This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 10.02 00:04:40.61 +55:32:17.7
116.30234 -6.73044 galactic Cas Second-epoch detections are separated by 1.2" and 5.7 pix
The object was found in VSX 3" DI Cas
Type: M
# Max. Min./Amp. JD0 Period
11.200 V 16.500 V 2437170.00000 363.900000000000 M5
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:04:40.61 +55:32:17.7: 14.33 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:04:40.61 +55:32:17.7: 14.24 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.28 +/- 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 07 04.3157* 00 04 40.61 +55 32 17.7 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
DI Cas,2461225.8157,10.02,0.05,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
DI Cas 20260704.3157 10.02CV 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 07 04.3157 2461225.8157 10.96 00:20:46.10 +50:11:50.5
117.91549 -12.37542 galactic Cas Second-epoch detections are separated by 2.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:20:46.10 +50:11:50.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:20:46.10 +50:11:50.5: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:20:46.10 +50:11:50.5: 15.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 20 46.10 +50 11 50.5 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,2461225.8157,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 7.39 23:58:26.78 +51:26:16.1
114.57612 -10.57217 galactic Cas Second-epoch detections are separated by 5.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:26.78 +51:26:16.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:58:26.78 +51:26:16.1: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:58:26.78 +51:26:16.1: 15.50 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.50 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 58 26.78 +51 26 16.1 7.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461225.8157,7.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 7.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 7.49 00:23:11.80 +55:47:31.5
118.94088 -6.86067 galactic Cas Second-epoch detections are separated by 2.9" and 5.7 pix
The object was found in VSX21" T Cas
Type: M
# Max. Min./Amp. JD0 Period
6.900 V 12.400 V 2459170.00000 443.500000000000 M6e-M9.0e
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:23:11.80 +55:47:31.5: 9.14 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:23:11.80 +55:47:31.5: 9.18 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.16 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 23 11.80 +55 47 31.5 7.5 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
T Cas,2461225.8157,7.49,0.05,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
T Cas 20260704.3157 7.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.41 00:06:46.16 +53:36:36.3
116.25718 -8.68177 galactic Cas Second-epoch detections are separated by 5.4" 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 | target | 00:06:46.16 +53:36:36.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:06:46.16 +53:36:36.3: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:06:46.16 +53:36:36.3: 15.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 06 46.16 +53 36 36.3 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461225.8157,13.41,0.05,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 20260704.3157 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.38 23:36:23.82 +53:17:52.2
111.74154 -7.93567 galactic Cas Second-epoch detections are separated by 8.9" 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 | 23:36:23.82 +53:17:52.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:36:23.82 +53:17:52.2: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:36:23.82 +53:17:52.2: 15.74 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 36 23.82 +53 17 52.2 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461225.8157,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.36 00:04:18.55 +51:51:34.0
115.56702 -10.33709 galactic Cas Second-epoch detections are separated by 8.0" 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 | 00:04:18.55 +51:51:34.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:04:18.55 +51:51:34.0: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:04:18.55 +51:51:34.0: 15.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 04 18.55 +51 51 34.0 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461225.8157,13.36,0.05,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 20260704.3157 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.30 23:29:20.51 +56:41:07.2
111.79630 -4.40099 galactic Cas Second-epoch detections are separated by 7.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:29:20.51 +56:41:07.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:29:20.51 +56:41:07.2: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:29:20.51 +56:41:07.2: 15.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 29 20.51 +56 41 07.2 13.3 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,2461225.8157,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.15 23:55:24.21 +51:47:36.3
114.18405 -10.12405 galactic Cas Second-epoch detections are separated by 7.3" 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 | ATO J358.8546+51.8043 | 23:55:24.21 +51:47:36.3 (user input) | CBH (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:55:24.21 +51:47:36.3: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:55:24.21 +51:47:36.3: 15.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 55 24.21 +51 47 36.3 13.2 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 J358.8546+51.8043,2461225.8157,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.8546+51.8043 20260704.3157 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 12.28 00:23:24.19 +54:55:49.4
118.87483 -7.72037 galactic Cas Second-epoch detections are separated by 4.3" 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 419675758603946752 | 00:23:29.13 +54:55:52.6 (Gaia DR3) | DSCT/GDOR (local) | 0.764200000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:23:24.19 +54:55:49.4: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:23:24.19 +54:55:49.4: 15.76 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 23 24.19 +54 55 49.4 12.3 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 419675758603946752,2461225.8157,12.28,0.05,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 419675758603946752 20260704.3157 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 12.26 23:42:59.05 +52:41:50.6
112.53597 -8.78713 galactic Cas Second-epoch detections are separated by 8.8" 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 1993026732733577216 | 23:43:01.74 +52:41:33.0 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:42:59.05 +52:41:50.6: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:42:59.05 +52:41:50.6: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 42 59.05 +52 41 50.6 12.3 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 1993026732733577216,2461225.8157,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993026732733577216 20260704.3157 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 11.80 23:46:41.23 +54:28:38.1
113.53506 -7.20886 galactic Cas Second-epoch detections are separated by 3.3" and 5.7 pix
The object was found in VSX20" Gaia DR3 1993783609051194496
Type: VAR
# Max. Min./Amp. JD0 Period
10.550 G 10.630 G 0.017361000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:46:41.23 +54:28:38.1: 13.06 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:46:41.23 +54:28:38.1: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 46 41.23 +54 28 38.1 11.8 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 1993783609051194496,2461225.8157,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993783609051194496 20260704.3157 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 11.74 00:14:53.52 +53:15:51.3
117.41060 -9.21526 galactic Cas Second-epoch detections are separated by 6.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:14:53.52 +53:15:51.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:14:53.52 +53:15:51.3: 14.35 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:14:53.52 +53:15:51.3: 14.22 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.28 +/- 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 07 04.3157* 00 14 53.52 +53 15 51.3 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
target,2461225.8157,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 12.30 23:59:20.52 +50:35:47.9
114.53998 -11.42431 galactic Cas Second-epoch detections are separated by 6.0" 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 | ATO J359.8180+50.5949 | 23:59:20.52 +50:35:47.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:59:20.52 +50:35:47.9: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:59:20.52 +50:35:47.9: 15.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 59 20.52 +50 35 47.9 12.3 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
ATO J359.8180+50.5949,2461225.8157,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.8180+50.5949 20260704.3157 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 12.40 00:23:00.46 +55:45:43.2
118.91093 -6.88763 galactic Cas Second-epoch detections are separated by 8.4" 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 | Gaia DR3 421412471580910336 | 00:23:03.42 +55:45:36.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:23:00.46 +55:45:43.2: 14.90 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:23:00.46 +55:45:43.2: 15.05 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 23 00.46 +55 45 43.2 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421412471580910336,2461225.8157,12.40,0.05,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 421412471580910336 20260704.3157 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 12.65 00:16:25.12 +53:58:17.8
117.73776 -8.54659 galactic Cas Second-epoch detections are separated by 6.2" 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 | target | 00:16:25.12 +53:58:17.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:16:25.12 +53:58:17.8: 15.29 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:16:25.12 +53:58:17.8: 15.19 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 16 25.12 +53 58 17.8 12.7 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
target,2461225.8157,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 12.66 23:31:40.65 +49:36:15.0
109.90924 -11.24014 galactic And Second-epoch detections are separated by 8.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:31:40.65 +49:36:15.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:31:40.65 +49:36:15.0: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:31:40.65 +49:36:15.0: 15.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 31 40.65 +49 36 15.0 12.7 U And 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,2461225.8157,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 12.95 23:36:25.20 +55:17:30.9
112.32407 -6.02724 galactic Cas Second-epoch detections are separated by 8.2" and 5.5 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 | 23:36:25.20 +55:17:30.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:36:25.20 +55:17:30.9: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:36:25.20 +55:17:30.9: 15.68 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 36 25.20 +55 17 30.9 12.9 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,2461225.8157,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.02 23:49:54.89 +53:28:41.6
113.75314 -8.29353 galactic Cas Second-epoch detections are separated by 6.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:49:54.89 +53:28:41.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:49:54.89 +53:28:41.6: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:49:54.89 +53:28:41.6: 15.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 49 54.89 +53 28 41.6 13.0 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,2461225.8157,13.02,0.05,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
target 20260704.3157 13.02CV 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 07 04.3157 2461225.8157 12.98 23:41:52.97 +52:45:15.2
112.38875 -8.68783 galactic Cas Second-epoch detections are separated by 8.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J355.4516+52.7548 | 23:41:52.97 +52:45:15.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:41:52.97 +52:45:15.2: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:41:52.97 +52:45:15.2: 15.79 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 41 52.97 +52 45 15.2 13.0 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 J355.4516+52.7548,2461225.8157,12.98,0.05,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
ATO J355.4516+52.7548 20260704.3157 12.98CV 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 07 04.3157 2461225.8157 13.12 23:43:28.34 +50:59:01.0
112.14956 -10.45973 galactic Cas Second-epoch detections are separated by 6.7" and 5.5 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 | 23:43:28.34 +50:59:01.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:43:28.34 +50:59:01.0: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:43:28.34 +50:59:01.0: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 43 28.34 +50 59 01.0 13.1 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,2461225.8157,13.12,0.05,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 20260704.3157 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 12.96 00:23:22.81 +55:49:22.8
118.97011 -6.83277 galactic Cas Second-epoch detections are separated by 6.6" and 5.5 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 J005.8518+55.8256 | 00:23:22.81 +55:49:22.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:23:22.81 +55:49:22.8: 14.66 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:23:22.81 +55:49:22.8: 14.88 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 23 22.81 +55 49 22.8 13.0 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 J005.8518+55.8256,2461225.8157,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J005.8518+55.8256 20260704.3157 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 12.97 00:10:23.32 +49:55:14.2
116.18694 -12.41278 galactic Cas Second-epoch detections are separated by 3.5" and 5.5 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 J002.6043+49.9106 | 00:10:23.32 +49:55:14.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:10:23.32 +49:55:14.2: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:10:23.32 +49:55:14.2: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 10 23.32 +49 55 14.2 13.0 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 J002.6043+49.9106,2461225.8157,12.97,0.05,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
ATO J002.6043+49.9106 20260704.3157 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.08 23:57:56.94 +50:30:33.7
114.30067 -11.46382 galactic Cas Second-epoch detections are separated by 6.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:57:56.94 +50:30:33.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:57:56.94 +50:30:33.7: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:57:56.94 +50:30:33.7: 15.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 57 56.94 +50 30 33.7 13.1 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,2461225.8157,13.08,0.05,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 20260704.3157 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.09 00:20:04.14 +50:09:07.3
117.79601 -12.40665 galactic Cas Second-epoch detections are separated by 5.3" 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 J005.0247+50.1555 | 00:20:04.14 +50:09:07.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:20:04.14 +50:09:07.3: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:20:04.14 +50:09:07.3: 15.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 20 04.14 +50 09 07.3 13.1 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
ATO J005.0247+50.1555,2461225.8157,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J005.0247+50.1555 20260704.3157 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.22 23:56:53.46 +52:11:52.1
114.49967 -9.77863 galactic Cas Second-epoch detections are separated by 7.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J359.2427+52.1987 | 23:56:53.46 +52:11:52.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:56:53.46 +52:11:52.1: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:56:53.46 +52:11:52.1: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 56 53.46 +52 11 52.1 13.2 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 J359.2427+52.1987,2461225.8157,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.2427+52.1987 20260704.3157 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.15 23:57:55.85 +50:31:26.0
114.30090 -11.44901 galactic Cas Second-epoch detections are separated by 3.4" 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 | ATO J359.4669+50.5308 | 23:57:55.85 +50:31:26.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:57:55.85 +50:31:26.0: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:57:55.85 +50:31:26.0: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 57 55.85 +50 31 26.0 13.2 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 J359.4669+50.5308,2461225.8157,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.4669+50.5308 20260704.3157 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.25 23:56:32.61 +53:44:58.8
114.78280 -8.25127 galactic Cas Second-epoch detections are separated by 0.9" 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 J359.1339+53.7382 | 23:56:32.61 +53:44:58.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:56:32.61 +53:44:58.8: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:56:32.61 +53:44:58.8: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 56 32.61 +53 44 58.8 13.2 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 J359.1339+53.7382,2461225.8157,13.25,0.05,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 J359.1339+53.7382 20260704.3157 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.30 00:00:55.42 +50:46:23.5
114.82656 -11.30186 galactic Cas Second-epoch detections are separated by 3.5" 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 | target | 00:00:55.42 +50:46:23.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:00:55.42 +50:46:23.5: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:00:55.42 +50:46:23.5: 15.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 00 55.42 +50 46 23.5 13.3 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,2461225.8157,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.29 00:22:12.97 +52:14:13.4
118.39127 -10.37688 galactic Cas Second-epoch detections are separated by 2.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:12.97 +52:14:13.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:22:12.97 +52:14:13.4: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:22:12.97 +52:14:13.4: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 22 12.97 +52 14 13.4 13.3 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,2461225.8157,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.19 00:03:29.58 +49:57:53.4
115.07712 -12.17428 galactic Cas Second-epoch detections are separated by 4.9" 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 | target | 00:03:29.58 +49:57:53.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:03:29.58 +49:57:53.4: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:03:29.58 +49:57:53.4: 15.91 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 03 29.58 +49 57 53.4 13.2 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,2461225.8157,13.19,0.05,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 20260704.3157 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.54 23:48:59.83 +51:53:04.9
113.22791 -9.80669 galactic Cas Second-epoch detections are separated by 6.9" and 5.5 pix
The object was found in VSX17" Gaia DR3 1945022291281062912
Type: ROT
# Max. Min./Amp. JD0 Period
17.470 G 17.540 G K
ATTENTION: measured mag 13.54 is 3.9 mag brighter than the VSX record maximum brightness 17.47 - possible unusual activity of a known variable!
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:48:59.83 +51:53:04.9: 15.70 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:48:59.83 +51:53:04.9: 15.77 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.73 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 48 59.83 +51 53 04.9 13.5 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 1945022291281062912,2461225.8157,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1945022291281062912 20260704.3157 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.51 23:43:20.60 +54:07:09.5
112.96712 -7.42973 galactic Cas Second-epoch detections are separated by 5.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:43:20.60 +54:07:09.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:43:20.60 +54:07:09.5: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:43:20.60 +54:07:09.5: 15.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 43 20.60 +54 07 09.5 13.5 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,2461225.8157,13.51,0.05,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 20260704.3157 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.38 00:22:22.53 +53:06:10.9
118.51638 -9.51938 galactic Cas Second-epoch detections are separated by 8.9" 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 | 00:22:22.53 +53:06:10.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:22:22.53 +53:06:10.9: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:22:22.53 +53:06:10.9: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 22 22.53 +53 06 10.9 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461225.8157,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.68 23:57:00.82 +53:45:33.1
114.85347 -8.25673 galactic Cas Second-epoch detections are separated by 6.0" 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 | 23:57:00.82 +53:45:33.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:57:00.82 +53:45:33.1: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:57:00.82 +53:45:33.1: 15.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 57 00.82 +53 45 33.1 13.7 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
target,2461225.8157,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 12.26 00:02:01.42 +53:59:28.5
115.63150 -8.17860 galactic Cas Second-epoch detections are separated by 1.8" 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 | NSVS J0002034+535901 | 00:02:03.89 +53:58:58.7 (Gaia DR3) | SR (local) | 216.381785400000 (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:02:01.42 +53:59:28.5: 14.92 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:02:01.42 +53:59:28.5: 14.94 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.93 +/- 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 07 04.3157* 00 02 01.42 +53 59 28.5 12.3 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
NSVS J0002034+535901,2461225.8157,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0002034+535901 20260704.3157 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 7.77 23:58:25.81 +51:26:22.8
114.57400 -10.56983 galactic Cas Second-epoch detections are separated by 3.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:25.81 +51:26:22.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:58:25.81 +51:26:22.8: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:58:25.81 +51:26:22.8: 15.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 58 25.81 +51 26 22.8 7.8 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,2461225.8157,7.77,0.05,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 20260704.3157 7.77CV 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 07 04.3157 2461225.8157 11.93 00:18:27.78 +53:39:34.4
117.99830 -8.89602 galactic Cas Second-epoch detections are separated by 5.6" and 5.8 pix
The object was found in VSX21" Gaia DR3 419316321382504448
Type: ROT
# Max. Min./Amp. JD0 Period
16.900 G 17.050 G K
ATTENTION: measured mag 11.93 is 5.0 mag brighter than the VSX record maximum brightness 16.90 - possible unusual activity of a known variable!
