This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.39 02:09:54.96 +65:15:24.2
131.02725 3.62582 galactic Cas Second-epoch detections are separated by 3.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:09:54.96 +65:15:24.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:54.96 +65:15:24.2: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:54.96 +65:15:24.2: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 02 09 54.96 +65 15 24.2 11.4 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,2461172.9050,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.35 01:33:12.61 +61:16:56.8
127.92939 -1.18333 galactic Cas Second-epoch detections are separated by 1.6" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:33:12.61 +61:16:56.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:12.61 +61:16:56.8: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:12.61 +61:16:56.8: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 33 12.61 +61 16 56.8 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,2461172.9050,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.22 01:12:41.28 +61:18:08.3
125.48095 -1.46423 galactic Cas Second-epoch detections are separated by 0.9" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:41.28 +61:18:08.3 (user input) | T | P | (position from user input) J-Ks=0.156+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:41.28 +61:18:08.3: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:41.28 +61:18:08.3: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 12 41.28 +61 18 08.3 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,11.22,0.05,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
target 20260512.4050 11.22CV 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 05 12.4050 2461172.9050 11.35 01:23:56.88 +62:15:29.3
126.70532 -0.37519 galactic Cas Second-epoch detections are separated by 3.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:23:56.88 +62:15:29.3 (user input) | T | P | (position from user input) J-Ks=0.526+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:56.88 +62:15:29.3: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:56.88 +62:15:29.3: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 23 56.88 +62 15 29.3 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,2461172.9050,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.19 01:13:20.08 +61:29:38.6
125.54204 -1.26667 galactic Cas Second-epoch detections are separated by 1.3" and 1.7 pix
The object was found in VSX17" Gaia DR3 522571492708068608
Type: ROT
# Max. Min./Amp. JD0 Period
14.070 G 14.120 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:20.08 +61:29:38.6: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:20.08 +61:29:38.6: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 13 20.08 +61 29 38.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522571492708068608,2461172.9050,11.19,0.05,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
Gaia DR3 522571492708068608 20260512.4050 11.19CV 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 05 12.4050 2461172.9050 11.46 01:18:35.27 +63:50:26.2
125.91925 1.12645 galactic Cas Second-epoch detections are separated by 1.9" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:35.27 +63:50:26.2 (user input) | T | P | (position from user input) J-Ks=0.534+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:35.27 +63:50:26.2: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:35.27 +63:50:26.2: 14.74 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 18 35.27 +63 50 26.2 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.01 01:39:15.88 +58:53:23.0
129.08775 -3.40922 galactic Cas Second-epoch detections are separated by 4.3" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:39:15.88 +58:53:23.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:15.88 +58:53:23.0: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:15.88 +58:53:23.0: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 39 15.88 +58 53 23.0 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.11 01:27:41.40 +59:04:48.2
127.58306 -3.46392 galactic Cas Second-epoch detections are separated by 1.2" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:27:41.40 +59:04:48.2 (user input) | T | P | (position from user input) J-Ks=0.895+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:41.40 +59:04:48.2: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:41.40 +59:04:48.2: 14.14 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 27 41.40 +59 04 48.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,11.11,0.05,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 20260512.4050 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.15 01:29:18.30 +63:15:50.2
127.17569 0.70463 galactic Cas Second-epoch detections are separated by 3.1" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:29:18.30 +63:15:50.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:18.30 +63:15:50.2: 12.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:18.30 +63:15:50.2: 13.61 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 29 18.30 +63 15 50.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.09 01:21:45.50 +58:34:14.5
126.88611 -4.06808 galactic Cas Second-epoch detections are separated by 2.0" and 1.0 pix
The object was found in VSX21" ZTF J012144.11+583432.6
Type: EA
# Max. Min./Amp. JD0 Period
17.914 r Y 0.259 r 2458650.93340 0.872868200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:45.50 +58:34:14.5: 12.61 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:45.50 +58:34:14.5: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 21 45.50 +58 34 14.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J012144.11+583432.6,2461172.9050,11.09,0.05,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
ZTF J012144.11+583432.6 20260512.4050 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 05 12.4050 2461172.9050 11.09 01:17:47.78 +57:25:43.5
126.48886 -5.26085 galactic Cas Second-epoch detections are separated by 2.9" and 0.8 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 J019.4502+57.4284 | 01:17:47.78 +57:25:43.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:47.78 +57:25:43.5: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:47.78 +57:25:43.5: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 17 47.78 +57 25 43.5 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
ATO J019.4502+57.4284,2461172.9050,11.09,0.05,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
ATO J019.4502+57.4284 20260512.4050 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 05 12.4050 2461172.9050 11.01 01:13:40.89 +60:51:26.3
