_mean_mag=11.0427 delta=2.75 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:39.20 +63:18:45.5: 12.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:39.74 +62:00:54.3: 13.21 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:39.20 +63:18:45.5: 14.12 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:39.74 +62:00:54.3: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.13
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Forced photometry filter KEPT candidate at 01:50:39.74 +62:00:54.3: ref_mag=13.91 +/- 0.05 new_mean_mag=10.9920 delta=2.92 (need > 0.90)
Forced photometry filter KEPT candidate at 01:29:39.20 +63:18:45.5: ref_mag=14.12 +/- 0.13 new_mean_mag=11.2110 delta=2.91 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:32.94 +59:40:06.7: 11.54 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.94 +59:40:06.7: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.05
Forced photometry filter KEPT candidate at 02:00:32.94 +59:40:06.7: ref_mag=12.91 +/- 0.05 new_mean_mag=10.8093 delta=2.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:53.56 +63:26:20.2: 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 02:01:03.88 +64:43:33.7: 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 01:51:53.56 +63:26:20.2: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.06
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:03.88 +64:43:33.7: 13.69 +/- 0.05 detection
Forced photometry filter KEPT candidate at 01:51:53.56 +63:26:20.2: ref_mag=14.16 +/- 0.06 new_mean_mag=11.0948 delta=3.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.69 +/- 0.05
Forced photometry filter KEPT candidate at 02:01:03.88 +64:43:33.7: ref_mag=13.69 +/- 0.05 new_mean_mag=10.9519 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:13.51 +59:52:26.5: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:30.76 +58:02:21.1: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:13.51 +59:52:26.5: 14.33 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:30.76 +58:02:21.1: 14.25 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.08
Forced photometry reference-image weighted average: 14.25 +/- 0.07
Forced photometry filter KEPT candidate at 01:22:13.51 +59:52:26.5: ref_mag=14.33 +/- 0.08 new_mean_mag=11.3282 delta=3.01 (need > 0.90)
Forced photometry filter KEPT candidate at 01:33:30.76 +58:02:21.1: ref_mag=14.25 +/- 0.07 new_mean_mag=11.2028 delta=3.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:57.30 +63:00:31.7: 13.18 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:57.30 +63:00:31.7: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.07
Forced photometry filter KEPT candidate at 01:56:57.30 +63:00:31.7: ref_mag=13.93 +/- 0.07 new_mean_mag=11.1199 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 01:20:52.42 +61:07:03.7: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:52.42 +61:07:03.7: 14.35 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.08
Forced photometry filter KEPT candidate at 01:20:52.42 +61:07:03.7: ref_mag=14.35 +/- 0.08 new_mean_mag=11.5743 delta=2.78 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:55.89 +63:45:22.2: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:55.89 +63:45:22.2: 14.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.07
Forced photometry filter KEPT candidate at 01:21:55.89 +63:45:22.2: ref_mag=14.31 +/- 0.07 new_mean_mag=11.4979 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 01:29:47.82 +60:57:24.3: 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 01:29:47.82 +60:57:24.3: 14.72 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.13
Forced photometry filter KEPT candidate at 01:29:47.82 +60:57:24.3: ref_mag=14.72 +/- 0.13 new_mean_mag=11.7102 delta=3.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:30.59 +65:36:57.6: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:30.59 +65:36:57.6: 14.33 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.07
Forced photometry filter KEPT candidate at 02:13:30.59 +65:36:57.6: ref_mag=14.33 +/- 0.07 new_mean_mag=10.4920 delta=3.84 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:12:37.60 +61:35:06.5: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:12:37.60 +61:35:06.5: 14.78 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.10
Forced photometry filter KEPT candidate at 02:12:37.60 +61:35:06.5: ref_mag=14.78 +/- 0.10 new_mean_mag=10.8872 delta=3.89 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:23.55 +65:01:37.4: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:47.45 +63:11:25.1: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:23.55 +65:01:37.4: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Forced photometry filter KEPT candidate at 02:15:23.55 +65:01:37.4: ref_mag=12.62 +/- 0.02 new_mean_mag=8.8216 delta=3.80 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:47.45 +63:11:25.1: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Forced photometry filter KEPT candidate at 02:13:47.45 +63:11:25.1: ref_mag=13.96 +/- 0.05 new_mean_mag=10.0613 delta=3.90 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:17.67 +60:58:57.3: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:17.67 +60:58:57.3: 14.74 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.09
Forced photometry filter KEPT candidate at 02:10:17.67 +60:58:57.3: ref_mag=14.74 +/- 0.09 new_mean_mag=10.9087 delta=3.84 (need > 0.90)
Adding exclusion_list_local.txt__out106568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out256827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out272005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out272341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out272661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out273501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out273668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out273919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out274038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out276659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out276906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out277390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93555.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 82s
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: 40s