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:18:27.78 +53:39:34.4: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:18:27.78 +53:39:34.4: 15.76 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 18 27.78 +53 39 34.4 11.9 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 419316321382504448,2461225.8157,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419316321382504448 20260704.3157 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 11.09 00:20:44.88 +50:11:52.7
117.91226 -12.37442 galactic Cas Second-epoch detections are separated by 1.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:20:44.88 +50:11:52.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:20:44.88 +50:11:52.7: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:20:44.88 +50:11:52.7: 15.83 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 20 44.88 +50 11 52.7 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,2461225.8157,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 11.26 00:11:07.91 +52:33:58.0
116.73580 -9.82006 galactic Cas Second-epoch detections are separated by 3.1" 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 | 00:11:07.91 +52:33:58.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:11:07.91 +52:33:58.0: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:11:07.91 +52:33:58.0: 15.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 11 07.91 +52 33 58.0 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,2461225.8157,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 11.65 23:35:01.60 +50:35:52.6
110.73682 -10.45567 galactic And Second-epoch detections are separated by 8.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:35:01.60 +50:35:52.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:35:01.60 +50:35:52.6: 15.63 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:35:01.60 +50:35:52.6: 15.64 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.63 +/- 0.36
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 35 01.60 +50 35 52.6 11.7 U And 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,2461225.8157,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 12.87 23:59:53.61 +56:58:39.7
115.92234 -5.19090 galactic Cas Second-epoch detections are separated by 7.0" and 5.5 pix
The object was found in VSX 9" V0533 Cas
Type: M
# Max. Min./Amp. JD0 Period
15.361 g Y 2.943 g 2458396.91440 296.168262100000 C(N)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:59:53.61 +56:58:39.7: 14.04 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:59:53.61 +56:58:39.7: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 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 07 04.3157* 23 59 53.61 +56 58 39.7 12.9 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
V0533 Cas,2461225.8157,12.87,0.05,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
V0533 Cas 20260704.3157 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 10.64 23:38:16.45 +56:01:55.4
112.78737 -5.39191 galactic Cas Second-epoch detections are separated by 4.3" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:38:16.45 +56:01:55.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:38:16.45 +56:01:55.4: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:38:16.45 +56:01:55.4: 15.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 23 38 16.45 +56 01 55.4 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,2461225.8157,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 13.23 00:13:23.75 +52:37:45.2
117.09039 -9.81051 galactic Cas Second-epoch detections are separated by 5.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:13:23.75 +52:37:45.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:13:23.75 +52:37:45.2: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:13:23.75 +52:37:45.2: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 13 23.75 +52 37 45.2 13.2 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,2461225.8157,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260704.3157 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 04.3157 2461225.8157 7.79 00:23:11.25 +55:47:39.7
118.93985 -6.85826 galactic Cas Second-epoch detections are separated by 0.8" and 5.7 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 | T Cas | 00:23:14.31 +55:47:33.1 (Gaia DR3) | M (local) | 443.500000000000 (local) | Gaia3var=VARIABLE SpType: M8e 1923ApJ....58..215M T Cas
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:23:11.25 +55:47:39.7: 9.94 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:23:11.25 +55:47:39.7: 9.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 04.3157* 00 23 11.25 +55 47 39.7 7.8 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
T Cas,2461225.8157,7.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
T Cas 20260704.3157 7.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.59778519 11.02.2026 02:20:38.640 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
First image: 2461082.59778519 11.02.2026 02:20:38.640 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Last image: 2461225.81596657 04.07.2026 07:34:49.512 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.78
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 22330
Objects passed selection criteria: 22209
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 15133.5
Average stars matched: 14104 (93.1972 %)
Memory usage VmPeak: 126848 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 3 15:05:03 CDT 2026
VaST build number 1.0rc89-123-g57107621
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 4 02:41:25 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: 2461082.59778519 11.02.2026 02:20:38.640 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
First image: 2461082.59778519 11.02.2026 02:20:38.640 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Last image: 2461225.81596657 04.07.2026 07:34:49.512 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 179
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
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: 96 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): 180339
Objects passed selection criteria: 179811
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 127787
Average stars matched: 117228 (91.7368 %)
Memory usage VmPeak: 1932004 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 3 15:05:03 CDT 2026
VaST build number 1.0rc89-123-g57107621
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 4 03:17:51 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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.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: 2461225.81543605
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits'
wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Image size: 941.8'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: 23:59:52.581 +53:59:29.78 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
Image size: 926.8'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:45.504 +54:01:37.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:52.581 +53:59:29.78
Second-epoch image center 23:59:45.504 +54:01:37.90
Angular distance between the image centers 0.0396 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Image size: 926.8'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:46.842 +54:02:09.45 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:52.581 +53:59:29.78
Second-epoch image center 23:59:46.842 +54:02:09.45
Angular distance between the image centers 0.0465 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:45.504 +54:01:37.90
Second-epoch second image center 23:59:46.842 +54:02:09.45
Angular distance between the image centers 0.00936 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits &> /tmp/tmp.q5D3SDwdhZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits &> /tmp/tmp.DrHGAD2Umt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits &> /tmp/tmp.8na7XnrJBq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits &> /tmp/tmp.yPy3oLzYsA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat' -> 'wcsmag.cat'
Read 29225 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9995 deg, Dec +47.7049 to +59.3705 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0002 to 359.9995 deg, Dec 47.7049 to 59.3705 deg
Loaded 162590 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): 14935 out of 16561 total matches.
Matched with Tycho-2 16561 out of 29225 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.842700
a=0.000000 b=1.000000 c=22.842700
From vast_summary.log: estimated ref. image limiting mag.: -7.78
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.06
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.06
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29225 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9995 deg, Dec +47.7049 to +59.3705 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0002 to 359.9995 deg, Dec 47.7049 to 59.3705 deg
Loaded 162590 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): 14935 out of 16561 total matches.
Matched with Tycho-2 16561 out of 29225 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits (aperture=6.0)
Read 29065 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0009 to 359.9998 deg, Dec +47.6373 to +59.3623 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0009 to 359.9998 deg, Dec 47.6373 to 59.3623 deg
Loaded 163448 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): 14807 out of 16429 total matches.
Matched with Tycho-2 16429 out of 29065 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
2.1 pix Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
2.1 pix wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
2.1 pix wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Limiting magnitude estimates:
15.1 mag. Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
15.1 mag. Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
13.9 mag. fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
13.9 mag. fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.q5D3SDwdhZ (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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3209, bad_region=7497, passed=29225
Got 29225 stars (including 19224 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
util/solve_plate_with_UCAC5 got 29225 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4494 through 0 to 15.3164, gap 15.3164 to 345.4494
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 22315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4506 through 0 to 15.3182, gap 15.3182 to 345.4506
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 22314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 22315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits N_match=973 sigma_overall_arcsec=0.484 sigma_q1_arcsec=0.551 sigma_q2_arcsec=0.430 sigma_q3_arcsec=0.487 sigma_q4_arcsec=0.426 n_q1=280 n_q2=198 n_q3=285 n_q4=210 worst_quadrant_to_overall_ratio=1.137
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits -region wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DrHGAD2Umt (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-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.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-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.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-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3195, bad_region=7496, passed=29065
Got 29065 stars (including 19086 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 29065 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4479 through 0 to 15.3165, gap 15.3165 to 345.4479
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 22203 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4487 through 0 to 15.3181, gap 15.3181 to 345.4487
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 22202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 22202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits N_match=972 sigma_overall_arcsec=0.506 sigma_q1_arcsec=0.539 sigma_q2_arcsec=0.430 sigma_q3_arcsec=0.560 sigma_q4_arcsec=0.425 n_q1=282 n_q2=199 n_q3=280 n_q4=211 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits -region wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8na7XnrJBq (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=750, bad_region=2272, passed=11045
Got 11045 stars (including 8147 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat
util/solve_plate_with_UCAC5 got 11045 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9619 through 0 to 14.7909, gap 14.7909 to 344.9619
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 327 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 237 matched stars entering correct_measured_positions(), 163 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 226 matched stars entering correct_measured_positions(), 2282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9488 through 0 to 14.8161, gap 14.8161 to 344.9488
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 404 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 339 matched stars entering correct_measured_positions(), 2337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.27"
Accuracy estimation diagnostic: 333 matched stars entering correct_measured_positions(), 3229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.90"
Excluding outliers - 333 stars left (next iteration limit 248)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits N_match=333 sigma_overall_arcsec=10.273 sigma_q1_arcsec=19.995 sigma_q2_arcsec=31.796 sigma_q3_arcsec=8.980 sigma_q4_arcsec=10.202 n_q1=32 n_q2=19 n_q3=124 n_q4=158 worst_quadrant_to_overall_ratio=3.095
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.yPy3oLzYsA (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=717, bad_region=2274, passed=11061
Got 11061 stars (including 8187 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat
util/solve_plate_with_UCAC5 got 11061 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9621 through 0 to 14.7906, gap 14.7906 to 344.9621
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 323 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 233 matched stars entering correct_measured_positions(), 159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 224 matched stars entering correct_measured_positions(), 2205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9485 through 0 to 14.8171, gap 14.8171 to 344.9485
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 399 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 342 matched stars entering correct_measured_positions(), 2266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.14"
Accuracy estimation diagnostic: 338 matched stars entering correct_measured_positions(), 3147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.80"
Excluding outliers - 338 stars left (next iteration limit 246)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits N_match=338 sigma_overall_arcsec=10.999 sigma_q1_arcsec=25.718 sigma_q2_arcsec=27.081 sigma_q3_arcsec=8.356 sigma_q4_arcsec=10.783 n_q1=37 n_q2=18 n_q3=126 n_q4=157 worst_quadrant_to_overall_ratio=2.462
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits sigma_overall=0.484 worst_q_ratio=1.137
ref2=Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits sigma_overall=0.506 worst_q_ratio=1.107
new1=fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits sigma_overall=10.273 worst_q_ratio=3.095
new2=fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits sigma_overall=10.999 worst_q_ratio=2.462
reference average sigma_overall=0.495 worst_q_ratio=1.122
warn-on-ratio threshold: 2.0x reference
###################################
WCS_QUALITY_RETRY: 1st new image (fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits) flagged: sigma=10.273 (ref avg 0.495), ratio=3.095 (ref avg 1.122), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/lib/make_outxyls_for_astrometric_calibration found 10612 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.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: "out1622709.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1622709.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 23.4803 (1.57526e+10), 7 match, 0 conflict, 18 distractors, 24 index.
RA,Dec = (359.937,54.0255), pixel scale 5.93178 arcsec/pix.
Hit/miss: Hit/miss: ----+-++-----+--+-+-----+(best)-------+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1622709.solved to indicate this.
Field: out1622709.xyls
Field center: (RA,Dec) = (359.938228, 54.026366) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:45.175, +54:01:34.916).
Field size: 15.6061 x 10.4338 degrees
Field rotation angle: up is 3.52246 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits' -> 'fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 4 02:49 fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
-rw-r--r-- 1 apache apache 8.5K Jul 4 02:49 out1622709.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits (fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.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: "out1622709.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1622709.axy"...
Only searching for solutions within 15.4467 degrees of RA,Dec (359.94,54.0272)
log-odds ratio 23.4803 (1.57526e+10), 7 match, 0 conflict, 18 distractors, 24 index.
RA,Dec = (359.937,54.0255), pixel scale 5.93178 arcsec/pix.
Hit/miss: Hit/miss: ----+-++-----+--+-+-----+(best)-------+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1622709.solved to indicate this.
Field: out1622709.xyls
Field center: (RA,Dec) = (359.938228, 54.026366) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:45.175, +54:01:34.916).
Field size: 15.6061 x 10.4338 degrees
Field rotation angle: up is 3.52246 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 4 02:49 fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
-rw-r--r-- 1 apache apache 8.5K Jul 4 02:49 out1622709.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.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-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 64152 sources.
Solving...
Reading file "./wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.axy"...
Verifying WCS using indices with quads of size [63.1537, 946.713] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
--> log-odds 10.6407
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
--> log-odds 8.42162
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
--> log-odds 6.4822
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
--> log-odds 4.407
Verifying WCS using indices with quads of size [63.1537, 946.713] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
--> log-odds 10.6407
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
--> log-odds 8.42162
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
--> log-odds 6.4822
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
--> log-odds 4.407
Got 0 solutions.
Field 1 did not solve (index index-5203-47.fits, field objects 1-10).
Field 1 did not solve (index index-5203-46.fits, field objects 1-10).
Field 1 did not solve (index index-5203-45.fits, field objects 1-10).
Field 1 did not solve (index index-5203-44.fits, field objects 1-10).
Field 1 did not solve (index index-5203-43.fits, field objects 1-10).
Field 1 did not solve (index index-5203-42.fits, field objects 1-10).
Field 1 did not solve (index index-5203-41.fits, field objects 1-10).
Field 1 did not solve (index index-5203-40.fits, field objects 1-10).
Field 1 did not solve (index index-5203-39.fits, field objects 1-10).
Field 1 did not solve (index index-5203-38.fits, field objects 1-10).
Field 1 did not solve (index index-5203-37.fits, field objects 1-10).
Field 1 did not solve (index index-5203-36.fits, field objects 1-10).
Field 1 did not solve (index index-5203-35.fits, field objects 1-10).
Field 1 did not solve (index index-5203-34.fits, field objects 1-10).
Field 1 did not solve (index index-5203-33.fits, field objects 1-10).
Field 1 did not solve (index index-5203-32.fits, field objects 1-10).
Field 1 did not solve (index index-5203-31.fits, field objects 1-10).
Field 1 did not solve (index index-5203-30.fits, field objects 1-10).
Field 1 did not solve (index index-5203-29.fits, field objects 1-10).
Field 1 did not solve (index index-5203-28.fits, field objects 1-10).
Field 1 did not solve (index index-5203-27.fits, field objects 1-10).
Field 1 did not solve (index index-5203-26.fits, field objects 1-10).
Field 1 did not solve (index index-5203-25.fits, field objects 1-10).
Field 1 did not solve (index index-5203-24.fits, field objects 1-10).
Field 1 did not solve (index index-5203-23.fits, field objects 1-10).
Field 1 did not solve (index index-5203-22.fits, field objects 1-10).
Field 1 did not solve (index index-5203-21.fits, field objects 1-10).
Field 1 did not solve (index index-5203-20.fits, field objects 1-10).
Field 1 did not solve (index index-5203-19.fits, field objects 1-10).
Field 1 did not solve (index index-5203-18.fits, field objects 1-10).
Field 1 did not solve (index index-5203-17.fits, field objects 1-10).
Field 1 did not solve (index index-5203-16.fits, field objects 1-10).
Field 1 did not solve (index index-5203-15.fits, field objects 1-10).
Field 1 did not solve (index index-5203-14.fits, field objects 1-10).
Field 1 did not solve (index index-5203-13.fits, field objects 1-10).
Field 1 did not solve (index index-5203-12.fits, field objects 1-10).
Field 1 did not solve (index index-5203-11.fits, field objects 1-10).
Field 1 did not solve (index index-5203-10.fits, field objects 1-10).
Field 1 did not solve (index index-5203-09.fits, field objects 1-10).