125.63824 -1.89751 galactic Cas Second-epoch detections are separated by 2.4" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:13:40.89 +60:51:26.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:40.89 +60:51:26.3: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:40.89 +60:51:26.3: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 13 40.89 +60 51 26.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.20 01:22:33.14 +60:44:42.2
126.72648 -1.89725 galactic Cas Second-epoch detections are separated by 2.3" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:22:33.14 +60:44:42.2 (user input) | T | P | (position from user input) J-Ks=1.158+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:33.14 +60:44:42.2: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:33.14 +60:44:42.2: 14.10 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 22 33.14 +60 44 42.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.94 01:43:08.00 +58:54:08.3
129.57650 -3.30091 galactic Cas Second-epoch detections are separated by 1.0" and 0.8 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 J025.7736+58.9016 | 01:43:08.00 +58:54:08.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.275+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:08.00 +58:54:08.3: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:08.00 +58:54:08.3: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 43 08.00 +58 54 08.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.7736+58.9016,2461172.9050,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.7736+58.9016 20260512.4050 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.11 01:12:01.08 +64:42:20.0
125.12905 1.92164 galactic Cas Second-epoch detections are separated by 2.6" and 2.5 pix
The object was found in VSX 1" ZTF J011201.03+644221.2
Type: RS
# Max. Min./Amp. JD0 Period
14.762 g Y 0.263 g 2458343.85900 3.018403700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:01.08 +64:42:20.0: 11.65 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:01.08 +64:42:20.0: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 12 01.08 +64 42 20.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J011201.03+644221.2,2461172.9050,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011201.03+644221.2 20260512.4050 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.99 01:26:05.52 +59:01:15.6
127.38730 -3.55064 galactic Cas Second-epoch detections are separated by 1.8" and 0.9 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 J021.5231+59.0209 | 01:26:05.52 +59:01:15.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.314+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.52 +59:01:15.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.52 +59:01:15.6: 13.94 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 26 05.52 +59 01 15.6 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.5231+59.0209,2461172.9050,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.5231+59.0209 20260512.4050 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.02 01:07:39.43 +59:59:17.3
124.96124 -2.81969 galactic Cas Second-epoch detections are separated by 7.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:39.43 +59:59:17.3 (user input) | T | P | (position from user input) J-Ks=0.895+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.43 +59:59:17.3: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.43 +59:59:17.3: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 07 39.43 +59 59 17.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.02 01:05:21.38 +64:15:22.1
124.44299 1.42523 galactic Cas Second-epoch detections are separated by 1.9" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:05:21.38 +64:15:22.1 (user input) | T | P | (position from user input) J-Ks=0.907+/-0.025 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:05:21.38 +64:15:22.1: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:21.38 +64:15:22.1: 13.80 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 05 21.38 +64 15 22.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.66 01:26:38.91 +59:41:40.1
127.36637 -2.87377 galactic Cas Second-epoch detections are separated by 5.2" and 0.8 pix
The object was found in VSX 4" Gaia DR3 510083239641442688
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.660 G 13.680 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:38.91 +59:41:40.1: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:38.91 +59:41:40.1: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 26 38.91 +59 41 40.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510083239641442688,2461172.9050,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510083239641442688 20260512.4050 10.66CV 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 05 12.4050 2461172.9050 10.71 01:25:45.74 +59:01:23.4
127.34489 -3.55417 galactic Cas Second-epoch detections are separated by 0.5" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:25:45.74 +59:01:23.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:45.74 +59:01:23.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:45.74 +59:01:23.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 25 45.74 +59 01 23.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.32 01:39:07.81 +59:42:42.9
128.91905 -2.60428 galactic Cas Second-epoch detections are separated by 1.6" and 0.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:39:07.81 +59:42:42.9 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:07.81 +59:42:42.9: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:07.81 +59:42:42.9: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 39 07.81 +59 42 42.9 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.29 01:37:25.50 +63:41:28.0
128.00114 1.27290 galactic Cas Second-epoch detections are separated by 2.5" and 1.9 pix
The object was found in VSX 1" ASASSN-V J013725.59+634128.8
Type: DCEP
# Max. Min./Amp. JD0 Period
13.174 r Y 0.560 r 2457052.73600 3.238890000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:25.50 +63:41:28.0: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:25.50 +63:41:28.0: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 37 25.50 +63 41 28.0 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013725.59+634128.8,2461172.9050,10.29,0.05,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
ASASSN-V J013725.59+634128.8 20260512.4050 10.29CV 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 05 12.4050 2461172.9050 9.95 01:11:14.86 +61:08:19.1
125.32112 -1.64118 galactic Cas Second-epoch detections are separated by 1.5" and 1.5 pix
The object was found in VSX 1" ZTF J011114.91+610818.6
Type: RS