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Considering the candidate 247629_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247629_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247638_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 247638_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:30:06.77 +61:51:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247645_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 247645_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 247646_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247646_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247648_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247648_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247650_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247650_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247660_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247660_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247661_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247661_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247665_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247665_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247666_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247666_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247667_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247667_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247671_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247671_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247677_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247677_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247678_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247678_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247680_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247680_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247684_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247684_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247689_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 247689_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:59:08.93 +59:51:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247694_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247694_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247695_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247695_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247697_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247697_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247699_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 247699_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:39:24.10 +58:23:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247701_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247701_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247702_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247702_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247703_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247703_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247709_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247709_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247715_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247715_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247717_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 247717_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:01:30.82 +65:05:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247724_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 247724_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:14:45.19 +60:30:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247726_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 247726_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:55:14.64 +59:32:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247728_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 247728_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:43:59.27 +61:55:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247729_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247729_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247730_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 247730_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:16:20.73 +62:42:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247731_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 247731_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 247732_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 247732_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:22:08.35 +60:22:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252208_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 252208_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:44:02.08 +61:53:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253172_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 253172_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:38:00.50 +57:56:45.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253375_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 253375_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:26:41.06 +60:46:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253479_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 253479_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:17:59.17 +57:47:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254524_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 254524_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:26:46.72 +57:46:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255598_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 255598_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:19:12.34 +65:35:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255811_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 255811_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:18:14.18 +61:44:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256827_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 256827_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 257307_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 257307_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:20:11.00 +58:12:08.