Field 1 did not solve (index index-5203-08.fits, field objects 1-10).
Field 1 did not solve (index index-5203-07.fits, field objects 1-10).
Field 1 did not solve (index index-5203-06.fits, field objects 1-10).
Field 1 did not solve (index index-5203-05.fits, field objects 1-10).
Field 1 did not solve (index index-5203-04.fits, field objects 1-10).
Field 1 did not solve (index index-5203-03.fits, field objects 1-10).
Field 1 did not solve (index index-5203-02.fits, field objects 1-10).
Field 1 did not solve (index index-5203-01.fits, field objects 1-10).
Field 1 did not solve (index index-5203-00.fits, field objects 1-10).
Field 1 did not solve (index index-5005-11.fits, field objects 1-10).
Field 1 did not solve (index index-5005-10.fits, field objects 1-10).
Field 1 did not solve (index index-5005-09.fits, field objects 1-10).
Field 1 did not solve (index index-5005-08.fits, field objects 1-10).
Field 1 did not solve (index index-5005-07.fits, field objects 1-10).
Field 1 did not solve (index index-5005-06.fits, field objects 1-10).
Field 1 did not solve (index index-5005-05.fits, field objects 1-10).
Field 1 did not solve (index index-5005-04.fits, field objects 1-10).
Field 1 did not solve (index index-5005-03.fits, field objects 1-10).
Field 1 did not solve (index index-5005-02.fits, field objects 1-10).
Field 1 did not solve (index index-5005-01.fits, field objects 1-10).
Field 1 did not solve (index index-5005-00.fits, field objects 1-10).
Field 1 did not solve (index index-4206-11.fits, field objects 1-10).
Field 1 did not solve (index index-4206-10.fits, field objects 1-10).
Field 1 did not solve (index index-4206-09.fits, field objects 1-10).
Field 1 did not solve (index index-4206-08.fits, field objects 1-10).
Field 1 did not solve (index index-4206-07.fits, field objects 1-10).
Field 1 did not solve (index index-4206-06.fits, field objects 1-10).
Field 1 did not solve (index index-4206-05.fits, field objects 1-10).
Field 1 did not solve (index index-4206-04.fits, field objects 1-10).
Field 1 did not solve (index index-4206-03.fits, field objects 1-10).
Field 1 did not solve (index index-4206-02.fits, field objects 1-10).
Field 1 did not solve (index index-4206-01.fits, field objects 1-10).
Field 1 did not solve (index index-4206-00.fits, field objects 1-10).
Field 1 did not solve (index index-4205-11.fits, field objects 1-10).
Field 1 did not solve (index index-4205-10.fits, field objects 1-10).
Field 1 did not solve (index index-4205-09.fits, field objects 1-10).
Field 1 did not solve (index index-4205-08.fits, field objects 1-10).
Field 1 did not solve (index index-4205-07.fits, field objects 1-10).
Field 1 did not solve (index index-4205-06.fits, field objects 1-10).
Field 1 did not solve (index index-4205-05.fits, field objects 1-10).
Field 1 did not solve (index index-4205-04.fits, field objects 1-10).
Field 1 did not solve (index index-4205-03.fits, field objects 1-10).
Field 1 did not solve (index index-4205-02.fits, field objects 1-10).
Field 1 did not solve (index index-4205-01.fits, field objects 1-10).
Field 1 did not solve (index index-4205-00.fits, field objects 1-10).
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
Field 1 did not solve (index index-4113.fits, field objects 1-10).
Field 1 did not solve (index index-4112.fits, field objects 1-10).
Field 1 did not solve (index index-4111.fits, field objects 1-10).
Field 1 did not solve (index index-4110.fits, field objects 1-10).
Field 1 did not solve (index index-4109.fits, field objects 1-10).
Field 1 did not solve (index index-4108.fits, field objects 1-10).
Field 1 did not solve (index index-4107.fits, field objects 1-10).
Field 1 did not solve (index index-204-11.fits, field objects 1-10).
Field 1 did not solve (index index-204-10.fits, field objects 1-10).
Field 1 did not solve (index index-204-09.fits, field objects 1-10).
Field 1 did not solve (index index-204-08.fits, field objects 1-10).
Field 1 did not solve (index index-204-07.fits, field objects 1-10).
Field 1 did not solve (index index-204-06.fits, field objects 1-10).
Field 1 did not solve (index index-204-05.fits, field objects 1-10).
Field 1 did not solve (index index-204-04.fits, field objects 1-10).
Field 1 did not solve (index index-204-03.fits, field objects 1-10).
Field 1 did not solve (index index-204-02.fits, field objects 1-10).
Field 1 did not solve (index index-204-01.fits, field objects 1-10).
Field 1 did not solve (index index-204-00.fits, field objects 1-10).
Field 1 did not solve (index index-5203-47.fits, field objects 11-20).
Field 1 did not solve (index index-5203-46.fits, field objects 11-20).
Field 1 did not solve (index index-5203-45.fits, field objects 11-20).
Field 1 did not solve (index index-5203-44.fits, field objects 11-20).
Field 1 did not solve (index index-5203-43.fits, field objects 11-20).
Field 1 did not solve (index index-5203-42.fits, field objects 11-20).
Field 1 did not solve (index index-5203-41.fits, field objects 11-20).
Field 1 did not solve (index index-5203-40.fits, field objects 11-20).
Field 1 did not solve (index index-5203-39.fits, field objects 11-20).
Field 1 did not solve (index index-5203-38.fits, field objects 11-20).
Field 1 did not solve (index index-5203-37.fits, field objects 11-20).
Field 1 did not solve (index index-5203-36.fits, field objects 11-20).
Field 1 did not solve (index index-5203-35.fits, field objects 11-20).
Field 1 did not solve (index index-5203-34.fits, field objects 11-20).
Field 1 did not solve (index index-5203-33.fits, field objects 11-20).
Field 1 did not solve (index index-5203-32.fits, field objects 11-20).
Field 1 did not solve (index index-5203-31.fits, field objects 11-20).
Field 1 did not solve (index index-5203-30.fits, field objects 11-20).
Field 1 did not solve (index index-5203-29.fits, field objects 11-20).
Field 1 did not solve (index index-5203-28.fits, field objects 11-20).
Field 1 did not solve (index index-5203-27.fits, field objects 11-20).
Field 1 did not solve (index index-5203-26.fits, field objects 11-20).
Field 1 did not solve (index index-5203-25.fits, field objects 11-20).
Field 1 did not solve (index index-5203-24.fits, field objects 11-20).
Field 1 did not solve (index index-5203-23.fits, field objects 11-20).
Field 1 did not solve (index index-5203-22.fits, field objects 11-20).
Field 1 did not solve (index index-5203-21.fits, field objects 11-20).
Field 1 did not solve (index index-5203-20.fits, field objects 11-20).
Field 1 did not solve (index index-5203-19.fits, field objects 11-20).
Field 1 did not solve (index index-5203-18.fits, field objects 11-20).
Field 1 did not solve (index index-5203-17.fits, field objects 11-20).
Field 1 did not solve (index index-5203-16.fits, field objects 11-20).
Field 1 did not solve (index index-5203-15.fits, field objects 11-20).
Field 1 did not solve (index index-5203-14.fits, field objects 11-20).
Field 1 did not solve (index index-5203-13.fits, field objects 11-20).
Field 1 did not solve (index index-5203-12.fits, field objects 11-20).
Field 1 did not solve (index index-5203-11.fits, field objects 11-20).
Field 1 did not solve (index index-5203-10.fits, field objects 11-20).
Field 1 did not solve (index index-5203-09.fits, field objects 11-20).
Field 1 did not solve (index index-5203-08.fits, field objects 11-20).
Field 1 did not solve (index index-5203-07.fits, field objects 11-20).
Field 1 did not solve (index index-5203-06.fits, field objects 11-20).
Field 1 did not solve (index index-5203-05.fits, field objects 11-20).
Field 1 did not solve (index index-5203-04.fits, field objects 11-20).
Field 1 did not solve (index index-5203-03.fits, field objects 11-20).
Field 1 did not solve (index index-5203-02.fits, field objects 11-20).
Field 1 did not solve (index index-5203-01.fits, field objects 11-20).
Field 1 did not solve (index index-5203-00.fits, field objects 11-20).
Field 1 did not solve (index index-5005-11.fits, field objects 11-20).
Field 1 did not solve (index index-5005-10.fits, field objects 11-20).
Field 1 did not solve (index index-5005-09.fits, field objects 11-20).
Field 1 did not solve (index index-5005-08.fits, field objects 11-20).
Field 1 did not solve (index index-5005-07.fits, field objects 11-20).
Field 1 did not solve (index index-5005-06.fits, field objects 11-20).
Field 1 did not solve (index index-5005-05.fits, field objects 11-20).
Field 1 did not solve (index index-5005-04.fits, field objects 11-20).
Field 1 did not solve (index index-5005-03.fits, field objects 11-20).
Field 1 did not solve (index index-5005-02.fits, field objects 11-20).
Field 1 did not solve (index index-5005-01.fits, field objects 11-20).
Field 1 did not solve (index index-5005-00.fits, field objects 11-20).
Field 1 did not solve (index index-4206-11.fits, field objects 11-20).
Field 1 did not solve (index index-4206-10.fits, field objects 11-20).
Field 1 did not solve (index index-4206-09.fits, field objects 11-20).
Field 1 did not solve (index index-4206-08.fits, field objects 11-20).
Field 1 did not solve (index index-4206-07.fits, field objects 11-20).
Field 1 did not solve (index index-4206-06.fits, field objects 11-20).
Field 1 did not solve (index index-4206-05.fits, field objects 11-20).
Field 1 did not solve (index index-4206-04.fits, field objects 11-20).
Field 1 did not solve (index index-4206-03.fits, field objects 11-20).
Field 1 did not solve (index index-4206-02.fits, field objects 11-20).
Field 1 did not solve (index index-4206-01.fits, field objects 11-20).
Field 1 did not solve (index index-4206-00.fits, field objects 11-20).
Field 1 did not solve (index index-4205-11.fits, field objects 11-20).
Field 1 did not solve (index index-4205-10.fits, field objects 11-20).
Field 1 did not solve (index index-4205-09.fits, field objects 11-20).
Field 1 did not solve (index index-4205-08.fits, field objects 11-20).
Field 1 did not solve (index index-4205-07.fits, field objects 11-20).
Field 1 did not solve (index index-4205-06.fits, field objects 11-20).
Field 1 did not solve (index index-4205-05.fits, field objects 11-20).
Field 1 did not solve (index index-4205-04.fits, field objects 11-20).
Field 1 did not solve (index index-4205-03.fits, field objects 11-20).
Field 1 did not solve (index index-4205-02.fits, field objects 11-20).
Field 1 did not solve (index index-4205-01.fits, field objects 11-20).
Field 1 did not solve (index index-4205-00.fits, field objects 11-20).
Field 1 did not solve (index index-4119.fits, field objects 11-20).
Field 1 did not solve (index index-4118.fits, field objects 11-20).
Field 1 did not solve (index index-4117.fits, field objects 11-20).
Field 1 did not solve (index index-4116.fits, field objects 11-20).
Field 1 did not solve (index index-4115.fits, field objects 11-20).
Field 1 did not solve (index index-4114.fits, field objects 11-20).
Field 1 did not solve (index index-4113.fits, field objects 11-20).
Field 1 did not solve (index index-4112.fits, field objects 11-20).
Field 1 did not solve (index index-4111.fits, field objects 11-20).
Field 1 did not solve (index index-4110.fits, field objects 11-20).
Field 1 did not solve (index index-4109.fits, field objects 11-20).
Field 1 did not solve (index index-4108.fits, field objects 11-20).
Field 1 did not solve (index index-4107.fits, field objects 11-20).
Field 1 did not solve (index index-204-11.fits, field objects 11-20).
Field 1 did not solve (index index-204-10.fits, field objects 11-20).
Field 1 did not solve (index index-204-09.fits, field objects 11-20).
Field 1 did not solve (index index-204-08.fits, field objects 11-20).
Field 1 did not solve (index index-204-07.fits, field objects 11-20).
Field 1 did not solve (index index-204-06.fits, field objects 11-20).
Field 1 did not solve (index index-204-05.fits, field objects 11-20).
Field 1 did not solve (index index-204-04.fits, field objects 11-20).
Field 1 did not solve (index index-204-03.fits, field objects 11-20).
Field 1 did not solve (index index-204-02.fits, field objects 11-20).
Field 1 did not solve (index index-204-01.fits, field objects 11-20).
Field 1 did not solve (index index-204-00.fits, field objects 11-20).
Field 1 did not solve (index index-5203-47.fits, field objects 21-30).
Field 1 did not solve (index index-5203-46.fits, field objects 21-30).
Field 1 did not solve (index index-5203-45.fits, field objects 21-30).
Field 1 did not solve (index index-5203-44.fits, field objects 21-30).
Field 1 did not solve (index index-5203-43.fits, field objects 21-30).
Field 1 did not solve (index index-5203-42.fits, field objects 21-30).
Field 1 did not solve (index index-5203-41.fits, field objects 21-30).
Field 1 did not solve (index index-5203-40.fits, field objects 21-30).
Field 1 did not solve (index index-5203-39.fits, field objects 21-30).
Field 1 did not solve (index index-5203-38.fits, field objects 21-30).
Field 1 did not solve (index index-5203-37.fits, field objects 21-30).
Field 1 did not solve (index index-5203-36.fits, field objects 21-30).
Field 1 did not solve (index index-5203-35.fits, field objects 21-30).
Field 1 did not solve (index index-5203-34.fits, field objects 21-30).
Field 1 did not solve (index index-5203-33.fits, field objects 21-30).
Field 1 did not solve (index index-5203-32.fits, field objects 21-30).
Field 1 did not solve (index index-5203-31.fits, field objects 21-30).
Field 1 did not solve (index index-5203-30.fits, field objects 21-30).
Field 1 did not solve (index index-5203-29.fits, field objects 21-30).
Field 1 did not solve (index index-5203-28.fits, field objects 21-30).
Field 1 did not solve (index index-5203-27.fits, field objects 21-30).
Field 1 did not solve (index index-5203-26.fits, field objects 21-30).
Field 1 did not solve (index index-5203-25.fits, field objects 21-30).
Field 1 did not solve (index index-5203-24.fits, field objects 21-30).
Field 1 did not solve (index index-5203-23.fits, field objects 21-30).
Field 1 did not solve (index index-5203-22.fits, field objects 21-30).
Field 1 did not solve (index index-5203-21.fits, field objects 21-30).
Field 1 did not solve (index index-5203-20.fits, field objects 21-30).
Field 1 did not solve (index index-5203-19.fits, field objects 21-30).
Field 1 did not solve (index index-5203-18.fits, field objects 21-30).
Field 1 did not solve (index index-5203-17.fits, field objects 21-30).
Field 1 did not solve (index index-5203-16.fits, field objects 21-30).
Field 1 did not solve (index index-5203-15.fits, field objects 21-30).
Field 1 did not solve (index index-5203-14.fits, field objects 21-30).
Field 1 did not solve (index index-5203-13.fits, field objects 21-30).
Field 1 did not solve (index index-5203-12.fits, field objects 21-30).
Field 1 did not solve (index index-5203-11.fits, field objects 21-30).
Field 1 did not solve (index index-5203-10.fits, field objects 21-30).
Field 1 did not solve (index index-5203-09.fits, field objects 21-30).
Field 1 did not solve (index index-5203-08.fits, field objects 21-30).
Field 1 did not solve (index index-5203-07.fits, field objects 21-30).
Field 1 did not solve (index index-5203-06.fits, field objects 21-30).
Field 1 did not solve (index index-5203-05.fits, field objects 21-30).
Field 1 did not solve (index index-5203-04.fits, field objects 21-30).
Field 1 did not solve (index index-5203-03.fits, field objects 21-30).