# Max. Min./Amp. JD0 Period
13.623 g Y 0.083 g 2458358.91940 0.779401400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:14.86 +61:08:19.1: 12.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:14.86 +61:08:19.1: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 11 14.86 +61 08 19.1 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J011114.91+610818.6,2461172.9050,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011114.91+610818.6 20260512.4050 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 9.43 01:15:30.66 +63:53:02.2
125.57770 1.13593 galactic Cas Second-epoch detections are separated by 1.3" and 2.0 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 524740829149634688 | 01:15:31.47 +63:52:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.371+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:30.66 +63:53:02.2: 9.54 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:30.66 +63:53:02.2: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 15 30.66 +63 53 02.2 9.4 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 524740829149634688,2461172.9050,9.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 524740829149634688 20260512.4050 9.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 9.25 01:25:56.63 +59:35:12.1
127.29260 -2.99258 galactic Cas Second-epoch detections are separated by 1.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510075336901717632 | 01:25:55.70 +59:34:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1960IzKry..24..160B [B60] +59 169 J-Ks=0.194+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:56.63 +59:35:12.1: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:56.63 +59:35:12.1: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 25 56.63 +59 35 12.1 9.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510075336901717632,2461172.9050,9.25,0.05,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
Gaia DR3 510075336901717632 20260512.4050 9.25CV 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 05 12.4050 2461172.9050 10.60 02:00:21.64 +64:56:38.6
130.14888 3.04249 galactic Cas Second-epoch detections are separated by 1.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 518139017740687360 | 02:00:16.12 +64:56:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9IV/V 1928MeUpp..37....1S BD+64 275 J-Ks=1.311+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:21.64 +64:56:38.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:21.64 +64:56:38.6: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 02 00 21.64 +64 56 38.6 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 518139017740687360,2461172.9050,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518139017740687360 20260512.4050 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.68 01:19:41.74 +62:51:06.7
126.14891 0.15675 galactic Cas Second-epoch detections are separated by 2.0" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:19:41.74 +62:51:06.7 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:41.74 +62:51:06.7: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:41.74 +62:51:06.7: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 19 41.74 +62 51 06.7 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.54 01:46:38.59 +60:07:34.5
129.76029 -2.01156 galactic Cas Second-epoch detections are separated by 0.5" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.6591+60.1406 | 01:46:39.63 +60:07:57.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.59 +60:07:34.5: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:38.59 +60:07:34.5: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 46 38.59 +60 07 34.5 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.6591+60.1406,2461172.9050,10.54,0.05,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
ATO J026.6591+60.1406 20260512.4050 10.54CV 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 05 12.4050 2461172.9050 10.76 01:36:16.40 +60:12:25.5
128.47844 -2.18094 galactic Cas Second-epoch detections are separated by 3.2" and 0.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 509768332640107392 | 01:36:16.56 +60:11:46.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:16.40 +60:12:25.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:16.40 +60:12:25.5: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 36 16.40 +60 12 25.5 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509768332640107392,2461172.9050,10.76,0.05,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 509768332640107392 20260512.4050 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.78 01:29:21.46 +61:44:14.8
127.40532 -0.80451 galactic Cas Second-epoch detections are separated by 0.3" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:29:21.46 +61:44:14.8 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.037 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:21.46 +61:44:14.8: 12.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:21.46 +61:44:14.8: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 29 21.46 +61 44 14.8 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.89 01:06:55.52 +59:18:56.0
124.91033 -3.49669 galactic Cas Second-epoch detections are separated by 5.6" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:55.52 +59:18:56.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.52 +59:18:56.0: 13.08 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.52 +59:18:56.0: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 06 55.52 +59 18 56.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.86 01:18:48.52 +64:12:23.2
125.90464 1.49279 galactic Cas Second-epoch detections are separated by 1.3" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:48.52 +64:12:23.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:48.52 +64:12:23.2: 11.79 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:48.52 +64:12:23.2: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 18 48.52 +64 12 23.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.91 01:44:03.34 +61:54:44.9
129.08293 -0.32926 galactic Cas Second-epoch detections are separated by 3.4" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511486800591720192 | 01:44:01.89 +61:55:16.8 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: B1V 1999A&AS..136..313S Cl* NGC 654 Sto 94 J-Ks=12.609+/- (unrealisitic color!)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:03.34 +61:54:44.9: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:03.34 +61:54:44.9: 13.94 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 44 03.34 +61 54 44.9 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511486800591720192,2461172.9050,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511486800591720192 20260512.4050 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.94 01:22:11.02 +59:09:04.3