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 257867_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 257867_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:21:28.16 +57:48:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257905_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 257905_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:58:16.29 +59:38:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258197_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 258197_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:46:33.62 +61:16:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258482_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 258482_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:16:08.65 +58:49:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258552_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 258552_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:43:53.19 +61:53:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258902_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 258902_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:44:17.81 +61:53:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259294_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 259294_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:51:02.50 +64:49:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259610_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 259610_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:44:32.43 +58:45:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259792_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 259792_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:43:03.31 +58:08:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260106_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 260106_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:19:22.36 +58:19:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260179_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 260179_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:11:50.17 +59:02:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260865_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 260865_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:39:56.92 +60:52:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261459_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 261459_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:16:12.72 +62:42:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261934_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 261934_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:15:58.94 +63:12:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262405_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 262405_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:08:33.07 +63:34:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262416_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 262416_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:00:36.90 +58:30:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262530_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 262530_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 262558_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 262558_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 262603_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 262603_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:16:05.00 +58:49:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262623_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 262623_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:04:26.83 +65:05:52.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262809_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 262809_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:27:02.31 +58:03:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262835_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 262835_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:34:10.28 +62:09:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263081_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 263081_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:29:33.25 +63:19:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263188_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 263188_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
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Considering the candidate 263249_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 263249_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:33:23.16 +57:44:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263265_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 263265_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:06:23.59 +62:44:01.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263377_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 263377_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:06:45.41 +59:50:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263427_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 263427_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:38:08.39 +61:03:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263503_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 263503_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:35:50.59 +61:27:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263622_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 263622_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:10:23.86 +60:01:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263758_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 263758_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:14:58.55 +60:30:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263773_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 263773_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:42:33.18 +63:52:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264005_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 264005_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 264136_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 264136_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:13:36.11 +57:52:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264336_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 264336_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:19:03.93 +63:57:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264801_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 264801_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:35:54.40 +60:13:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264970_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 264970_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:37:13.54 +58:38:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265208_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 265208_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:38:12.08 +61:01:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265217_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 265217_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:19:41.62 +62:51:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265369_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 265369_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:34:34.81 +65:48:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265546_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 265546_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:13:30.82 +58:34:24.