Field 1 did not solve (index index-5203-02.fits, field objects 21-30).
Field 1 did not solve (index index-5203-01.fits, field objects 21-30).
Field 1 did not solve (index index-5203-00.fits, field objects 21-30).
Field 1 did not solve (index index-5005-11.fits, field objects 21-30).
Field 1 did not solve (index index-5005-10.fits, field objects 21-30).
Field 1 did not solve (index index-5005-09.fits, field objects 21-30).
Field 1 did not solve (index index-5005-08.fits, field objects 21-30).
Field 1 did not solve (index index-5005-07.fits, field objects 21-30).
Field 1 did not solve (index index-5005-06.fits, field objects 21-30).
Field 1 did not solve (index index-5005-05.fits, field objects 21-30).
Field 1 did not solve (index index-5005-04.fits, field objects 21-30).
Field 1 did not solve (index index-5005-03.fits, field objects 21-30).
Field 1 did not solve (index index-5005-02.fits, field objects 21-30).
Field 1 did not solve (index index-5005-01.fits, field objects 21-30).
Field 1 did not solve (index index-5005-00.fits, field objects 21-30).
Field 1 did not solve (index index-4206-11.fits, field objects 21-30).
Field 1 did not solve (index index-4206-10.fits, field objects 21-30).
Field 1 did not solve (index index-4206-09.fits, field objects 21-30).
Field 1 did not solve (index index-4206-08.fits, field objects 21-30).
Field 1 did not solve (index index-4206-07.fits, field objects 21-30).
Field 1 did not solve (index index-4206-06.fits, field objects 21-30).
Field 1 did not solve (index index-4206-05.fits, field objects 21-30).
Field 1 did not solve (index index-4206-04.fits, field objects 21-30).
Field 1 did not solve (index index-4206-03.fits, field objects 21-30).
Field 1 did not solve (index index-4206-02.fits, field objects 21-30).
Field 1 did not solve (index index-4206-01.fits, field objects 21-30).
Field 1 did not solve (index index-4206-00.fits, field objects 21-30).
Field 1 did not solve (index index-4205-11.fits, field objects 21-30).
Field 1 did not solve (index index-4205-10.fits, field objects 21-30).
Field 1 did not solve (index index-4205-09.fits, field objects 21-30).
Field 1 did not solve (index index-4205-08.fits, field objects 21-30).
Field 1 did not solve (index index-4205-07.fits, field objects 21-30).
Field 1 did not solve (index index-4205-06.fits, field objects 21-30).
Field 1 did not solve (index index-4205-05.fits, field objects 21-30).
Field 1 did not solve (index index-4205-04.fits, field objects 21-30).
Field 1 did not solve (index index-4205-03.fits, field objects 21-30).
Field 1 did not solve (index index-4205-02.fits, field objects 21-30).
Field 1 did not solve (index index-4205-01.fits, field objects 21-30).
Field 1 did not solve (index index-4205-00.fits, field objects 21-30).
Field 1 did not solve (index index-4119.fits, field objects 21-30).
Field 1 did not solve (index index-4118.fits, field objects 21-30).
Field 1 did not solve (index index-4117.fits, field objects 21-30).
Field 1 did not solve (index index-4116.fits, field objects 21-30).
Field 1 did not solve (index index-4115.fits, field objects 21-30).
Total CPU time limit reached!
Field 1 did not solve (index index-4114.fits, field objects 21-30).
Field: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
Did not solve (or no WCS file was written).
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
Generating wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat from image00003.cat
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits created.
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
Image size: 926.8'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:45.504 +54:01:37.90 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 11045 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/correct_sextractor_wcs_catalog_usingxy2sky1952156.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=750, bad_region=2272, passed=11045
Got 11045 stars (including 8147 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat
util/solve_plate_with_UCAC5 got 11045 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9619 through 0 to 14.7909, gap 14.7909 to 344.9619
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 327 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 237 matched stars entering correct_measured_positions(), 163 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 226 matched stars entering correct_measured_positions(), 2282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9488 through 0 to 14.8161, gap 14.8161 to 344.9488
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 404 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 339 matched stars entering correct_measured_positions(), 2337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.27"
Accuracy estimation diagnostic: 333 matched stars entering correct_measured_positions(), 3229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.90"
Excluding outliers - 333 stars left (next iteration limit 248)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits N_match=333 sigma_overall_arcsec=10.273 sigma_q1_arcsec=19.995 sigma_q2_arcsec=31.796 sigma_q3_arcsec=8.980 sigma_q4_arcsec=10.202 n_q1=32 n_q2=19 n_q3=124 n_q4=158 worst_quadrant_to_overall_ratio=3.095
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 1st new image (fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits): sigma 10.273->10.273, ratio 3.095->3.095; reverting to order 3
WCS_QUALITY_RETRY: 2nd new image (fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits) flagged: sigma=10.999 (ref avg 0.495), ratio=2.462 (ref avg 1.122), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits .... Determining astrometry method...
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_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/lib/make_outxyls_for_astrometric_calibration found 10642 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.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: "out1952759.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1952759.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 24.6638 (5.14452e+10), 7 match, 0 conflict, 18 distractors, 24 index.
RA,Dec = (359.942,54.0343), pixel scale 5.93186 arcsec/pix.
Hit/miss: Hit/miss: ----+++--------++-+-----+(best)-------+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1952759.solved to indicate this.
Field: out1952759.xyls
Field center: (RA,Dec) = (359.943800, 54.035131) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:46.512, +54:02:06.471).
Field size: 15.6065 x 10.4342 degrees
Field rotation angle: up is 3.52249 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits' -> 'fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 4 03:00 fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
-rw-r--r-- 1 apache apache 8.5K Jul 4 03:00 out1952759.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits (fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.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: "out1952759.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1952759.axy"...
Only searching for solutions within 15.4467 degrees of RA,Dec (359.945,54.036)
log-odds ratio 24.6638 (5.14452e+10), 7 match, 0 conflict, 18 distractors, 24 index.
RA,Dec = (359.942,54.0343), pixel scale 5.93186 arcsec/pix.
Hit/miss: Hit/miss: ----+++--------++-+-----+(best)-------+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1952759.solved to indicate this.
Field: out1952759.xyls
Field center: (RA,Dec) = (359.943800, 54.035131) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:46.512, +54:02:06.471).
Field size: 15.6065 x 10.4342 degrees
Field rotation angle: up is 3.52249 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 4 03:00 fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
-rw-r--r-- 1 apache apache 8.5K Jul 4 03:00 out1952759.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.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-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 64114 sources.
Solving...
Reading file "./wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.axy"...
Verifying WCS using indices with quads of size [63.1545, 946.724] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS using indices with quads of size [63.1545, 946.724] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
--> log-odds 0
Got 0 solutions.
Field 1 did not solve (index index-5203-47.fits, field objects 1-10).
Field 1 did not solve (index index-5203-46.fits, field objects 1-10).
Field 1 did not solve (index index-5203-45.fits, field objects 1-10).
Field 1 did not solve (index index-5203-44.fits, field objects 1-10).
Field 1 did not solve (index index-5203-43.fits, field objects 1-10).
Field 1 did not solve (index index-5203-42.fits, field objects 1-10).
Field 1 did not solve (index index-5203-41.fits, field objects 1-10).
Field 1 did not solve (index index-5203-40.fits, field objects 1-10).
Field 1 did not solve (index index-5203-39.fits, field objects 1-10).
Field 1 did not solve (index index-5203-38.fits, field objects 1-10).
Field 1 did not solve (index index-5203-37.fits, field objects 1-10).
Field 1 did not solve (index index-5203-36.fits, field objects 1-10).
Field 1 did not solve (index index-5203-35.fits, field objects 1-10).
Field 1 did not solve (index index-5203-34.fits, field objects 1-10).
Field 1 did not solve (index index-5203-33.fits, field objects 1-10).
Field 1 did not solve (index index-5203-32.fits, field objects 1-10).
Field 1 did not solve (index index-5203-31.fits, field objects 1-10).
Field 1 did not solve (index index-5203-30.fits, field objects 1-10).
Field 1 did not solve (index index-5203-29.fits, field objects 1-10).
Field 1 did not solve (index index-5203-28.fits, field objects 1-10).
Field 1 did not solve (index index-5203-27.fits, field objects 1-10).
Field 1 did not solve (index index-5203-26.fits, field objects 1-10).
Field 1 did not solve (index index-5203-25.fits, field objects 1-10).
Field 1 did not solve (index index-5203-24.fits, field objects 1-10).
Field 1 did not solve (index index-5203-23.fits, field objects 1-10).
Field 1 did not solve (index index-5203-22.fits, field objects 1-10).
Field 1 did not solve (index index-5203-21.fits, field objects 1-10).
Field 1 did not solve (index index-5203-20.fits, field objects 1-10).
Field 1 did not solve (index index-5203-19.fits, field objects 1-10).
Field 1 did not solve (index index-5203-18.fits, field objects 1-10).
Field 1 did not solve (index index-5203-17.fits, field objects 1-10).
Field 1 did not solve (index index-5203-16.fits, field objects 1-10).
Field 1 did not solve (index index-5203-15.fits, field objects 1-10).
Field 1 did not solve (index index-5203-14.fits, field objects 1-10).
Field 1 did not solve (index index-5203-13.fits, field objects 1-10).
Field 1 did not solve (index index-5203-12.fits, field objects 1-10).
Field 1 did not solve (index index-5203-11.fits, field objects 1-10).
Field 1 did not solve (index index-5203-10.fits, field objects 1-10).
Field 1 did not solve (index index-5203-09.fits, field objects 1-10).
Field 1 did not solve (index index-5203-08.fits, field objects 1-10).
Field 1 did not solve (index index-5203-07.fits, field objects 1-10).
Field 1 did not solve (index index-5203-06.fits, field objects 1-10).
Field 1 did not solve (index index-5203-05.fits, field objects 1-10).
Field 1 did not solve (index index-5203-04.fits, field objects 1-10).
Field 1 did not solve (index index-5203-03.fits, field objects 1-10).
Field 1 did not solve (index index-5203-02.fits, field objects 1-10).
Field 1 did not solve (index index-5203-01.fits, field objects 1-10).
Field 1 did not solve (index index-5203-00.fits, field objects 1-10).
Field 1 did not solve (index index-5005-11.fits, field objects 1-10).
Field 1 did not solve (index index-5005-10.fits, field objects 1-10).
Field 1 did not solve (index index-5005-09.fits, field objects 1-10).
Field 1 did not solve (index index-5005-08.fits, field objects 1-10).
Field 1 did not solve (index index-5005-07.fits, field objects 1-10).
Field 1 did not solve (index index-5005-06.fits, field objects 1-10).
Field 1 did not solve (index index-5005-05.fits, field objects 1-10).
Field 1 did not solve (index index-5005-04.fits, field objects 1-10).
Field 1 did not solve (index index-5005-03.fits, field objects 1-10).
Field 1 did not solve (index index-5005-02.fits, field objects 1-10).
Field 1 did not solve (index index-5005-01.fits, field objects 1-10).
Field 1 did not solve (index index-5005-00.fits, field objects 1-10).
Field 1 did not solve (index index-4206-11.fits, field objects 1-10).
Field 1 did not solve (index index-4206-10.fits, field objects 1-10).
Field 1 did not solve (index index-4206-09.fits, field objects 1-10).
Field 1 did not solve (index index-4206-08.fits, field objects 1-10).
Field 1 did not solve (index index-4206-07.fits, field objects 1-10).
Field 1 did not solve (index index-4206-06.fits, field objects 1-10).
Field 1 did not solve (index index-4206-05.fits, field objects 1-10).
Field 1 did not solve (index index-4206-04.fits, field objects 1-10).
Field 1 did not solve (index index-4206-03.fits, field objects 1-10).
Field 1 did not solve (index index-4206-02.fits, field objects 1-10).
Field 1 did not solve (index index-4206-01.fits, field objects 1-10).
Field 1 did not solve (index index-4206-00.fits, field objects 1-10).
Field 1 did not solve (index index-4205-11.fits, field objects 1-10).
Field 1 did not solve (index index-4205-10.fits, field objects 1-10).
Field 1 did not solve (index index-4205-09.fits, field objects 1-10).
Field 1 did not solve (index index-4205-08.fits, field objects 1-10).
Field 1 did not solve (index index-4205-07.fits, field objects 1-10).
Field 1 did not solve (index index-4205-06.fits, field objects 1-10).
Field 1 did not solve (index index-4205-05.fits, field objects 1-10).
Field 1 did not solve (index index-4205-04.fits, field objects 1-10).
Field 1 did not solve (index index-4205-03.fits, field objects 1-10).
Field 1 did not solve (index index-4205-02.fits, field objects 1-10).
Field 1 did not solve (index index-4205-01.fits, field objects 1-10).
Field 1 did not solve (index index-4205-00.fits, field objects 1-10).
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
Field 1 did not solve (index index-4113.fits, field objects 1-10).
Field 1 did not solve (index index-4112.fits, field objects 1-10).
Field 1 did not solve (index index-4111.fits, field objects 1-10).
Field 1 did not solve (index index-4110.fits, field objects 1-10).
Field 1 did not solve (index index-4109.fits, field objects 1-10).
Field 1 did not solve (index index-4108.fits, field objects 1-10).
Field 1 did not solve (index index-4107.fits, field objects 1-10).
Field 1 did not solve (index index-204-11.fits, field objects 1-10).
Field 1 did not solve (index index-204-10.fits, field objects 1-10).
Field 1 did not solve (index index-204-09.fits, field objects 1-10).
Field 1 did not solve (index index-204-08.fits, field objects 1-10).
Field 1 did not solve (index index-204-07.fits, field objects 1-10).
Field 1 did not solve (index index-204-06.fits, field objects 1-10).
Field 1 did not solve (index index-204-05.fits, field objects 1-10).
Field 1 did not solve (index index-204-04.fits, field objects 1-10).
Field 1 did not solve (index index-204-03.fits, field objects 1-10).
Field 1 did not solve (index index-204-02.fits, field objects 1-10).
Field 1 did not solve (index index-204-01.fits, field objects 1-10).
Field 1 did not solve (index index-204-00.fits, field objects 1-10).
Field 1 did not solve (index index-5203-47.fits, field objects 11-20).
Field 1 did not solve (index index-5203-46.fits, field objects 11-20).
Field 1 did not solve (index index-5203-45.fits, field objects 11-20).
Field 1 did not solve (index index-5203-44.fits, field objects 11-20).
Field 1 did not solve (index index-5203-43.fits, field objects 11-20).
Field 1 did not solve (index index-5203-42.fits, field objects 11-20).
Field 1 did not solve (index index-5203-41.fits, field objects 11-20).
Field 1 did not solve (index index-5203-40.fits, field objects 11-20).
Field 1 did not solve (index index-5203-39.fits, field objects 11-20).
Field 1 did not solve (index index-5203-38.fits, field objects 11-20).
Field 1 did not solve (index index-5203-37.fits, field objects 11-20).
Field 1 did not solve (index index-5203-36.fits, field objects 11-20).
Field 1 did not solve (index index-5203-35.fits, field objects 11-20).
Field 1 did not solve (index index-5203-34.fits, field objects 11-20).
Field 1 did not solve (index index-5203-33.fits, field objects 11-20).
Field 1 did not solve (index index-5203-32.fits, field objects 11-20).
Field 1 did not solve (index index-5203-31.fits, field objects 11-20).
Field 1 did not solve (index index-5203-30.fits, field objects 11-20).
Field 1 did not solve (index index-5203-29.fits, field objects 11-20).
Field 1 did not solve (index index-5203-28.fits, field objects 11-20).
Field 1 did not solve (index index-5203-27.fits, field objects 11-20).
Field 1 did not solve (index index-5203-26.fits, field objects 11-20).
Field 1 did not solve (index index-5203-25.fits, field objects 11-20).