126.87190 -3.48515 galactic Cas Second-epoch detections are separated by 2.0" and 1.0 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 413976852405588480 | 01:22:13.31 +59:08:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1960IzKry..24..160B [B60] +58 184 J-Ks=0.462+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:11.02 +59:09:04.3: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:11.02 +59:09:04.3: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 22 11.02 +59 09 04.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413976852405588480,2461172.9050,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413976852405588480 20260512.4050 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.02 01:50:39.80 +62:00:55.7
129.81906 -0.06174 galactic Cas Second-epoch detections are separated by 1.8" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511356332360621440 | 01:50:34.89 +62:00:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1955ApJS....2..123F LF 5 +61 158 J-Ks=1.202+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:39.80 +62:00:55.7: 13.28 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:39.80 +62:00:55.7: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 50 39.80 +62 00 55.7 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511356332360621440,2461172.9050,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511356332360621440 20260512.4050 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.90 01:14:41.59 +58:46:46.7
125.94881 -3.95582 galactic Cas Second-epoch detections are separated by 1.7" and 1.1 pix
The object was found in VSX22" Gaia DR3 414091266028390144
Type: ROT
# Max. Min./Amp. JD0 Period
18.000 G 18.140 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:41.59 +58:46:46.7: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:41.59 +58:46:46.7: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 14 41.59 +58 46 46.7 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414091266028390144,2461172.9050,10.90,0.05,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 414091266028390144 20260512.4050 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.88 01:32:40.44 +61:07:36.9
127.89059 -1.34720 galactic Cas Second-epoch detections are separated by 1.6" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:32:40.44 +61:07:36.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:40.44 +61:07:36.9: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:40.44 +61:07:36.9: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 32 40.44 +61 07 36.9 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.99 01:38:05.89 +61:04:13.2
128.54623 -1.29176 galactic Cas Second-epoch detections are separated by 3.0" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:38:05.89 +61:04:13.2 (user input) | T | P | (position from user input) J-Ks=0.901+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:05.89 +61:04:13.2: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:05.89 +61:04:13.2: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 38 05.89 +61 04 13.2 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,2461172.9050,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.05 01:36:50.76 +59:55:50.2
128.59705 -2.44074 galactic Cas Second-epoch detections are separated by 1.0" and 1.2 pix
The object was found in VSX 2" Gaia DR3 509760361181182976
Type: ROT
# Max. Min./Amp. JD0 Period
13.870 G 13.910 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:50.76 +59:55:50.2: 12.64 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:50.76 +59:55:50.2: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 36 50.76 +59 55 50.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509760361181182976,2461172.9050,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509760361181182976 20260512.4050 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.04 01:15:11.25 +60:52:42.7
125.81900 -1.86002 galactic Cas Second-epoch detections are separated by 0.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:15:11.25 +60:52:42.7 (user input) | T | P | (position from user input) J-Ks=0.440+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:11.25 +60:52:42.7: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:11.25 +60:52:42.7: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 15 11.25 +60 52 42.7 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.09 01:09:22.71 +57:26:31.0
125.35441 -5.34539 galactic Cas Second-epoch detections are separated by 3.5" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.3204+57.4562 | 01:09:17.29 +57:26:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.782+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:22.71 +57:26:31.0: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.71 +57:26:31.0: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 09 22.71 +57 26 31.0 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
ATO J017.3204+57.4562,2461172.9050,11.09,0.05,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
ATO J017.3204+57.4562 20260512.4050 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 05 12.4050 2461172.9050 10.87 02:00:32.86 +59:40:05.4
131.56358 -2.04038 galactic Cas Second-epoch detections are separated by 6.3" and 1.4 pix
The object was found in VSX 4" ZTF J020033.07+594008.7
Type: SR
# Max. Min./Amp. JD0 Period
13.621 r Y 0.477 r 2458342.93970 344.838134100000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:32.86 +59:40:05.4: 11.56 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.86 +59:40:05.4: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 02 00 32.86 +59 40 05.4 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J020033.07+594008.7,2461172.9050,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J020033.07+594008.7 20260512.4050 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.09 01:31:48.61 +64:22:27.5
127.28095 1.84400 galactic Cas Second-epoch detections are separated by 2.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:31:48.61 +64:22:27.5 (user input) | T | P | (position from user input) J-Ks=0.844+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.61 +64:22:27.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.61 +64:22:27.5: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 31 48.61 +64 22 27.5 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,2461172.9050,11.09,0.05,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 20260512.4050 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 05 12.4050 2461172.9050 11.11 01:59:34.22 +63:37:08.3