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 265599_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 265599_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:47:19.01 +63:38:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265654_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 265654_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:31:32.66 +61:02:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265734_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 265734_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 265773_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 265773_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:38:33.90 +60:47:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265793_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 265793_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:44:56.49 +59:46:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265828_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 265828_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 265870_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 265870_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:54:19.00 +63:38:02.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 265897_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 265897_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:16:24.29 +58:04:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266112_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 266112_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 266162_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 266162_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:54:53.12 +58:16:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266174_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 266174_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:20:40.67 +60:23:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266285_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 266285_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:42:28.04 +58:17:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266384_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 266384_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:01:15.09 +59:23:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266449_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 266449_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 266529_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 266529_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:55:53.04 +64:15:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266557_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 266557_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:23:07.66 +61:11:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266575_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 266575_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:02:53.96 +60:15:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266638_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 266638_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 266932_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 266932_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:42:55.10 +64:01:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266963_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 266963_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:14:00.70 +59:02:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266968_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 266968_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 267010_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 267010_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:20:49.37 +64:40:19.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 267017_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 267017_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:01:36.77 +59:57:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267153_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 267153_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 267161_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 267161_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:43:12.88 +64:00:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267534_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 267534_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:17:21.71 +59:22:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267880_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 267880_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:38:07.76 +61:01:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267957_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 267957_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:48:39.98 +59:09:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267989_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 267989_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:44:32.08 +61:36:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267994_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 267994_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:58:04.16 +57:58:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268026_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 268026_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:01:38.97 +61:45:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268030_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 268030_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:44:34.69 +62:36:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268070_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 268070_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 268228_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 268228_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 268303_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 268303_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 268531_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 268531_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:14:22.01 +59:59:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268703_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 268703_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:46:18.30 +60:59:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268970_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 268970_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:20:50.46 +58:20:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268972_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 268972_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:18:04.36 +65:36:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269175_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 269175_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:34:42.71 +58:42:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269360_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 269360_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:27:56.38 +62:46:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269406_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 269406_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:16:37.34 +64:56:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269410_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 269410_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:59:06.10 +59:55:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269499_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 269499_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:54:30.21 +59:06:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269687_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 269687_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:33:46.82 +62:31:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269746_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 269746_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:27:03.99 +64:43:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269932_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 269932_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 270051_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 270051_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 270110_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 270110_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:43:03.37 +58:57:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270193_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 270193_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:46:50.81 +60:39:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270265_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 270265_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:37:41.52 +58:37:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270371_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 270371_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 270457_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 270457_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 270534_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 270534_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 270676_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 270676_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 270740_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 270740_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:58:05.11 +59:36:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270947_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 270947_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:14:00.30 +61:42:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271183_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 271183_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 271240_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 271240_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:29:49.71 +58:44:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271455_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 271455_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:37:13.15 +58:38:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271501_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 271501_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:23:07.93 +63:07:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271701_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 271701_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 272005_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 272005_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 272071_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 272071_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:25:18.85 +62:14:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272341_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 272341_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 272661_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 272661_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 272770_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 272770_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:56:25.42 +62:05:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 273501_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 273501_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 273668_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 273668_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 273919_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 273919_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 274038_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 274038_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 274408_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 274408_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:38:57.24 +63:28:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 274789_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 274789_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:49:06.40 +65:23:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 275457_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 275457_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:41:41.18 +57:56:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 276659_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 276659_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 276906_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 276906_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 277390_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 277390_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 12954_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 12954_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 93555_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 93555_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 