Field 1 did not solve (index index-5203-24.fits, field objects 11-20).
Field 1 did not solve (index index-5203-23.fits, field objects 11-20).
Field 1 did not solve (index index-5203-22.fits, field objects 11-20).
Field 1 did not solve (index index-5203-21.fits, field objects 11-20).
Field 1 did not solve (index index-5203-20.fits, field objects 11-20).
Field 1 did not solve (index index-5203-19.fits, field objects 11-20).
Field 1 did not solve (index index-5203-18.fits, field objects 11-20).
Field 1 did not solve (index index-5203-17.fits, field objects 11-20).
Field 1 did not solve (index index-5203-16.fits, field objects 11-20).
Field 1 did not solve (index index-5203-15.fits, field objects 11-20).
Field 1 did not solve (index index-5203-14.fits, field objects 11-20).
Field 1 did not solve (index index-5203-13.fits, field objects 11-20).
Field 1 did not solve (index index-5203-12.fits, field objects 11-20).
Field 1 did not solve (index index-5203-11.fits, field objects 11-20).
Field 1 did not solve (index index-5203-10.fits, field objects 11-20).
Field 1 did not solve (index index-5203-09.fits, field objects 11-20).
Field 1 did not solve (index index-5203-08.fits, field objects 11-20).
Field 1 did not solve (index index-5203-07.fits, field objects 11-20).
Field 1 did not solve (index index-5203-06.fits, field objects 11-20).
Field 1 did not solve (index index-5203-05.fits, field objects 11-20).
Field 1 did not solve (index index-5203-04.fits, field objects 11-20).
Field 1 did not solve (index index-5203-03.fits, field objects 11-20).
Field 1 did not solve (index index-5203-02.fits, field objects 11-20).
Field 1 did not solve (index index-5203-01.fits, field objects 11-20).
Field 1 did not solve (index index-5203-00.fits, field objects 11-20).
Field 1 did not solve (index index-5005-11.fits, field objects 11-20).
Field 1 did not solve (index index-5005-10.fits, field objects 11-20).
Field 1 did not solve (index index-5005-09.fits, field objects 11-20).
Field 1 did not solve (index index-5005-08.fits, field objects 11-20).
Field 1 did not solve (index index-5005-07.fits, field objects 11-20).
Field 1 did not solve (index index-5005-06.fits, field objects 11-20).
Field 1 did not solve (index index-5005-05.fits, field objects 11-20).
Field 1 did not solve (index index-5005-04.fits, field objects 11-20).
Field 1 did not solve (index index-5005-03.fits, field objects 11-20).
Field 1 did not solve (index index-5005-02.fits, field objects 11-20).
Field 1 did not solve (index index-5005-01.fits, field objects 11-20).
Field 1 did not solve (index index-5005-00.fits, field objects 11-20).
Field 1 did not solve (index index-4206-11.fits, field objects 11-20).
Field 1 did not solve (index index-4206-10.fits, field objects 11-20).
Field 1 did not solve (index index-4206-09.fits, field objects 11-20).
Field 1 did not solve (index index-4206-08.fits, field objects 11-20).
Field 1 did not solve (index index-4206-07.fits, field objects 11-20).
Field 1 did not solve (index index-4206-06.fits, field objects 11-20).
Field 1 did not solve (index index-4206-05.fits, field objects 11-20).
Field 1 did not solve (index index-4206-04.fits, field objects 11-20).
Field 1 did not solve (index index-4206-03.fits, field objects 11-20).
Field 1 did not solve (index index-4206-02.fits, field objects 11-20).
Field 1 did not solve (index index-4206-01.fits, field objects 11-20).
Field 1 did not solve (index index-4206-00.fits, field objects 11-20).
Field 1 did not solve (index index-4205-11.fits, field objects 11-20).
Field 1 did not solve (index index-4205-10.fits, field objects 11-20).
Field 1 did not solve (index index-4205-09.fits, field objects 11-20).
Field 1 did not solve (index index-4205-08.fits, field objects 11-20).
Field 1 did not solve (index index-4205-07.fits, field objects 11-20).
Field 1 did not solve (index index-4205-06.fits, field objects 11-20).
Field 1 did not solve (index index-4205-05.fits, field objects 11-20).
Field 1 did not solve (index index-4205-04.fits, field objects 11-20).
Field 1 did not solve (index index-4205-03.fits, field objects 11-20).
Field 1 did not solve (index index-4205-02.fits, field objects 11-20).
Field 1 did not solve (index index-4205-01.fits, field objects 11-20).
Field 1 did not solve (index index-4205-00.fits, field objects 11-20).
Field 1 did not solve (index index-4119.fits, field objects 11-20).
Field 1 did not solve (index index-4118.fits, field objects 11-20).
Field 1 did not solve (index index-4117.fits, field objects 11-20).
Field 1 did not solve (index index-4116.fits, field objects 11-20).
Field 1 did not solve (index index-4115.fits, field objects 11-20).
Field 1 did not solve (index index-4114.fits, field objects 11-20).
Field 1 did not solve (index index-4113.fits, field objects 11-20).
Field 1 did not solve (index index-4112.fits, field objects 11-20).
Field 1 did not solve (index index-4111.fits, field objects 11-20).
Field 1 did not solve (index index-4110.fits, field objects 11-20).
Field 1 did not solve (index index-4109.fits, field objects 11-20).
Field 1 did not solve (index index-4108.fits, field objects 11-20).
Field 1 did not solve (index index-4107.fits, field objects 11-20).
Field 1 did not solve (index index-204-11.fits, field objects 11-20).
Field 1 did not solve (index index-204-10.fits, field objects 11-20).
Field 1 did not solve (index index-204-09.fits, field objects 11-20).
Field 1 did not solve (index index-204-08.fits, field objects 11-20).
Field 1 did not solve (index index-204-07.fits, field objects 11-20).
Field 1 did not solve (index index-204-06.fits, field objects 11-20).
Field 1 did not solve (index index-204-05.fits, field objects 11-20).
Field 1 did not solve (index index-204-04.fits, field objects 11-20).
Field 1 did not solve (index index-204-03.fits, field objects 11-20).
Field 1 did not solve (index index-204-02.fits, field objects 11-20).
Field 1 did not solve (index index-204-01.fits, field objects 11-20).
Field 1 did not solve (index index-204-00.fits, field objects 11-20).
Field 1 did not solve (index index-5203-47.fits, field objects 21-30).
Field 1 did not solve (index index-5203-46.fits, field objects 21-30).
Field 1 did not solve (index index-5203-45.fits, field objects 21-30).
Field 1 did not solve (index index-5203-44.fits, field objects 21-30).
Field 1 did not solve (index index-5203-43.fits, field objects 21-30).
Field 1 did not solve (index index-5203-42.fits, field objects 21-30).
Field 1 did not solve (index index-5203-41.fits, field objects 21-30).
Field 1 did not solve (index index-5203-40.fits, field objects 21-30).
Field 1 did not solve (index index-5203-39.fits, field objects 21-30).
Field 1 did not solve (index index-5203-38.fits, field objects 21-30).
Field 1 did not solve (index index-5203-37.fits, field objects 21-30).
Field 1 did not solve (index index-5203-36.fits, field objects 21-30).
Field 1 did not solve (index index-5203-35.fits, field objects 21-30).
Field 1 did not solve (index index-5203-34.fits, field objects 21-30).
Field 1 did not solve (index index-5203-33.fits, field objects 21-30).
Field 1 did not solve (index index-5203-32.fits, field objects 21-30).
Field 1 did not solve (index index-5203-31.fits, field objects 21-30).
Field 1 did not solve (index index-5203-30.fits, field objects 21-30).
Field 1 did not solve (index index-5203-29.fits, field objects 21-30).
Field 1 did not solve (index index-5203-28.fits, field objects 21-30).
Field 1 did not solve (index index-5203-27.fits, field objects 21-30).
Field 1 did not solve (index index-5203-26.fits, field objects 21-30).
Field 1 did not solve (index index-5203-25.fits, field objects 21-30).
Field 1 did not solve (index index-5203-24.fits, field objects 21-30).
Field 1 did not solve (index index-5203-23.fits, field objects 21-30).
Field 1 did not solve (index index-5203-22.fits, field objects 21-30).
Field 1 did not solve (index index-5203-21.fits, field objects 21-30).
Field 1 did not solve (index index-5203-20.fits, field objects 21-30).
Field 1 did not solve (index index-5203-19.fits, field objects 21-30).
Field 1 did not solve (index index-5203-18.fits, field objects 21-30).
Field 1 did not solve (index index-5203-17.fits, field objects 21-30).
Field 1 did not solve (index index-5203-16.fits, field objects 21-30).
Field 1 did not solve (index index-5203-15.fits, field objects 21-30).
Field 1 did not solve (index index-5203-14.fits, field objects 21-30).
Field 1 did not solve (index index-5203-13.fits, field objects 21-30).
Field 1 did not solve (index index-5203-12.fits, field objects 21-30).
Field 1 did not solve (index index-5203-11.fits, field objects 21-30).
Field 1 did not solve (index index-5203-10.fits, field objects 21-30).
Field 1 did not solve (index index-5203-09.fits, field objects 21-30).
Field 1 did not solve (index index-5203-08.fits, field objects 21-30).
Field 1 did not solve (index index-5203-07.fits, field objects 21-30).
Field 1 did not solve (index index-5203-06.fits, field objects 21-30).
Field 1 did not solve (index index-5203-05.fits, field objects 21-30).
Field 1 did not solve (index index-5203-04.fits, field objects 21-30).
Field 1 did not solve (index index-5203-03.fits, field objects 21-30).
Field 1 did not solve (index index-5203-02.fits, field objects 21-30).
Field 1 did not solve (index index-5203-01.fits, field objects 21-30).
Field 1 did not solve (index index-5203-00.fits, field objects 21-30).
Field 1 did not solve (index index-5005-11.fits, field objects 21-30).
Field 1 did not solve (index index-5005-10.fits, field objects 21-30).
Field 1 did not solve (index index-5005-09.fits, field objects 21-30).
Field 1 did not solve (index index-5005-08.fits, field objects 21-30).
Field 1 did not solve (index index-5005-07.fits, field objects 21-30).
Field 1 did not solve (index index-5005-06.fits, field objects 21-30).
Field 1 did not solve (index index-5005-05.fits, field objects 21-30).
Field 1 did not solve (index index-5005-04.fits, field objects 21-30).
Field 1 did not solve (index index-5005-03.fits, field objects 21-30).
Field 1 did not solve (index index-5005-02.fits, field objects 21-30).
Field 1 did not solve (index index-5005-01.fits, field objects 21-30).
Field 1 did not solve (index index-5005-00.fits, field objects 21-30).
Field 1 did not solve (index index-4206-11.fits, field objects 21-30).
Field 1 did not solve (index index-4206-10.fits, field objects 21-30).
Field 1 did not solve (index index-4206-09.fits, field objects 21-30).
Field 1 did not solve (index index-4206-08.fits, field objects 21-30).
Field 1 did not solve (index index-4206-07.fits, field objects 21-30).
Field 1 did not solve (index index-4206-06.fits, field objects 21-30).
Field 1 did not solve (index index-4206-05.fits, field objects 21-30).
Field 1 did not solve (index index-4206-04.fits, field objects 21-30).
Field 1 did not solve (index index-4206-03.fits, field objects 21-30).
Field 1 did not solve (index index-4206-02.fits, field objects 21-30).
Field 1 did not solve (index index-4206-01.fits, field objects 21-30).
Field 1 did not solve (index index-4206-00.fits, field objects 21-30).
Field 1 did not solve (index index-4205-11.fits, field objects 21-30).
Field 1 did not solve (index index-4205-10.fits, field objects 21-30).
Field 1 did not solve (index index-4205-09.fits, field objects 21-30).
Field 1 did not solve (index index-4205-08.fits, field objects 21-30).
Field 1 did not solve (index index-4205-07.fits, field objects 21-30).
Field 1 did not solve (index index-4205-06.fits, field objects 21-30).
Field 1 did not solve (index index-4205-05.fits, field objects 21-30).
Field 1 did not solve (index index-4205-04.fits, field objects 21-30).
Field 1 did not solve (index index-4205-03.fits, field objects 21-30).
Field 1 did not solve (index index-4205-02.fits, field objects 21-30).
Field 1 did not solve (index index-4205-01.fits, field objects 21-30).
Field 1 did not solve (index index-4205-00.fits, field objects 21-30).
Field 1 did not solve (index index-4119.fits, field objects 21-30).
Field 1 did not solve (index index-4118.fits, field objects 21-30).
Field 1 did not solve (index index-4117.fits, field objects 21-30).
Field 1 did not solve (index index-4116.fits, field objects 21-30).
Field 1 did not solve (index index-4115.fits, field objects 21-30).
Total CPU time limit reached!
Field 1 did not solve (index index-4114.fits, field objects 21-30).
Field: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Did not solve (or no WCS file was written).
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Generating wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat from image00004.cat
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits created.
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Image size: 926.8'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:46.842 +54:02:09.45 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 11061 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/correct_sextractor_wcs_catalog_usingxy2sky2402258.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=717, bad_region=2274, passed=11061
Got 11061 stars (including 8187 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat
util/solve_plate_with_UCAC5 got 11061 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9621 through 0 to 14.7906, gap 14.7906 to 344.9621
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 323 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 233 matched stars entering correct_measured_positions(), 159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 224 matched stars entering correct_measured_positions(), 2205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9485 through 0 to 14.8171, gap 14.8171 to 344.9485
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 399 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 342 matched stars entering correct_measured_positions(), 2266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.14"
Accuracy estimation diagnostic: 338 matched stars entering correct_measured_positions(), 3147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.80"
Excluding outliers - 338 stars left (next iteration limit 246)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits N_match=338 sigma_overall_arcsec=10.999 sigma_q1_arcsec=25.718 sigma_q2_arcsec=27.081 sigma_q3_arcsec=8.356 sigma_q4_arcsec=10.783 n_q1=37 n_q2=18 n_q3=126 n_q4=157 worst_quadrant_to_overall_ratio=2.462
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 2nd new image (fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits): sigma 10.999->10.999, ratio 2.462->2.462; reverting to order 3
WARNING: 1st new image has sigma_overall_arcsec=10.273 -- 20.75x the reference average (0.495); plate solution may be of low accuracy
WARNING: 2nd new image has sigma_overall_arcsec=10.999 -- 22.22x the reference average (0.495); plate solution may be of low accuracy
WARNING: 1st new image has worst_quadrant_to_overall_ratio=3.095 -- 2.76x the reference average (1.122); plate solution may be of low accuracy
WARNING: 2nd new image has worst_quadrant_to_overall_ratio=2.462 -- 2.19x the reference average (1.122); plate solution may be of low accuracy
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006_astrometric_residuals.png (973 matched stars from wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007_astrometric_residuals.png (972 matched stars from wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302_astrometric_residuals.png (333 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 4.10 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303_astrometric_residuals.png (338 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.72 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:04:40.61 +55:32:17.7: 14.33 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:20:46.10 +50:11:50.5: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:58:26.78 +51:26:16.1: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:23:11.80 +55:47:31.5: 9.14 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:20:46.10 +50:11:50.5: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:58:26.78 +51:26:16.1: 15.50 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:04:40.61 +55:32:17.7: 14.24 +/- 0.09 detection
Forced photometry reference-image weighted average: 15.50 +/- 0.34
Forced photometry reference-image weighted average: 14.28 +/- 0.07
Forced photometry filter KEPT candidate at 23:58:26.78 +51:26:16.1: ref_mag=15.50 +/- 0.34 new_mean_mag=7.3843 delta=8.11 (need > 0.90)
Forced photometry filter KEPT candidate at 00:04:40.61 +55:32:17.7: ref_mag=14.28 +/- 0.07 new_mean_mag=10.0159 delta=4.27 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:23:11.80 +55:47:31.5: 9.18 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.16 +/- 0.00
Forced photometry filter KEPT candidate at 00:23:11.80 +55:47:31.5: ref_mag=9.16 +/- 0.00 new_mean_mag=7.4860 delta=1.68 (need > 0.90)
Adding exclusion_list_local.txt__out08367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33121.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32048_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 32048_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32426_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 32426_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:55:50.55 +53:44:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32438_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 32438_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:44:31.65 +56:34:50.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33121_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 33121_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33651_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 33651_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33675_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 33675_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 00:06:02.16 +55:12:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09534_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 09534_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21888_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 21888_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08367_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 08367_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18981_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 18981_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 23s
Prepared the HTML report for the field Cas-04-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 ####
00:23:11.80 +55:47:31.5
23:58:26.78 +51:26:16.1
00:04:40.61 +55:32:17.7
00:20:46.10 +50:11:50.5
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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Image size: 941.8'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: 23:59:52.581 +53:59:29.78 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
Image size: 926.8'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:45.504 +54:01:37.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:52.581 +53:59:29.78
Second-epoch image center 23:59:45.504 +54:01:37.90
Angular distance between the image centers 0.0396 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Image size: 926.8'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:46.842 +54:02:09.45 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:52.581 +53:59:29.78
Second-epoch image center 23:59:46.842 +54:02:09.45
Angular distance between the image centers 0.0465 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:45.504 +54:01:37.90
Second-epoch second image center 23:59:46.842 +54:02:09.45
Angular distance between the image centers 0.00936 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits &> /tmp/tmp.GGDs4QTFcI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits &> /tmp/tmp.4twyArqDS7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits &> /tmp/tmp.J3UdtqdfkK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits &> /tmp/tmp.IAiCtvGGhB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat' -> 'wcsmag.cat'
Read 217609 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9999 deg, Dec +47.6392 to +59.3793 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0001 to 359.9999 deg, Dec 47.6392 to 59.3793 deg
Loaded 163629 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): 11705 out of 17839 total matches.