130.41409 1.74135 galactic Cas Second-epoch detections are separated by 3.8" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:59:34.22 +63:37:08.3 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:34.22 +63:37:08.3: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:34.22 +63:37:08.3: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 59 34.22 +63 37 08.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,11.11,0.05,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 20260512.4050 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.06 01:44:15.55 +61:53:39.0
129.11011 -0.34232 galactic Cas Second-epoch detections are separated by 0.2" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:44:15.55 +61:53:39.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:15.55 +61:53:39.0: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:15.55 +61:53:39.0: 14.03 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 44 15.55 +61 53 39.0 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,2461172.9050,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.03 02:02:25.11 +64:38:23.6
130.44182 2.80812 galactic Cas Second-epoch detections are separated by 8.7" and 3.3 pix
The object was found in VSX 5" ASASSN-V J020225.96+643822.9
Type: SR
# Max. Min./Amp. JD0 Period
14.090 V 14.200 V 2457555.11300 70.630000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:25.11 +64:38:23.6: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:25.11 +64:38:23.6: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 02 02 25.11 +64 38 23.6 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
ASASSN-V J020225.96+643822.9,2461172.9050,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J020225.96+643822.9 20260512.4050 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.29 01:38:35.72 +64:48:50.3
127.92434 2.40031 galactic Cas Second-epoch detections are separated by 1.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 513065252614504576 | 01:38:36.54 +64:48:07.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.864+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:35.72 +64:48:50.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:35.72 +64:48:50.3: 14.23 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 38 35.72 +64 48 50.3 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
Gaia DR3 513065252614504576,2461172.9050,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 513065252614504576 20260512.4050 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.23 01:40:22.27 +60:45:17.6
128.87599 -1.55088 galactic Cas Second-epoch detections are separated by 7.9" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:40:22.27 +60:45:17.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:22.27 +60:45:17.6: 11.86 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:22.27 +60:45:17.6: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 40 22.27 +60 45 17.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.51 01:23:26.87 +61:39:56.3
126.72099 -0.97039 galactic Cas Second-epoch detections are separated by 0.7" and 1.6 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 | Large-amplitude variable Gaia DR2 510913783233562880 | 01:23:29.77 +61:40:30.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A0 1960IzKry..24..160B [B60] +61 183
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:26.87 +61:39:56.3: 13.22 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:26.87 +61:39:56.3: 14.42 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 23 26.87 +61 39 56.3 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 510913783233562880,2461172.9050,11.51,0.05,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
Large-amplitude variable Gaia DR2 510913783233562880 20260512.4050 11.51CV 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 05 12.4050 2461172.9050 11.42 02:01:06.89 +64:35:49.8
130.31863 2.72937 galactic Cas Second-epoch detections are separated by 2.6" and 2.0 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 518077479449762560 | 02:01:07.64 +64:35:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.841+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:06.89 +64:35:49.8: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:06.89 +64:35:49.8: 14.25 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 02 01 06.89 +64 35 49.8 11.4 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 518077479449762560,2461172.9050,11.42,0.05,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 518077479449762560 20260512.4050 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.77 01:41:40.27 +62:34:08.6
128.68076 0.25933 galactic Cas Second-epoch detections are separated by 2.3" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511660484767387136 | 01:41:35.49 +62:34:37.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.349+/-0.041 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:40.27 +62:34:08.6: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:40.27 +62:34:08.6: 14.61 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 41 40.27 +62 34 08.6 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 511660484767387136,2461172.9050,11.77,0.05,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
Gaia DR3 511660484767387136 20260512.4050 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.73 01:27:06.79 +61:26:14.9
127.18370 -1.13942 galactic Cas Second-epoch detections are separated by 0.7" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:27:06.79 +61:26:14.9 (user input) | T | P | (position from user input) J-Ks=0.535+/-0.040 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:06.79 +61:26:14.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:06.79 +61:26:14.9: 14.76 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.76 +/- 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 05 12.4050* 01 27 06.79 +61 26 14.9 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,2461172.9050,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 11.82 01:17:18.16 +61:15:41.0
126.03688 -1.45433 galactic Cas Second-epoch detections are separated by 2.1" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510541289312876160 | 01:17:21.32 +61:16:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.028+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:18.16 +61:15:41.0: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:18.16 +61:15:41.0: 14.88 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 17 18.16 +61 15 41.0 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 510541289312876160,2461172.9050,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510541289312876160 20260512.4050 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.19 02:13:47.36 +63:11:26.1