70271_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:20:32.46 +62:32:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84112_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 84112_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:07:46.59 +62:11:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21138_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 21138_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 58464_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 58464_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 112593_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:21:55.34 +61:20:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 72532_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:45:35.80 +63:07:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233956_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 233956_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:18:51.78 +62:48:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106568_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
Preparing report for the candidate 106568_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
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Considering the candidate 76113_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 76113_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 02:02:02.19 +62:41:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417
The candidate 39378_fd_Cas-03-Q2b1x1_2026-05-13_04-37-54_20.00sec_-5.00C_LIGHT_0417 did not pass the final checks
**** FOUND 01:47:55.68 +64:32:53.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 126s
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 ####
02:10:17.67 +60:58:57.3
02:13:30.59 +65:36:57.6
02:15:23.55 +65:01:37.4
01:31:14.40 +63:03:09.2
01:22:33.33 +60:44:40.2
02:16:03.16 +63:19:18.9
02:03:44.67 +60:07:55.1
01:28:35.57 +62:13:54.9
01:12:01.08 +64:42:19.2
01:52:14.57 +60:44:05.1
01:04:37.02 +62:52:12.1
01:33:19.94 +62:33:19.0
01:33:32.02 +60:52:20.1
01:06:17.37 +57:53:08.9
01:09:25.30 +64:35:18.7
01:07:39.26 +59:59:17.8
01:30:26.87 +58:02:20.9
01:26:05.70 +59:01:14.2
01:08:25.67 +59:48:03.0
01:10:43.96 +60:59:18.8
01:56:43.25 +58:07:17.2
01:13:07.66 +58:55:54.6
01:26:39.14 +59:41:39.5
02:00:46.85 +57:53:48.5
01:09:09.23 +61:37:26.9
01:20:24.35 +59:10:24.1
01:25:56.61 +59:35:11.5
01:10:34.54 +60:31:05.9
01:07:24.47 +60:56:06.9
01:18:36.77 +58:41:37.9
01:24:45.37 +63:08:24.2
01:10:45.41 +64:05:35.4
01:06:55.45 +59:18:56.9
01:29:21.50 +61:44:12.7
01:22:11.10 +59:09:02.5
01:51:09.50 +64:52:45.9
01:31:48.49 +64:22:26.7
01:31:48.42 +64:21:55.1
01:32:40.27 +61:07:38.4
01:48:29.74 +60:27:35.5
01:07:29.17 +63:11:00.7
01:15:06.86 +60:09:19.2
01:38:11.84 +65:32:59.7
01:36:50.86 +59:55:48.0
01:38:05.75 +61:04:12.5
01:08:36.96 +60:44:52.3
01:50:39.74 +62:00:54.3
01:29:39.20 +63:18:45.5
02:00:32.94 +59:40:06.7
01:51:53.56 +63:26:20.2
02:01:03.88 +64:43:33.7
01:22:13.51 +59:52:26.5
01:33:30.76 +58:02:21.1
01:56:57.30 +63:00:31.7
01:20:52.42 +61:07:03.7
01:21:55.89 +63:45:22.2
01:29:47.82 +60:57:24.3
02:13:47.45 +63:11:25.1
02:12:37.60 +61:35:06.5
########### 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 ####
01:31:14.40 +63:03:09.2
01:22:33.33 +60:44:40.2
02:16:03.16 +63:19:18.9
02:03:44.67 +60:07:55.1
01:28:35.57 +62:13:54.9
01:12:01.08 +64:42:19.2
01:52:14.57 +60:44:05.1
01:04:37.02 +62:52:12.1
01:33:19.94 +62:33:19.0
01:33:32.02 +60:52:20.1
01:06:17.37 +57:53:08.9
01:09:25.30 +64:35:18.7
01:07:39.26 +59:59:17.8
01:30:26.87 +58:02:20.9
01:26:05.70 +59:01:14.2
01:08:25.67 +59:48:03.0
01:10:43.96 +60:59:18.8
01:56:43.25 +58:07:17.2
01:13:07.66 +58:55:54.6
01:26:39.14 +59:41:39.5
02:00:46.85 +57:53:48.5
01:09:09.23 +61:37:26.9
01:20:24.35 +59:10:24.1
01:25:56.61 +59:35:11.5
01:10:34.54 +60:31:05.9
01:07:24.47 +60:56:06.9
01:18:36.77 +58:41:37.9
01:24:45.37 +63:08:24.2
01:10:45.41 +64:05:35.4
01:06:55.45 +59:18:56.9
01:29:21.50 +61:44:12.7
01:22:11.10 +59:09:02.5
01:51:09.50 +64:52:45.9
01:31:48.49 +64:22:26.7
01:31:48.42 +64:21:55.1
01:32:40.27 +61:07:38.4
01:48:29.74 +60:27:35.5
01:07:29.17 +63:11:00.7
01:15:06.86 +60:09:19.2
01:38:11.84 +65:32:59.7
01:36:50.86 +59:55:48.0
01:38:05.75 +61:04:12.5
01:08:36.96 +60:44:52.3
01:50:39.74 +62:00:54.3
01:29:39.20 +63:18:45.5
02:00:32.94 +59:40:06.7
01:51:53.56 +63:26:20.2
02:01:03.88 +64:43:33.7
01:22:13.51 +59:52:26.5
01:33:30.76 +58:02:21.1
01:56:57.30 +63:00:31.7
01:20:52.42 +61:07:03.7
01:21:55.89 +63:45:22.2
01:29:47.82 +60:57:24.3
02:13:30.59 +65:36:57.6
02:12:37.60 +61:35:06.5
02:15:23.55 +65:01:37.4
02:13:47.45 +63:11:25.1
02:10:17.67 +60:58:57.3
###################################################################################
01:31:14.40 +63:03:09.2 -- not an asteroid (will add it to exclusion list)
01:22:33.33 +60:44:40.2 -- not an asteroid (will add it to exclusion list)
02:16:03.16 +63:19:18.9 -- not an asteroid (will add it to exclusion list)
02:03:44.67 +60:07:55.1 -- not an asteroid (will add it to exclusion list)
01:28:35.57 +62:13:54.9 -- not an asteroid (will add it to exclusion list)
01:12:01.08 +64:42:19.2 -- not an asteroid (will add it to exclusion list)
01:52:14.57 +60:44:05.1 -- not an asteroid (will add it to exclusion list)
01:04:37.02 +62:52:12.1 -- not an asteroid (will add it to exclusion list)
01:33:19.94 +62:33:19.0 -- not an asteroid (will add it to exclusion list)
01:33:32.02 +60:52:20.1 -- not an asteroid (will add it to exclusion list)
01:06:17.37 +57:53:08.9 -- not an asteroid (will add it to exclusion list)
01:09:25.30 +64:35:18.7 -- not an asteroid (will add it to exclusion list)
01:07:39.26 +59:59:17.8 -- not an asteroid (will add it to exclusion list)
01:30:26.87 +58:02:20.9 -- not an asteroid (will add it to exclusion list)
01:26:05.70 +59:01:14.2 -- not an asteroid (will add it to exclusion list)
01:08:25.67 +59:48:03.0 -- not an asteroid (will add it to exclusion list)
01:10:43.96 +60:59:18.8 -- not an asteroid (will add it to exclusion list)
01:56:43.25 +58:07:17.2 -- not an asteroid (will add it to exclusion list)
01:13:07.66 +58:55:54.6 -- not an asteroid (will add it to exclusion list)
01:26:39.14 +59:41:39.5 -- not an asteroid (will add it to exclusion list)
02:00:46.85 +57:53:48.5 -- not an asteroid (will add it to exclusion list)
01:09:09.23 +61:37:26.9 -- not an asteroid (will add it to exclusion list)
01:20:24.35 +59:10:24.1 -- not an asteroid (will add it to exclusion list)
01:25:56.61 +59:35:11.5 -- not an asteroid (will add it to exclusion list)
01:10:34.54 +60:31:05.9 -- not an asteroid (will add it to exclusion list)
01:07:24.47 +60:56:06.9 -- not an asteroid (will add it to exclusion list)