Matched with Tycho-2 17839 out of 217609 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.676500
a=0.000000 b=1.000000 c=22.676500
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 217609 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9999 deg, Dec +47.6392 to +59.3793 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0001 to 359.9999 deg, Dec 47.6392 to 59.3793 deg
Loaded 163629 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): 11705 out of 17839 total matches.
Matched with Tycho-2 17839 out of 217609 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits (aperture=4.4)
Read 217552 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9999 deg, Dec +47.6349 to +59.3691 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0001 to 359.9999 deg, Dec 47.6349 to 59.3691 deg
Loaded 163556 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): 11613 out of 17712 total matches.
Matched with Tycho-2 17712 out of 217552 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 159 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
1.9 pix Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
1.9 pix wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
1.9 pix wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Limiting magnitude estimates:
15.3 mag. Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
15.3 mag. Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
14.0 mag. fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
14.0 mag. fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.GGDs4QTFcI (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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.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-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=32857, bad_region=42414, passed=217571
Got 217571 stars (including 147921 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
util/solve_plate_with_UCAC5 got 217571 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4355 through 0 to 15.4567, gap 15.4567 to 345.4355
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
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: 971 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 179159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4369 through 0 to 15.4586, gap 15.4586 to 345.4369
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
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: 971 matched stars entering correct_measured_positions(), 179160 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 179161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits N_match=971 sigma_overall_arcsec=0.474 sigma_q1_arcsec=0.568 sigma_q2_arcsec=0.428 sigma_q3_arcsec=0.484 sigma_q4_arcsec=0.397 n_q1=296 n_q2=177 n_q3=309 n_q4=189 worst_quadrant_to_overall_ratio=1.196
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits -region wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4twyArqDS7 (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-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.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-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.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-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=32499, bad_region=42352, passed=217519
Got 217519 stars (including 148225 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 217519 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4449 through 0 to 15.4097, gap 15.4097 to 345.4449
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 179634 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4458 through 0 to 15.4120, gap 15.4120 to 345.4458
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 179634 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 179635 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits N_match=973 sigma_overall_arcsec=0.506 sigma_q1_arcsec=0.566 sigma_q2_arcsec=0.449 sigma_q3_arcsec=0.521 sigma_q4_arcsec=0.419 n_q1=298 n_q2=185 n_q3=304 n_q4=186 worst_quadrant_to_overall_ratio=1.118
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits -region wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.J3UdtqdfkK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=6943, bad_region=11063, passed=92627
Got 92627 stars (including 75756 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat
util/solve_plate_with_UCAC5 got 92627 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9311 through 0 to 14.8937, gap 14.8937 to 344.9311
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 325 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 240 matched stars entering correct_measured_positions(), 162 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 228 matched stars entering correct_measured_positions(), 23330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.00"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9212 through 0 to 14.9207, gap 14.9207 to 344.9212
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 397 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 325 matched stars entering correct_measured_positions(), 23375 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.99"
Accuracy estimation diagnostic: 324 matched stars entering correct_measured_positions(), 31075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.04"
Excluding outliers - 324 stars left (next iteration limit 250)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits N_match=324 sigma_overall_arcsec=9.321 sigma_q1_arcsec=24.458 sigma_q2_arcsec=24.290 sigma_q3_arcsec=6.037 sigma_q4_arcsec=8.593 n_q1=42 n_q2=21 n_q3=121 n_q4=140 worst_quadrant_to_overall_ratio=2.624
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.IAiCtvGGhB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=6872, bad_region=11108, passed=92772
Got 92772 stars (including 75919 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat
util/solve_plate_with_UCAC5 got 92772 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9622 through 0 to 14.8803, gap 14.8803 to 344.9622
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 325 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 242 matched stars entering correct_measured_positions(), 163 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.16"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 232 matched stars entering correct_measured_positions(), 24550 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9524 through 0 to 14.9073, gap 14.9073 to 344.9524
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 388 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 323 matched stars entering correct_measured_positions(), 24592 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.29"
Accuracy estimation diagnostic: 322 matched stars entering correct_measured_positions(), 31194 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.42"
Excluding outliers - 322 stars left (next iteration limit 255)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits N_match=322 sigma_overall_arcsec=9.572 sigma_q1_arcsec=31.372 sigma_q2_arcsec=25.478 sigma_q3_arcsec=6.397 sigma_q4_arcsec=9.440 n_q1=37 n_q2=25 n_q3=125 n_q4=135 worst_quadrant_to_overall_ratio=3.278
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-03_20.00sec_4.90C_LIGHT_0302.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-04_CI_Cas-04-Q2b1x1_023534_TTUQ2b1x1_924889_ZYUIJiBB/wcs_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:49:33.10 +57:52:51.6: 13.92 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:36:23.82 +53:17:52.2: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:06:46.16 +53:36:36.3: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:59:28.42 +55:04:58.0: 13.61 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:29:20.51 +56:41:07.2: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:55:24.21 +51:47:36.3: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:48:04.74 +57:46:38.3: 12.99 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:04:18.55 +51:51:34.0: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:36:23.82 +53:17:52.2: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:49:33.10 +57:52:51.6: 13.73 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:06:46.16 +53:36:36.3: 15.96 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry filter REJECTED candidate at 23:49:33.10 +57:52:51.6: ref_mag=13.81 +/- 0.04 new_mean_mag=13.6595 delta=0.15 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:45:58.30 +56:53:27.4: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:29:20.51 +56:41:07.2: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:55:24.21 +51:47:36.3: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:59:28.42 +55:04:58.0: 13.58 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:48:04.74 +57:46:38.3: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:04:18.55 +51:51:34.0: 15.75 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter REJECTED candidate at 23:59:28.42 +55:04:58.0: ref_mag=13.60 +/- 0.03 new_mean_mag=13.3070 delta=0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:48:04.74 +57:46:38.3: ref_mag=13.02 +/- 0.02 new_mean_mag=13.2711 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:45:58.30 +56:53:27.4: 13.18 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Forced photometry filter REJECTED candidate at 23:45:58.30 +56:53:27.4: ref_mag=13.10 +/- 0.03 new_mean_mag=13.0140 delta=0.09 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:01:22.43 +56:07:44.6: 12.49 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:54:49.94 +56:15:42.2: 12.62 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:47:40.51 +56:15:45.8: 11.89 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:01:22.43 +56:07:44.6: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter REJECTED candidate at 00:01:22.43 +56:07:44.6: ref_mag=12.44 +/- 0.01 new_mean_mag=12.8439 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:54:49.94 +56:15:42.2: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:47:40.51 +56:15:45.8: 11.99 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 23:54:49.94 +56:15:42.2: ref_mag=12.61 +/- 0.01 new_mean_mag=12.5891 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry filter REJECTED candidate at 23:47:40.51 +56:15:45.8: ref_mag=11.93 +/- 0.01 new_mean_mag=12.7342 delta=-0.80 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:23:24.19 +54:55:49.4: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:42:59.05 +52:41:50.6: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:59:15.49 +55:57:37.4: 12.00 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:38:45.92 +56:37:01.5: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:23:24.19 +54:55:49.4: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:42:59.05 +52:41:50.6: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:59:15.49 +55:57:37.4: 11.99 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:38:45.92 +56:37:01.5: 9.37 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 23:38:45.92 +56:37:01.5: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter REJECTED candidate at 23:59:15.49 +55:57:37.4: ref_mag=11.99 +/- 0.01 new_mean_mag=11.9142 delta=0.08 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:46:41.23 +54:28:38.1: 13.06 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:14:53.52 +53:15:51.3: 14.35 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:46:41.23 +54:28:38.1: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 23:46:41.23 +54:28:38.1: ref_mag=13.11 +/- 0.02 new_mean_mag=11.8067 delta=1.30 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:44:10.21 +56:38:08.1: 12.08 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:14:53.52 +53:15:51.3: 14.22 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.07
Forced photometry filter KEPT candidate at 00:14:53.52 +53:15:51.3: ref_mag=14.28 +/- 0.07 new_mean_mag=11.7418 delta=2.54 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:44:10.21 +56:38:08.1: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter REJECTED candidate at 23:44:10.21 +56:38:08.1: ref_mag=12.09 +/- 0.01 new_mean_mag=12.1940 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:59:20.52 +50:35:47.9: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:59:20.52 +50:35:47.9: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:33:26.05 +52:55:09.4: 12.65 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:33:26.05 +52:55:09.4: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.02
Forced photometry filter REJECTED candidate at 23:33:26.05 +52:55:09.4: ref_mag=12.61 +/- 0.02 new_mean_mag=12.3599 delta=0.25 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:22:43.72 +57:06:28.2: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:22:43.72 +57:06:28.2: 13.09 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter REJECTED candidate at 00:22:43.72 +57:06:28.2: ref_mag=13.07 +/- 0.02 new_mean_mag=12.4450 delta=0.62 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:23:00.46 +55:45:43.2: 14.90 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:23:00.46 +55:45:43.2: 15.05 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.16
Forced photometry filter KEPT candidate at 00:23:00.46 +55:45:43.2: ref_mag=14.98 +/- 0.16 new_mean_mag=12.3948 delta=2.58 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:54:35.75 +57:28:17.1: 12.72 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:54:35.75 +57:28:17.1: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Forced photometry filter REJECTED candidate at 23:54:35.75 +57:28:17.1: ref_mag=12.74 +/- 0.02 new_mean_mag=12.5741 delta=0.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:16:25.12 +53:58:17.8: 15.29 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:31:40.65 +49:36:15.0: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:16:25.12 +53:58:17.8: 15.19 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.14
Forced photometry filter KEPT candidate at 00:16:25.12 +53:58:17.8: ref_mag=15.23 +/- 0.14 new_mean_mag=12.6450 delta=2.59 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:31:40.65 +49:36:15.0: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:59:19.39 +55:58:47.5: 12.91 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:59:19.39 +55:58:47.5: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter REJECTED candidate at 23:59:19.39 +55:58:47.5: ref_mag=12.91 +/- 0.02 new_mean_mag=12.7336 delta=0.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:03:20.27 +55:39:11.8: 12.66 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:57:55.26 +56:28:26.2: 12.13 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:03:20.27 +55:39:11.8: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter REJECTED candidate at 00:03:20.27 +55:39:11.8: ref_mag=12.66 +/- 0.02 new_mean_mag=12.8081 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:36:25.20 +55:17:30.9: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:57:55.26 +56:28:26.2: 12.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.02
Forced photometry filter REJECTED candidate at 23:57:55.26 +56:28:26.2: ref_mag=12.13 +/- 0.02 new_mean_mag=12.8339 delta=-0.70 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:36:25.20 +55:17:30.9: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:49:54.89 +53:28:41.6: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:41:52.97 +52:45:15.2: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:43:28.34 +50:59:01.0: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:49:54.89 +53:28:41.6: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:41:52.97 +52:45:15.2: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:23:22.81 +55:49:22.8: 14.66 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:03:11.05 +55:41:50.2: 12.80 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:43:28.34 +50:59:01.0: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:23:22.81 +55:49:22.8: 14.88 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.11
Forced photometry filter KEPT candidate at 00:23:22.81 +55:49:22.8: ref_mag=14.75 +/- 0.11 new_mean_mag=12.9635 delta=1.78 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:03:11.05 +55:41:50.2: 12.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry filter REJECTED candidate at 00:03:11.05 +55:41:50.2: ref_mag=12.81 +/- 0.02 new_mean_mag=13.0025 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:10:23.32 +49:55:14.2: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:26:19.63 +56:46:42.6: 13.07 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:10:23.32 +49:55:14.2: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:26:19.63 +56:46:42.6: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Forced photometry filter REJECTED candidate at 00:26:19.63 +56:46:42.6: ref_mag=13.09 +/- 0.03 new_mean_mag=12.8947 delta=0.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:57:56.94 +50:30:33.7: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:57:56.94 +50:30:33.7: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:24:35.80 +56:58:54.0: 13.30 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:24:35.80 +56:58:54.0: 13.31 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.04
Forced photometry filter REJECTED candidate at 00:24:35.80 +56:58:54.0: ref_mag=13.31 +/- 0.04 new_mean_mag=12.9801 delta=0.33 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:00:12.98 +55:43:04.5: 12.97 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:00:12.98 +55:43:04.5: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter REJECTED candidate at 00:00:12.98 +55:43:04.5: ref_mag=13.01 +/- 0.02 new_mean_mag=13.0356 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:56:18.54 +56:44:43.2: 12.94 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:56:18.54 +56:44:43.2: 12.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.03
Forced photometry filter REJECTED candidate at 23:56:18.54 +56:44:43.2: ref_mag=12.95 +/- 0.03 new_mean_mag=13.0724 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:21:03.17 +57:36:48.1: 13.47 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:21:03.17 +57:36:48.1: 13.35 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry filter REJECTED candidate at 00:21:03.17 +57:36:48.1: ref_mag=13.41 +/- 0.03 new_mean_mag=13.0674 delta=0.34 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:49:46.60 +56:38:29.9: 13.24 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:49:46.60 +56:38:29.9: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry filter REJECTED candidate at 23:49:46.60 +56:38:29.9: ref_mag=13.31 +/- 0.03 new_mean_mag=13.2056 delta=0.11 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:19:15.20 +57:46:01.4: 13.03 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:00:22.23 +56:51:45.1: 12.80 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:19:15.20 +57:46:01.4: 13.09 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Forced photometry filter REJECTED candidate at 00:19:15.20 +57:46:01.4: ref_mag=13.06 +/- 0.03 new_mean_mag=13.1248 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:00:22.23 +56:51:45.1: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter REJECTED candidate at 00:00:22.23 +56:51:45.1: ref_mag=12.84 +/- 0.02 new_mean_mag=13.1476 delta=-0.30 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:13:37.08 +56:24:42.7: 13.18 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:13:37.08 +56:24:42.7: 13.23 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Forced photometry filter REJECTED candidate at 00:13:37.08 +56:24:42.7: ref_mag=13.21 +/- 0.03 new_mean_mag=13.0850 delta=0.12 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:41:19.18 +57:33:44.9: 13.04 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:20:04.14 +50:09:07.3: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:41:19.18 +57:33:44.9: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry filter REJECTED candidate at 23:41:19.18 +57:33:44.9: ref_mag=13.08 +/- 0.03 new_mean_mag=13.1834 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:20:04.14 +50:09:07.3: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:56:53.46 +52:11:52.1: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:56:53.46 +52:11:52.1: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:57:55.85 +50:31:26.0: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:57:55.85 +50:31:26.0: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:05:11.14 +57:46:29.9: 12.94 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:56:32.61 +53:44:58.8: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:05:11.14 +57:46:29.9: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter REJECTED candidate at 00:05:11.14 +57:46:29.9: ref_mag=12.93 +/- 0.02 new_mean_mag=13.1123 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:03:22.34 +58:09:11.8: 13.34 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:56:32.61 +53:44:58.8: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:00:55.42 +50:46:23.5: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:03:22.34 +58:09:11.8: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter REJECTED candidate at 00:03:22.34 +58:09:11.8: ref_mag=13.38 +/- 0.03 new_mean_mag=13.2800 delta=0.10 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:00:55.42 +50:46:23.5: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:40:54.21 +57:50:52.2: 13.36 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:22:12.97 +52:14:13.4: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:40:54.21 +57:50:52.2: 13.50 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter REJECTED candidate at 23:40:54.21 +57:50:52.2: ref_mag=13.43 +/- 0.03 new_mean_mag=13.3533 delta=0.07 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:03:29.58 +49:57:53.4: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:22:12.97 +52:14:13.4: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:03:29.58 +49:57:53.4: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:11:54.25 +57:16:15.3: 13.60 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:11:54.25 +57:16:15.3: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Forced photometry filter REJECTED candidate at 00:11:54.25 +57:16:15.3: ref_mag=13.63 +/- 0.04 new_mean_mag=13.2732 delta=0.35 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:51:13.64 +56:34:50.8: 13.75 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:51:13.64 +56:34:50.8: 13.73 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter REJECTED candidate at 23:51:13.64 +56:34:50.8: ref_mag=13.74 +/- 0.04 new_mean_mag=13.4479 delta=0.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:48:59.83 +51:53:04.9: 15.70 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:48:59.83 +51:53:04.9: 15.77 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.73 +/- 0.22