132.06202 1.78797 galactic Cas Second-epoch detections are separated by 2.7" and 1.9 pix
The object was found in VSX 3" NSVS J0213478+631127
Type: L:
# Max. Min./Amp. JD0 Period
11.122 R1 Y 0.644 R1 355.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:47.36 +63:11:26.1: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:47.36 +63:11:26.1: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 02 13 47.36 +63 11 26.1 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0213478+631127,2461172.9050,10.19,0.05,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
NSVS J0213478+631127 20260512.4050 10.19CV 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 05 12.4050 2461172.9050 8.93 02:15:23.54 +65:01:38.2
131.64673 3.58573 galactic Cas Second-epoch detections are separated by 0.4" and 2.1 pix
The object was found in VSX 2" V0931 Cas
Type: SR
# Max. Min./Amp. JD0 Period
12.800 V 13.500 V 2451453.00000 138.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:23.54 +65:01:38.2: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:23.54 +65:01:38.2: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 02 15 23.54 +65 01 38.2 8.9 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
V0931 Cas,2461172.9050,8.93,0.05,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
V0931 Cas 20260512.4050 8.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.4050 2461172.9050 10.78 01:33:44.46 +60:46:16.7
128.07587 -1.67725 galactic Cas Second-epoch detections are separated by 2.8" and 0.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:33:44.46 +60:46:16.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:44.46 +60:46:16.7: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:44.46 +60:46:16.7: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.4050* 01 33 44.46 +60 46 16.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.9050,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.4050 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461172.90610792 12.05.2026 09:44:37.724 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 13 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): 26170
Objects passed selection criteria: 26040
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 18876.2
Average stars matched: 17204 (91.141 %)
Memory usage VmPeak: 128288 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 10 15:05:05 CDT 2026
VaST build number 1.0rc89-44-gd532a530
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 12 06:40:16 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461172.90610792 12.05.2026 09:44:37.724 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 225
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 120 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): 189828
Objects passed selection criteria: 189331
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 141727
Average stars matched: 129166 (91.1372 %)
Memory usage VmPeak: 2000196 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 10 15:05:05 CDT 2026
VaST build number 1.0rc89-44-gd532a530
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 12 06:46:22 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.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: 2461172.90386410
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
Entering WCS image calibration mode.
Entering WCS image calibration mode.
Entering WCS image calibration mode.
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits was not set. Trying to guess...
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits was not set. Trying to guess...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
The guess is 605 arcmin.
The guess is 605 arcmin.
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits .... Determining astrometry method...
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Using the local copy of Astrometry.net software...
Choosing aperture...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits was not set. Trying to guess...
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits was not set. Trying to guess...
The guess is 569 arcmin.
The guess is 570 arcmin.
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/lib/make_outxyls_for_astrometric_calibration found 17033 high-SNR stars for plate solving
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Generating wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat from image00001.cat
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/lib/make_outxyls_for_astrometric_calibration found 16336 high-SNR stars for plate solving
Generating wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat from image00002.cat
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits created.
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits created.
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.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: "out2255977.xyls"...
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.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: "out2255979.xyls"...
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:54.565 +61:59:40.70 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 31559 stars ###
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/correct_sextractor_wcs_catalog_usingxy2sky2256351.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
### Converted positions of 31681 stars ###
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/correct_sextractor_wcs_catalog_usingxy2sky2256360.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2255979.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).
Reading file "./out2255977.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
log-odds ratio 55.6018 (1.40468e+24), 15 match, 0 conflict, 42 distractors, 89 index.
RA,Dec = (25.6108,61.9983), pixel scale 5.92047 arcsec/pix.
Hit/miss: Hit/miss: ----+----+--+---++--++--+---+---+---+---+---+-------+---+(best)-----------+-----------+-----------+-------
log-odds ratio 54.7904 (6.23999e+23), 15 match, 0 conflict, 42 distractors, 89 index.
RA,Dec = (25.6067,61.9997), pixel scale 5.92188 arcsec/pix.
Hit/miss: Hit/miss: ----+----+--+---++--++--+---+---+---+---+---+-------+---+(best)-----------+-----------+-----------+-------
Field 1: solved with index index-4114.fits.
Field 1 solved: writing to file ./out2255979.solved to indicate this.
Field 1: solved with index index-4114.fits.
Field 1 solved: writing to file ./out2255977.solved to indicate this.
Field: out2255979.xyls
Field: out2255977.xyls
Field center: (RA,Dec) = (25.681785, 61.991877) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:42:43.628, +61:59:30.759).