01:18:36.77 +58:41:37.9 -- not an asteroid (will add it to exclusion list)
01:24:45.37 +63:08:24.2 -- not an asteroid (will add it to exclusion list)
01:10:45.41 +64:05:35.4 -- not an asteroid (will add it to exclusion list)
01:06:55.45 +59:18:56.9 -- not an asteroid (will add it to exclusion list)
01:29:21.50 +61:44:12.7 -- not an asteroid (will add it to exclusion list)
01:22:11.10 +59:09:02.5 -- not an asteroid (will add it to exclusion list)
01:51:09.50 +64:52:45.9 -- not an asteroid (will add it to exclusion list)
01:31:48.49 +64:22:26.7 -- not an asteroid (will add it to exclusion list)
01:31:48.42 +64:21:55.1 -- not an asteroid (will add it to exclusion list)
01:32:40.27 +61:07:38.4 -- not an asteroid (will add it to exclusion list)
01:48:29.74 +60:27:35.5 -- not an asteroid (will add it to exclusion list)
01:07:29.17 +63:11:00.7 -- not an asteroid (will add it to exclusion list)
01:15:06.86 +60:09:19.2 -- not an asteroid (will add it to exclusion list)
01:38:11.84 +65:32:59.7 -- not an asteroid (will add it to exclusion list)
01:36:50.86 +59:55:48.0 -- not an asteroid (will add it to exclusion list)
01:38:05.75 +61:04:12.5 -- not an asteroid (will add it to exclusion list)
01:08:36.96 +60:44:52.3 -- not an asteroid (will add it to exclusion list)
01:50:39.74 +62:00:54.3 -- not an asteroid (will add it to exclusion list)
01:29:39.20 +63:18:45.5 -- not an asteroid (will add it to exclusion list)
02:00:32.94 +59:40:06.7 -- not an asteroid (will add it to exclusion list)
01:51:53.56 +63:26:20.2 -- not an asteroid (will add it to exclusion list)
02:01:03.88 +64:43:33.7 -- not an asteroid (will add it to exclusion list)
01:22:13.51 +59:52:26.5 -- not an asteroid (will add it to exclusion list)
01:33:30.76 +58:02:21.1 -- not an asteroid (will add it to exclusion list)
01:56:57.30 +63:00:31.7 -- not an asteroid (will add it to exclusion list)
01:20:52.42 +61:07:03.7 -- not an asteroid (will add it to exclusion list)
01:21:55.89 +63:45:22.2 -- not an asteroid (will add it to exclusion list)
01:29:47.82 +60:57:24.3 -- not an asteroid (will add it to exclusion list)
02:13:30.59 +65:36:57.6 -- not an asteroid (will add it to exclusion list)
02:12:37.60 +61:35:06.5 -- not an asteroid (will add it to exclusion list)
02:15:23.55 +65:01:37.4 -- not an asteroid (will add it to exclusion list)
02:13:47.45 +63:11:25.1 -- not an asteroid (will add it to exclusion list)
02:10:17.67 +60:58:57.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:04:37.02 +62:52:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:17.37 +57:53:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:55.45 +59:18:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:24.47 +60:56:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:29.17 +63:11:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.26 +59:59:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:25.67 +59:48:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:36.96 +60:44:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:09.23 +61:37:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:25.30 +64:35:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:34.54 +60:31:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:43.96 +60:59:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:45.41 +64:05:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:01.08 +64:42:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:07.66 +58:55:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:06.86 +60:09:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:36.77 +58:41:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:24.35 +59:10:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:52.42 +61:07:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:55.89 +63:45:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:11.10 +59:09:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:13.51 +59:52:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:33.33 +60:44:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:45.37 +63:08:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:56.61 +59:35:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:05.70 +59:01:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:39.14 +59:41:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:35.57 +62:13:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:21.50 +61:44:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:39.20 +63:18:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:47.82 +60:57:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:26.87 +58:02:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:14.40 +63:03:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.42 +64:21:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.49 +64:22:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:40.27 +61:07:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:19.94 +62:33:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:30.76 +58:02:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:32.02 +60:52:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:50.86 +59:55:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:05.75 +61:04:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:11.84 +65:32:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:29.74 +60:27:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:39.74 +62:00:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:09.50 +64:52:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:53.56 +63:26:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:14.57 +60:44:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:43.25 +58:07:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:57.30 +63:00:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:32.94 +59:40:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:46.85 +57:53:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:03.88 +64:43:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:44.67 +60:07:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:17.67 +60:58:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:37.60 +61:35:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:30.59 +65:36:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:47.45 +63:11:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:23.55 +65:01:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:03.16 +63:19:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:04:37.02 +62:52:12.1 -- a known variable star
01:06:17.37 +57:53:08.9 -- not a known variable star
01:06:55.45 +59:18:56.9 -- not a known variable star
01:07:24.47 +60:56:06.9 -- a known variable star
01:07:29.17 +63:11:00.7 -- not a known variable star