Forced photometry filter KEPT candidate at 23:48:59.83 +51:53:04.9: ref_mag=15.73 +/- 0.22 new_mean_mag=13.5308 delta=2.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:43:20.60 +54:07:09.5: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:42:20.49 +57:04:49.5: 13.49 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:43:20.60 +54:07:09.5: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:42:20.49 +57:04:49.5: 13.49 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter REJECTED candidate at 23:42:20.49 +57:04:49.5: ref_mag=13.49 +/- 0.03 new_mean_mag=13.4644 delta=0.02 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:22:22.53 +53:06:10.9: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:22:22.53 +53:06:10.9: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:57:00.82 +53:45:33.1: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:57:00.82 +53:45:33.1: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:50:24.10 +54:13:22.2: 14.78 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:51:57.97 +56:02:28.6: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:50:24.10 +54:13:22.2: 14.79 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.10
Forced photometry filter KEPT candidate at 23:50:24.10 +54:13:22.2: ref_mag=14.78 +/- 0.10 new_mean_mag=13.7708 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:51:57.97 +56:02:28.6: 15.56 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.56 +/- 0.29
Forced photometry filter KEPT candidate at 23:51:57.97 +56:02:28.6: ref_mag=15.56 +/- 0.29 new_mean_mag=13.9893 delta=1.57 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:02:01.42 +53:59:28.5: 14.92 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:02:01.42 +53:59:28.5: 14.94 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.10
Forced photometry filter KEPT candidate at 00:02:01.42 +53:59:28.5: ref_mag=14.93 +/- 0.10 new_mean_mag=12.2538 delta=2.67 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:58:25.81 +51:26:22.8: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:58:25.81 +51:26:22.8: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:18:27.78 +53:39:34.4: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:18:27.78 +53:39:34.4: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:44:31.44 +56:34:47.4: 13.52 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:44:31.44 +56:34:47.4: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Forced photometry filter KEPT candidate at 23:44:31.44 +56:34:47.4: ref_mag=13.52 +/- 0.03 new_mean_mag=10.8027 delta=2.72 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:20:44.88 +50:11:52.7: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:20:44.88 +50:11:52.7: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:11:07.91 +52:33:58.0: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:11:07.91 +52:33:58.0: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:35:01.60 +50:35:52.6: 15.63 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:35:01.60 +50:35:52.6: 15.64 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.63 +/- 0.36
Forced photometry filter KEPT candidate at 23:35:01.60 +50:35:52.6: ref_mag=15.63 +/- 0.36 new_mean_mag=11.6489 delta=3.98 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:59:53.61 +56:58:39.7: 14.04 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:38:16.45 +56:01:55.4: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:59:53.61 +56:58:39.7: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Forced photometry filter KEPT candidate at 23:59:53.61 +56:58:39.7: ref_mag=13.95 +/- 0.04 new_mean_mag=12.8663 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:38:16.45 +56:01:55.4: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:13:23.75 +52:37:45.2: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:13:23.75 +52:37:45.2: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:23:11.25 +55:47:39.7: 9.94 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:23:11.25 +55:47:39.7: 9.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.96 +/- 0.01
Forced photometry filter KEPT candidate at 00:23:11.25 +55:47:39.7: ref_mag=9.96 +/- 0.01 new_mean_mag=7.7917 delta=2.17 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out266870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out267158.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out117774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out256099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out256441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out256657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out256670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out259171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out259355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out259617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out259640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71796.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 67s
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: 26s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243667_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243667_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243669_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243669_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243677_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243677_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243678_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243678_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243681_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 243681_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243684_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243684_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (36.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243697_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243697_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243702_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243702_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:54:56.82 +56:12:37.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243704_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 243704_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243705_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243705_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243707_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 243707_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243708_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243708_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243713_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243713_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243714_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 243714_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243719_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 243719_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243722_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243722_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243727_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243727_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243731_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243731_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243732_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243732_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243734_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243734_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243735_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243735_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243736_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243736_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 00:03:08.12 +57:26:59.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243737_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243737_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243739_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243739_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243740_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243740_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (28.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243742_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243742_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243744_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243744_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (34.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243745_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243745_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (39.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243748_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 243748_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243749_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 243749_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243750_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243750_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243751_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 243751_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245710_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 245710_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246242_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 246242_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 00:06:02.18 +55:11:55.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246949_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 246949_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247543_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 247543_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247674_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 247674_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247937_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 247937_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:39:37.73 +57:07:31.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249185_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 249185_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250435_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 250435_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250548_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 250548_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250815_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 250815_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251104_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 251104_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:42:05.15 +57:16:05.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251253_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 251253_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251363_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 251363_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251896_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 251896_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252057_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 252057_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 00:24:07.08 +52:01:07.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252102_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 252102_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:55:16.87 +58:06:28.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252143_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 252143_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:43:56.08 +56:20:00.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252385_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 252385_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:59:25.36 +57:41:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252813_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 252813_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252834_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 252834_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253317_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 253317_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253468_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 253468_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:42:06.50 +57:15:35.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253552_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 253552_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:47:14.02 +57:25:42.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254035_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 254035_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254099_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 254099_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254218_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 254218_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 00:25:45.95 +57:58:56.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254777_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 254777_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:56:19.49 +55:11:15.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254935_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 254935_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255489_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 255489_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255514_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 255514_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255536_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 255536_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 00:21:18.61 +57:37:43.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255819_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 255819_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 00:31:46.90 +56:53:34.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255836_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 255836_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256099_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 256099_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256159_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 256159_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256441_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 256441_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256657_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 256657_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256669_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 256669_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256670_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 256670_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256671_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 256671_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257132_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 257132_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257188_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 257188_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 00:02:35.86 +55:35:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257262_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 257262_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257316_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 257316_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257443_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 257443_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257522_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 257522_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257559_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 257559_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257683_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 257683_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257755_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 257755_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257768_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 257768_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257796_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 257796_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257944_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 257944_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:54:26.99 +55:07:27.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257946_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 257946_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258072_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 258072_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (28.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258141_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 258141_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258152_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 258152_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258213_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 258213_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258279_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 258279_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 00:05:42.10 +58:17:40.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258287_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 258287_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258390_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 258390_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:56:58.27 +55:42:24.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258538_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 258538_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258642_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 258642_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258649_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 258649_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258845_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 258845_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258862_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 258862_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:57:15.69 +56:30:02.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258925_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 258925_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259169_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 259169_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259171_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 259171_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259261_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 259261_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259270_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 259270_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259355_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 259355_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259378_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 259378_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259599_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 259599_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259603_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 259603_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:58:51.34 +54:42:06.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259617_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 259617_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259640_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 259640_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259701_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 259701_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (47.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259803_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 259803_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:50:37.29 +57:09:26.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259870_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 259870_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260264_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 260264_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260327_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 260327_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260503_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 260503_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260522_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 260522_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260569_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 260569_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260590_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 260590_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260969_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 260969_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (28.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260997_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 260997_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261173_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 261173_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261217_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 261217_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (25.