Field size: 15.744 x 10.5361 degrees
Field rotation angle: up is -2.27748 degrees E of N
Field parity: neg
Field center: (RA,Dec) = (25.677500, 61.992808) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:42:42.600, +61:59:34.109).
Field size: 15.7482 x 10.5389 degrees
Field rotation angle: up is -2.29672 degrees E of N
Field parity: neg
Inserting WCS header... Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits' -> 'fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits'
'/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits' -> 'fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits'
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 12 06:40 fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
-rw-r--r-- 1 apache apache 12K May 12 06:40 out2255977.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits for reading... done!
Creating new image file (wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits)... done!
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 12 06:40 fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
-rw-r--r-- 1 apache apache 12K May 12 06:40 out2255979.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits for reading... done!
Creating new image file (wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits)... done!
done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits (fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits (fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.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: "out2255977.xyls"...
Reading input file 1 of 1: "out2255979.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2255977.axy"...
Only searching for solutions within 15.685 degrees of RA,Dec (25.6792,61.9937)
log-odds ratio 234.897 (1.03437e+102), 23 match, 0 conflict, 31 distractors, 27 index.
RA,Dec = (25.6873,62.0051), pixel scale 5.95814 arcsec/pix.
Hit/miss: Hit/miss: ++-++++-++--+--++---+++-+-+-+-+--++----+------+------+(best)----------------------------------------------
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2255979.axy"...
Only searching for solutions within 15.68 degrees of RA,Dec (25.6835,61.9927)
log-odds ratio 144.657 (6.66412e+62), 19 match, 0 conflict, 30 distractors, 27 index.
RA,Dec = (25.684,61.9913), pixel scale 5.96105 arcsec/pix.
Hit/miss: Hit/miss: ++-+---+++----++--+-+-----+-++++--++---------+--+(best)---------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2255977.solved to indicate this.
Field: out2255977.xyls
Field center: (RA,Dec) = (25.676553, 61.992035) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:42:42.373, +61:59:31.324).
Field size: 15.7306 x 10.5398 degrees
Field rotation angle: up is -2.30354 degrees E of N
Field parity: neg
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2255979.solved to indicate this.
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 12 06:40 fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
-rw-r--r-- 1 apache apache 12K May 12 06:40 out2255977.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits for reading... done!
Creating new image file (wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits)... done!
Field: out2255979.xyls
Field center: (RA,Dec) = (25.682917, 61.990654) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:42:43.900, +61:59:26.356).
Field size: 15.7202 x 10.5362 degrees
Field rotation angle: up is -2.30469 degrees E of N
Field parity: neg
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 12 06:40 fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
-rw-r--r-- 1 apache apache 12K May 12 06:40 out2255979.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits for reading... done!
Creating new image file (wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits)... done!
done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 82193 sources.
simplexy: found 81736 sources.
Solving...
Reading file "./wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.axy"...
Verifying WCS using indices with quads of size [63.5127, 952.095] arcmin
Verifying WCS with index 39 of 61 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 40 of 61 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 42.6672 (3.38959e+18), 24 match, 0 conflict, 469 distractors, 27 index.
RA,Dec = (25.6812,61.9898), pixel scale 5.9655 arcsec/pix.
Hit/miss: Hit/miss: ----------------------------+-----+------------------+---------+-+---------+------------------------
--> log-odds 42.6672
Verifying WCS with index 41 of 61 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 212.144 (1.35852e+92), 40 match, 0 conflict, 453 distractors, 49 index.
RA,Dec = (25.6812,61.9898), pixel scale 5.9655 arcsec/pix.
Hit/miss: Hit/miss: ---------------+-----+---+--+--+--+--------+------+--+---------+-+------+--+------+-------++--------
--> log-odds 212.144
Verifying WCS with index 42 of 61 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 545.239 (6.22837e+236), 75 match, 0 conflict, 418 distractors, 91 index.
RA,Dec = (25.6812,61.9898), pixel scale 5.9655 arcsec/pix.
Hit/miss: Hit/miss: --+--+---+-----+---+-+---+--++-+--+-------++---+--+--+-----++--+-+------+-++----+-+-----+-++--------
--> log-odds 545.239
Verifying WCS with index 43 of 61 (/usr/local/astrometry/data/index-4113.fits)
Solving...
Verifying WCS of field 1.
log-odds ratio 1153.91 (inf), 147 match, 0 conflict, 479 distractors, 191 index.
RA,Dec = (25.6812,61.9898), pixel scale 5.9655 arcsec/pix.
Hit/miss: Hit/miss: --++-+-+++-----+--++++-+++--++-++++--+----++-+-+--+--+-----++-++++++--+-+-+++---+-++-+--+-+++-------
Reading file "./wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.axy"...