01:07:39.26 +59:59:17.8 -- not a known variable star
01:08:25.67 +59:48:03.0 -- not a known variable star
01:08:36.96 +60:44:52.3 -- not a known variable star
01:09:09.23 +61:37:26.9 -- a known variable star
01:09:25.30 +64:35:18.7 -- not a known variable star
01:10:34.54 +60:31:05.9 -- a known variable star
01:10:43.96 +60:59:18.8 -- not a known variable star
01:10:45.41 +64:05:35.4 -- not a known variable star
01:12:01.08 +64:42:19.2 -- a known variable star
01:13:07.66 +58:55:54.6 -- a known variable star
01:15:06.86 +60:09:19.2 -- not a known variable star
01:18:36.77 +58:41:37.9 -- a known variable star
01:20:24.35 +59:10:24.1 -- not a known variable star
01:20:52.42 +61:07:03.7 -- not a known variable star
01:21:55.89 +63:45:22.2 -- not a known variable star
01:22:11.10 +59:09:02.5 -- not a known variable star
01:22:13.51 +59:52:26.5 -- not a known variable star
01:22:33.33 +60:44:40.2 -- not a known variable star
01:24:45.37 +63:08:24.2 -- not a known variable star
01:25:56.61 +59:35:11.5 -- not a known variable star
01:26:05.70 +59:01:14.2 -- not a known variable star
01:26:39.14 +59:41:39.5 -- a known variable star
01:28:35.57 +62:13:54.9 -- not a known variable star
01:29:21.50 +61:44:12.7 -- not a known variable star
01:29:39.20 +63:18:45.5 -- not a known variable star
01:29:47.82 +60:57:24.3 -- not a known variable star
01:30:26.87 +58:02:20.9 -- not a known variable star
01:31:14.40 +63:03:09.2 -- a known variable star
01:31:48.42 +64:21:55.1 -- not a known variable star
01:31:48.49 +64:22:26.7 -- not a known variable star
01:32:40.27 +61:07:38.4 -- not a known variable star
01:33:19.94 +62:33:19.0 -- not a known variable star
01:33:30.76 +58:02:21.1 -- not a known variable star
01:33:32.02 +60:52:20.1 -- a known variable star
01:36:50.86 +59:55:48.0 -- a known variable star
01:38:05.75 +61:04:12.5 -- not a known variable star
01:38:11.84 +65:32:59.7 -- a known variable star
01:48:29.74 +60:27:35.5 -- not a known variable star
01:50:39.74 +62:00:54.3 -- not a known variable star
01:51:09.50 +64:52:45.9 -- a known variable star
01:51:53.56 +63:26:20.2 -- a known variable star
01:52:14.57 +60:44:05.1 -- a known variable star
01:56:43.25 +58:07:17.2 -- not a known variable star
01:56:57.30 +63:00:31.7 -- not a known variable star
02:00:32.94 +59:40:06.7 -- a known variable star
02:00:46.85 +57:53:48.5 -- not a known variable star
02:01:03.88 +64:43:33.7 -- not a known variable star
02:03:44.67 +60:07:55.1 -- a known variable star
02:10:17.67 +60:58:57.3 -- a known variable star
02:12:37.60 +61:35:06.5 -- a known variable star
02:13:30.59 +65:36:57.6 -- a known variable star
02:13:47.45 +63:11:25.1 -- a known variable star
02:15:23.55 +65:01:37.4 -- a known variable star
02:16:03.16 +63:19:18.9 -- not a known variable star
Found 37 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
59 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 59 (excluding asteroids and hot pixels, 37 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461173.90097382 -observatory V36
03:13:38.93 +17:53:54.2 Mercury (-2.3mag)
05:28:36.45 +24:38:39.6 Venus (-3.9mag)
01:35:32.03 +09:06:06.9 Mars (1.2mag)
07:28:35.68 +22:16:41.2 Jupiter (-2.0mag)
00:40:39.58 +01:58:51.0 Saturn (0.9mag)
03:53:57.88 +20:07:00.8 Uranus (5.8mag)
00:14:03.53 +00:04:34.0 Neptune (7.8mag)
20:34:13.07 -22:56:32.3 Pluto (14.5mag)
00:18:15.24 +03:48:55.1 Moon (-9.3mag)
-rw-r--r-- 1 apache apache 362 May 13 06:40 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461173.90097382:
07:28:39.30 +22:16:30.3 Io (5.9mag)
07:28:25.03 +22:17:08.2 Europa (6.1mag)
07:28:50.76 +22:16:07.7 Ganymede (5.5mag)
07:28:13.66 +22:17:40.7 Callisto (6.7mag)
07:30:27.59 +21:54:52.6 Himalia (15.5mag)
07:28:37.02 +22:16:39.4 Thebe (16.4mag)
07:30:55.31 +22:21:08.1 Elara (17.4mag)
07:29:17.13 +22:42:16.9 Pasiphae (17.6mag)
07:36:10.14 +22:16:44.5 Carme (18.7mag)
00:40:51.46 +01:58:45.0 Titan (8.7mag)
00:40:38.56 +01:58:50.0 Rhea (10.0mag)
00:40:32.44 +01:57:03.1 Iapetus (11.4mag)
00:40:28.46 +01:59:06.9 Hyperion (14.7mag)
00:41:51.17 +02:04:21.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 13 06:40 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461173.90097382:
17:01:05.54 -29:58:00.5 JWST
17:03:12.96 +44:04:52.0 Chandra
20:43:58.27 +36:52:46.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 13 06:40 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461173.90097382 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
-rw-r--r-- 1 apache apache 67 May 13 06:40 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -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
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
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
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
12:59:50.45 -10:58:38.80 2026-05-9.06 17.5
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
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
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
12:59:50.45 -10:58:38.80 2026-05-9.06 17.5
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 2026-04-9.29 13.32
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
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
-rw-r--r-- 1 apache apache 5.8K May 13 06:40 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
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
-rw-r--r-- 1 apache apache 188K May 13 06:40 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:09:54.646 +28:11:51.05 AT 2026lqu 2026-05-07.78 19.48
14:13:25.435 +31:44:42.42 AT 2026lqt 2026-05-07.24 19.7698
14:06:22.543 +38:49:54.42 AT 2026lqs 2026-05-07.24 19.8631
14:54:10.237 -03:52:49.28 AT 2026lqr 2026-05-07.25 19.8999
13:02:32.987 -03:48:25.48 AT 2026lqq 2026-05-07.19 19.9293
16:41:22.394 +13:54:09.90 AT 2026lqp 2026-05-07.34 19.5433
13:59:13.517 -07:06:16.95 AT 2026lqo 2026-05-07.29 20.0474
16:06:17.802 +01:31:51.31 AT 2026lqn 2026-05-07.33 19.6684
19:47:24.194 +05:07:23.61 AT 2026lqm 2026-05-07.37 19.6683
16:04:43.617 +22:06:14.17 AT 2026lql 2026-05-07.33 19.8474
16:29:59.999 -11:56:47.82 AT 2026lqk 2026-05-07.34 19.7484
20:27:21.425 +83:01:37.26 AT 2026lqj 2026-05-08.31 19.889
10:36:13.003 -11:05:58.46 AT 2026lqi 2026-05-07.21 18.876
15:48:00.654 +16:46:23.35 AT 2026lqh 2026-05-06.03 20.03
14:09:34.482 +54:26:30.92 AT 2026lqg 2026-05-06.01 19.54
11:36:44.072 +07:14:34.91 AT 2026lqf 2026-05-07.27 19.909
11:50:54.655 +61:14:46.88 AT 2026lqe 2026-05-07.19 19.9549
08:08:30.782 +17:43:25.65 AT 2026lqd 2026-05-07.30 19.184
14:49:57.889 -13:06:09.83 AT 2026lqc 2026-05-07.37 19.424
12:47:29.648 +01:58:18.11 AT 2026lqb 2026-05-07.19 19.818
-rw-r--r-- 1 apache apache 30K May 13 06:40 tns_transients_list.txt