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261280_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 261280_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261686_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 261686_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261913_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 261913_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261945_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 261945_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262384_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 262384_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262386_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 262386_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262392_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 262392_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262684_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 262684_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:54:49.86 +56:11:34.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262772_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 262772_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262909_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 262909_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262919_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 262919_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263001_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 263001_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263079_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 263079_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263606_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 263606_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (28.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263786_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 263786_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264133_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 264133_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265042_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 265042_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265186_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 265186_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265577_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 265577_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265954_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 265954_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 00:08:36.88 +55:38:46.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266210_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 266210_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266870_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 266870_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:50:24.10 +54:13:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 4.174 1993729629901668608 357.60222553701 +54.22235815179 14.5747 13.7970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267158_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 267158_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:51:57.97 +56:02:28.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117774_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 117774_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174810_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 174810_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130430_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 130430_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:50:44.80 +53:34:43.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119320_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 119320_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79234_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 79234_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 00:04:40.98 +55:32:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58579_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 58579_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 23:44:31.44 +56:34:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)GAIADR2_OUTPUT=# 5.734 1997999342783263104 356.13172697795 +56.58137488816 9.5919 8.0380 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179137_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 179137_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146843_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 146843_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177194_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 177194_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195948_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 195948_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (49.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125040_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
The candidate 125040_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46239_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 46239_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71796_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 71796_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143637_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 143637_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69970_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
Preparing report for the candidate 69970_fd_Cas-04-Q2b1x1_2026-07-04_02-34-49_20.00sec_5.00C_LIGHT_0303
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 97s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:23:11.80 +55:47:31.5
23:58:26.78 +51:26:16.1
00:04:40.61 +55:32:17.7
00:20:46.10 +50:11:50.5
00:02:01.42 +53:59:28.5
00:18:27.78 +53:39:34.4
00:13:23.75 +52:37:45.2
00:11:07.91 +52:33:58.0
23:58:25.81 +51:26:22.8
23:35:01.60 +50:35:52.6
00:20:44.88 +50:11:52.7
00:06:46.16 +53:36:36.3
23:36:23.82 +53:17:52.2
00:04:18.55 +51:51:34.0
23:29:20.51 +56:41:07.2
23:55:24.21 +51:47:36.3
00:23:24.19 +54:55:49.4
23:42:59.05 +52:41:50.6
23:46:41.23 +54:28:38.1
00:14:53.52 +53:15:51.3
23:59:20.52 +50:35:47.9
00:23:00.46 +55:45:43.2
00:16:25.12 +53:58:17.8
23:31:40.65 +49:36:15.0
23:36:25.20 +55:17:30.9
23:49:54.89 +53:28:41.6
23:41:52.97 +52:45:15.2
23:43:28.34 +50:59:01.0
00:23:22.81 +55:49:22.8
00:10:23.32 +49:55:14.2
23:57:56.94 +50:30:33.7
00:20:04.14 +50:09:07.3
23:56:53.46 +52:11:52.1
23:57:55.85 +50:31:26.0
23:56:32.61 +53:44:58.8
00:00:55.42 +50:46:23.5
00:22:12.97 +52:14:13.4
00:03:29.58 +49:57:53.4
23:48:59.83 +51:53:04.9
23:43:20.60 +54:07:09.5
00:22:22.53 +53:06:10.9
23:57:00.82 +53:45:33.1
23:59:53.61 +56:58:39.7
00:23:11.25 +55:47:39.7
23:38:16.45 +56:01:55.4
########### Completed Cas-04-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 ####
00:04:40.61 +55:32:17.7
00:20:46.10 +50:11:50.5
23:58:26.78 +51:26:16.1
00:23:11.80 +55:47:31.5
00:06:46.16 +53:36:36.3
23:36:23.82 +53:17:52.2
00:04:18.55 +51:51:34.0
23:29:20.51 +56:41:07.2
23:55:24.21 +51:47:36.3
00:23:24.19 +54:55:49.4
23:42:59.05 +52:41:50.6
23:46:41.23 +54:28:38.1
00:14:53.52 +53:15:51.3
23:59:20.52 +50:35:47.9
00:23:00.46 +55:45:43.2
00:16:25.12 +53:58:17.8
23:31:40.65 +49:36:15.0
23:36:25.20 +55:17:30.9
23:49:54.89 +53:28:41.6
23:41:52.97 +52:45:15.2
23:43:28.34 +50:59:01.0
00:23:22.81 +55:49:22.8
00:10:23.32 +49:55:14.2
23:57:56.94 +50:30:33.7
00:20:04.14 +50:09:07.3
23:56:53.46 +52:11:52.1
23:57:55.85 +50:31:26.0
23:56:32.61 +53:44:58.8
00:00:55.42 +50:46:23.5
00:22:12.97 +52:14:13.4
00:03:29.58 +49:57:53.4
23:48:59.83 +51:53:04.9
23:43:20.60 +54:07:09.5
00:22:22.53 +53:06:10.9
23:57:00.82 +53:45:33.1
00:02:01.42 +53:59:28.5
23:58:25.81 +51:26:22.8
00:18:27.78 +53:39:34.4
00:20:44.88 +50:11:52.7
00:11:07.91 +52:33:58.0
23:35:01.60 +50:35:52.6
23:59:53.61 +56:58:39.7
23:38:16.45 +56:01:55.4
00:13:23.75 +52:37:45.2
00:23:11.25 +55:47:39.7
###################################################################################
00:04:40.61 +55:32:17.7 -- not an asteroid (will add it to exclusion list)
00:20:46.10 +50:11:50.5 -- not an asteroid (will add it to exclusion list)
23:58:26.78 +51:26:16.1 -- not an asteroid (will add it to exclusion list)
00:23:11.80 +55:47:31.5 -- not an asteroid (will add it to exclusion list)
00:06:46.16 +53:36:36.3 -- not an asteroid (will add it to exclusion list)
23:36:23.82 +53:17:52.2 -- not an asteroid (will add it to exclusion list)
00:04:18.55 +51:51:34.0 -- not an asteroid (will add it to exclusion list)
23:29:20.51 +56:41:07.2 -- not an asteroid (will add it to exclusion list)
23:55:24.21 +51:47:36.3 -- not an asteroid (will add it to exclusion list)
00:23:24.19 +54:55:49.4 -- not an asteroid (will add it to exclusion list)
23:42:59.05 +52:41:50.6 -- not an asteroid (will add it to exclusion list)
23:46:41.23 +54:28:38.1 -- not an asteroid (will add it to exclusion list)
00:14:53.52 +53:15:51.3 -- not an asteroid (will add it to exclusion list)
23:59:20.52 +50:35:47.9 -- not an asteroid (will add it to exclusion list)
00:23:00.46 +55:45:43.2 -- not an asteroid (will add it to exclusion list)
00:16:25.12 +53:58:17.8 -- not an asteroid (will add it to exclusion list)
23:31:40.65 +49:36:15.0 -- not an asteroid (will add it to exclusion list)
23:36:25.20 +55:17:30.9 -- not an asteroid (will add it to exclusion list)
23:49:54.89 +53:28:41.6 -- not an asteroid (will add it to exclusion list)
23:41:52.97 +52:45:15.2 -- not an asteroid (will add it to exclusion list)
23:43:28.34 +50:59:01.0 -- not an asteroid (will add it to exclusion list)
00:23:22.81 +55:49:22.8 -- not an asteroid (will add it to exclusion list)
00:10:23.32 +49:55:14.2 -- not an asteroid (will add it to exclusion list)
23:57:56.94 +50:30:33.7 -- not an asteroid (will add it to exclusion list)
00:20:04.14 +50:09:07.3 -- not an asteroid (will add it to exclusion list)
23:56:53.46 +52:11:52.1 -- not an asteroid (will add it to exclusion list)
23:57:55.85 +50:31:26.0 -- not an asteroid (will add it to exclusion list)
23:56:32.61 +53:44:58.8 -- not an asteroid (will add it to exclusion list)
00:00:55.42 +50:46:23.5 -- not an asteroid (will add it to exclusion list)
00:22:12.97 +52:14:13.4 -- not an asteroid (will add it to exclusion list)
00:03:29.58 +49:57:53.4 -- not an asteroid (will add it to exclusion list)
23:48:59.83 +51:53:04.9 -- not an asteroid (will add it to exclusion list)
23:43:20.60 +54:07:09.5 -- not an asteroid (will add it to exclusion list)
00:22:22.53 +53:06:10.9 -- not an asteroid (will add it to exclusion list)
23:57:00.82 +53:45:33.1 -- not an asteroid (will add it to exclusion list)
00:02:01.42 +53:59:28.5 -- not an asteroid (will add it to exclusion list)
23:58:25.81 +51:26:22.8 -- not an asteroid (will add it to exclusion list)
00:18:27.78 +53:39:34.4 -- not an asteroid (will add it to exclusion list)
00:20:44.88 +50:11:52.7 -- not an asteroid (will add it to exclusion list)
00:11:07.91 +52:33:58.0 -- not an asteroid (will add it to exclusion list)
23:35:01.60 +50:35:52.6 -- not an asteroid (will add it to exclusion list)
23:59:53.61 +56:58:39.7 -- not an asteroid (will add it to exclusion list)
23:38:16.45 +56:01:55.4 -- not an asteroid (will add it to exclusion list)
00:13:23.75 +52:37:45.2 -- not an asteroid (will add it to exclusion list)
00:23:11.25 +55:47:39.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:55.42 +50:46:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:01.42 +53:59:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:29.58 +49:57:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:18.55 +51:51:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:40.61 +55:32:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:46.16 +53:36:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:23.32 +49:55:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:07.91 +52:33:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:23.75 +52:37:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:53.52 +53:15:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:25.12 +53:58:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:27.78 +53:39:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:04.14 +50:09:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:44.88 +50:11:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:46.10 +50:11:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:12.97 +52:14:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:22.53 +53:06:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:00.46 +55:45:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:11.25 +55:47:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:11.80 +55:47:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:22.81 +55:49:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:24.19 +54:55:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:20.51 +56:41:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:40.65 +49:36:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:01.60 +50:35:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:23.82 +53:17:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:25.20 +55:17:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:16.45 +56:01:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:52.97 +52:45:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:59.05 +52:41:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:20.60 +54:07:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:28.34 +50:59:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:41.23 +54:28:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:59.83 +51:53:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:54.89 +53:28:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:24.21 +51:47:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:32.61 +53:44:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:53.46 +52:11:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:00.82 +53:45:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:55.85 +50:31:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:56.94 +50:30:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:25.81 +51:26:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:26.78 +51:26:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:20.52 +50:35:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:53.61 +56:58:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:00:55.42 +50:46:23.5 -- not a known variable star
00:02:01.42 +53:59:28.5 -- not a known variable star
00:03:29.58 +49:57:53.4 -- not a known variable star
00:04:18.55 +51:51:34.0 -- not a known variable star
00:04:40.61 +55:32:17.7 -- a known variable star
00:06:46.16 +53:36:36.3 -- not a known variable star
00:10:23.32 +49:55:14.2 -- not a known variable star
00:11:07.91 +52:33:58.0 -- not a known variable star
00:13:23.75 +52:37:45.2 -- not a known variable star
00:14:53.52 +53:15:51.3 -- not a known variable star
00:16:25.12 +53:58:17.8 -- not a known variable star
00:18:27.78 +53:39:34.4 -- a known variable star
00:20:04.14 +50:09:07.3 -- not a known variable star
00:20:44.88 +50:11:52.7 -- not a known variable star
00:20:46.10 +50:11:50.5 -- not a known variable star
00:22:12.97 +52:14:13.4 -- not a known variable star
00:22:22.53 +53:06:10.9 -- not a known variable star
00:23:00.46 +55:45:43.2 -- not a known variable star
00:23:11.25 +55:47:39.7 -- not a known variable star
00:23:11.80 +55:47:31.5 -- a known variable star
00:23:22.81 +55:49:22.8 -- not a known variable star
00:23:24.19 +54:55:49.4 -- not a known variable star
23:29:20.51 +56:41:07.2 -- not a known variable star
23:31:40.65 +49:36:15.0 -- not a known variable star
23:35:01.60 +50:35:52.6 -- not a known variable star
23:36:23.82 +53:17:52.2 -- not a known variable star
23:36:25.20 +55:17:30.9 -- not a known variable star
23:38:16.45 +56:01:55.4 -- not a known variable star
23:41:52.97 +52:45:15.2 -- not a known variable star
23:42:59.05 +52:41:50.6 -- not a known variable star
23:43:20.60 +54:07:09.5 -- not a known variable star
23:43:28.34 +50:59:01.0 -- not a known variable star
23:46:41.23 +54:28:38.1 -- a known variable star
23:48:59.83 +51:53:04.9 -- a known variable star
23:49:54.89 +53:28:41.6 -- not a known variable star
23:55:24.21 +51:47:36.3 -- not a known variable star
23:56:32.61 +53:44:58.8 -- not a known variable star
23:56:53.46 +52:11:52.1 -- not a known variable star
23:57:00.82 +53:45:33.1 -- not a known variable star
23:57:55.85 +50:31:26.0 -- not a known variable star
23:57:56.94 +50:30:33.7 -- not a known variable star
23:58:25.81 +51:26:22.8 -- not a known variable star
23:58:26.78 +51:26:16.1 -- not a known variable star
23:59:20.52 +50:35:47.9 -- not a known variable star
23:59:53.61 +56:58:39.7 -- a known variable star
Found 39 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
45 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 45 (excluding asteroids and hot pixels, 39 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)2461225.81543605 -observatory V36
07:45:37.51 +17:48:41.3 Mercury (3.1mag)
09:45:50.71 +15:14:11.5 Venus (-4.1mag)
04:06:17.58 +20:36:04.3 Mars (1.3mag)
08:11:12.98 +20:28:20.4 Jupiter (-1.8mag)
00:55:04.44 +03:17:25.2 Saturn (0.8mag)
04:06:02.39 +20:41:48.8 Uranus (5.8mag)
00:17:00.93 +00:20:58.4 Neptune (7.8mag)
20:31:27.35 -23:15:21.3 Pluto (14.5mag)
22:11:10.47 -12:01:35.5 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Jul 4 02:41 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461225.81543605:
08:11:07.90 +20:28:39.1 Io (6.1mag)
08:11:23.28 +20:27:43.5 Europa (6.3mag)
08:11:26.24 +20:27:30.7 Ganymede (5.6mag)
08:11:06.64 +20:28:48.4 Callisto (6.9mag)
08:10:02.06 +20:10:11.3 Himalia (15.7mag)
08:11:13.27 +20:28:20.3 Thebe (16.6mag)
08:09:26.28 +20:16:12.0 Elara (17.6mag)
08:14:32.99 +20:25:46.0 Pasiphae (17.8mag)
08:16:30.97 +20:32:37.0 Carme (18.9mag)
00:55:07.49 +03:17:51.0 Titan (8.6mag)
00:55:07.14 +03:17:32.9 Rhea (9.9mag)
00:54:44.22 +03:17:46.4 Iapetus (11.2mag)
00:55:16.50 +03:16:55.1 Hyperion (14.6mag)
00:55:13.21 +03:15:32.2 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 4 02:41 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461225.81543605:
17:39:20.70 -34:06:42.8 JWST
08:54:36.25 +20:58:45.9 Chandra
23:17:30.95 +60:59:28.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 4 02:41 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461225.81543605 -observatory V36
02:27:31.90 +13:40:57.0 17.9mag P/1996 R2 (Lagerkvist)
18:22:45.65 -34:09:32.2 13.7mag P/2010 H2 (Vales)
06:19:36.65 -68:03:44.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:58:40.09 +32:20:50.9 17.6mag C/2017 K2 (PANSTARRS)
17:04:57.38 +16:03:05.0 18.0mag C/2021 G2 (ATLAS)
01:08:51.37 -05:40:03.8 15.3mag P/2021 N1 (ZTF)
23:02:54.28 +32:15:30.9 17.2mag C/2022 E2 (ATLAS)
06:05:25.34 +26:58:13.3 16.6mag C/2022 N2 (PANSTARRS)
09:50:20.06 +30:02:47.6 16.8mag C/2022 QE78 (ATLAS)
09:05:53.45 +04:51:57.9 17.8mag C/2022 R6 (PANSTARRS)
18:10:59.91 +21:29:20.9 17.9mag C/2023 A3 (Tsuchinshan-ATLAS)
15:12:23.52 -11:15:52.8 17.7mag P/2023 B1 (PANSTARRS)
21:56:02.11 +67:35:39.6 17.8mag C/2023 H5 (Lemmon)
16:43:28.57 -09:26:19.3 13.8mag C/2023 R1 (PANSTARRS)
07:50:24.63 +65:23:52.6 17.9mag C/2024 A1 (ATLAS)
07:24:45.81 +29:40:52.0 14.5mag C/2024 E1 (Wierzchos)
15:19:29.19 +15:08:02.1 17.5mag C/2024 G6 (ATLAS)
19:48:41.62 +38:06:53.6 13.8mag C/2024 J3 (ATLAS)
21:53:21.81 +45:02:54.5 17.9mag C/2024 R4 (PANSTARRS)
04:43:51.99 -14:05:55.5 15.8mag C/2024 T5 (ATLAS)
06:29:27.96 +30:04:30.0 18.0mag C/2025 J1 (Borisov)
07:09:52.77 -12:23:40.7 16.1mag C/2025 R3 (PANSTARRS)
09:49:18.06 +22:40:34.7 17.7mag C/2025 V2 (Rankin)
12:42:50.05 +04:10:17.7 17.1mag C/2025 Y1 (ATLAS)
17:09:36.71 +78:51:52.7 17.5mag C/2026 A2 (Bok)
02:39:21.54 +44:57:39.9 16.6mag C/2026 B2 (Sun-Gao)
11:21:52.99 +03:23:01.8 16.9mag A/2026 E1
21:09:15.95 -13:07:42.7 7.5mag 10P/Tempel
11:10:45.69 -01:38:50.7 16.1mag 29P/Schwassmann-Wachmann
03:51:21.14 +28:52:46.4 17.8mag 47P/Ashbrook-Jackson
09:55:25.01 +15:55:05.8 17.0mag 63P/Wild
00:45:23.69 -05:12:10.2 15.6mag 65P/Gunn
08:07:54.63 +34:25:26.4 17.7mag 76P/West-Kohoutek-Ikemura
04:12:44.02 +19:48:31.3 13.7mag 78P/Gehrels
02:12:07.55 +09:43:10.7 16.1mag 88P/Howell
06:17:15.69 +30:48:31.8 15.6mag 93P/Lovas
04:01:36.87 +30:46:04.7 17.0mag 114P/Wiseman-Skiff
07:53:55.18 +31:19:22.8 15.3mag 123P/West-Hartley
10:36:57.54 +03:39:36.4 16.7mag 124P/Mrkos
04:41:57.47 +20:36:43.8 16.3mag 128P/Shoemaker-Holt
05:24:45.11 +19:43:28.2 17.8mag 131P/Mueller
07:36:22.06 +14:24:08.3 17.8mag 141P/Machholz
07:35:46.98 +14:27:35.1 17.8mag 141P-A/Machholz
06:50:17.58 +18:15:47.2 14.8mag 141P-D/Machholz
03:13:59.08 -21:38:54.3 15.7mag 161P/Hartley-IRAS
05:11:24.89 +32:30:24.5 15.2mag 162P/SidingSpring
19:16:56.71 +11:44:25.4 15.2mag 169P/NEAT
01:26:17.25 +06:50:47.6 17.7mag 220P/McNaught
16:37:20.15 -08:11:45.2 16.9mag 235P/LINEAR
08:32:25.00 +33:49:39.9 17.8mag 240P/NEAT
20:43:51.70 -48:07:59.3 17.9mag 259P/Garradd
01:42:32.26 +09:16:15.2 15.8mag 260P/McNaught
05:19:02.67 +36:16:39.5 17.4mag 295P/LINEAR
15:07:13.92 +06:33:55.1 17.5mag 391P/Kowalski
08:29:13.48 +19:54:44.8 17.9mag 450P/LONEOS
07:42:12.56 +39:42:36.5 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 4 02:41 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
16:41:15.63 +39:17:14.70 2026-06-26.38 16.07
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
16:41:15.63 +39:17:14.70 2026-06-26.38 16.07
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
-rw-r--r-- 1 apache apache 5.6K Jul 4 02:41 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 4 02:41 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:30:39.340 +49:35:39.05 AT 2026qqr 2026-02-06.44 18.4425
02:16:29.646 -64:35:11.42 AT 2026qqq 2026-06-24.39 18.764
18:46:50.404 -57:44:13.07 AT 2026qqp 2026-06-27.19 17.811
18:52:25.568 -53:48:28.81 AT 2026qqo 2026-06-27.19 17.994
22:48:08.203 -71:09:43.31 AT 2026qqn 2026-06-27.28 18.614
21:45:30.534 -52:24:04.42 AT 2026qqm 2026-06-17.16 19.196
22:56:20.865 -25:59:31.71 AT 2026qql 2026-06-25.54 19.21
04:31:33.921 -71:04:40.00 AT 2026qqk 2026-06-27.35 18.232
22:12:27.288 -61:04:57.21 AT 2026qqj 2026-06-24.29 18.906
02:29:17.720 -54:48:23.47 AT 2026qqi 2026-06-27.34 17.773
21:48:06.694 -12:00:04.55 AT 2026qqh 2026-06-26.41 21.23
11:06:55.391 -04:07:04.72 AT 2026qqg 2026-06-27.97 18.081
05:12:36.560 -58:31:08.03 AT 2026qqf 2026-06-24.41 18.215
12:37:59.373 +03:20:56.02 AT 2026qqe 2026-06-25.05 18.266
01:16:11.239 -55:40:02.88 AT 2026qqd 2026-06-24.38 18.401
00:39:40.551 -56:06:55.52 AT 2026qqc 2026-06-24.36 18.488
12:32:13.060 +56:22:40.90 AT 2026qqb 2026-06-27.90 18.72
03:43:49.750 -46:38:15.17 AT 2026qqa 2026-06-23.42 18.775
22:17:40.013 -69:03:01.29 AT 2026qpz 2026-06-24.32 18.664
06:02:54.764 -64:43:45.31 AT 2026qpy 2026-06-24.42 18.203
-rw-r--r-- 1 apache apache 30K Jul 4 02:41 tns_transients_list.txt