Verifying WCS using indices with quads of size [63.5416, 952.527] arcmin
Verifying WCS with index 39 of 61 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 40 of 61 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 12.9158
Verifying WCS with index 41 of 61 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 179.427 (8.40109e+77), 34 match, 0 conflict, 348 distractors, 49 index.
RA,Dec = (25.6749,61.9912), pixel scale 5.96822 arcsec/pix.
Hit/miss: Hit/miss: ---+---++------------+-+--------------+-------+-----+----+--------------+-+----+---++-------------+-
--> log-odds 1153.91
Verifying WCS with index 44 of 61 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 2385.61 (inf), 299 match, 0 conflict, 610 distractors, 384 index.
RA,Dec = (25.6812,61.9898), pixel scale 5.9655 arcsec/pix.
Hit/miss: Hit/miss: +-++-+++++--+--++-++++++++--++-++++-++---+++-+-+--+-++----++++++++++-++++++++++++++++++++-+++---+-++
--> log-odds 179.427
Verifying WCS with index 42 of 61 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 539.923 (3.06023e+234), 67 match, 0 conflict, 350 distractors, 91 index.
RA,Dec = (25.6749,61.9912), pixel scale 5.96822 arcsec/pix.
Hit/miss: Hit/miss: ---+---++---+---+----+-+--+-----+---+-+-------+-----++---+-------+-+---++-++---+--+++-----------+-+-
--> log-odds 539.923
Verifying WCS with index 43 of 61 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 1256.07 (inf), 145 match, 0 conflict, 504 distractors, 191 index.
RA,Dec = (25.6749,61.9912), pixel scale 5.96822 arcsec/pix.
Hit/miss: Hit/miss: +--++++++-+++--++-+--+-++-+-----+---++++-+-++-+-++--++---+---+---+-+-++++-+++--+--+++-----------+-++
--> log-odds 2385.61
Verifying WCS with index 45 of 61 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 3835.48 (inf), 512 match, 0 conflict, 667 distractors, 728 index.
RA,Dec = (25.6812,61.9898), pixel scale 5.9655 arcsec/pix.
Hit/miss: Hit/miss: +-++-+++++-++-++++++++++++-++++++++-++++++++-+-++-+-++-++-+++++++++++++++++++++++++++++++-++++++++++
--> log-odds 1256.07
Verifying WCS with index 44 of 61 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 2561.11 (inf), 295 match, 0 conflict, 561 distractors, 385 index.
RA,Dec = (25.6749,61.9912), pixel scale 5.96822 arcsec/pix.
Hit/miss: Hit/miss: +++++++++-+++-+++++-+++++-+----++-+-++++-++++-+++++++++-++--++++++-+-++++-++++-+--+++++++-+++-+-+-++
--> log-odds 2561.11
Verifying WCS with index 45 of 61 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 4501.63 (inf), 547 match, 0 conflict, 855 distractors, 729 index.
RA,Dec = (25.6749,61.9912), pixel scale 5.96822 arcsec/pix.
Hit/miss: Hit/miss: +++++++++-+++++++++-+++++-+++-+++++-++++++++++++++++++++++--++++++-++++++++++++++-+++++++-++++++++++
--> log-odds 3835.48
Verifying WCS with index 46 of 61 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 6914.96 (inf), 1010 match, 0 conflict, 1686 distractors, 1446 index.
RA,Dec = (25.6812,61.9898), pixel scale 5.9655 arcsec/pix.
Hit/miss: Hit/miss: +-+++++++++++-++++++++++++-++++++++-+++++++++++++-++++-++++++++++++++++++++++++++++++++++-++++++++++
--> log-odds 4501.63
Verifying WCS with index 46 of 61 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 8125.5 (inf), 1071 match, 0 conflict, 1577 distractors, 1447 index.
RA,Dec = (25.6749,61.9912), pixel scale 5.96822 arcsec/pix.
Hit/miss: Hit/miss: +++++++++-+++++++++-++++++++++++++++++++++++++++++++++++++-+++++++-+++++++++++++++++++++++++++++++++
--> log-odds 6914.96
Got 7 solutions.
Field: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Field center: (RA,Dec) = (25.682901, 61.990778) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:42:43.896, +61:59:26.802).
Field size: 15.7253 x 10.5365 degrees
Field rotation angle: up is -2.28187 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.new"...
--> log-odds 8125.5
Got 6 solutions.
Field: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
Field center: (RA,Dec) = (25.678767, 61.991766) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:42:42.904, +61:59:30.359).
Field size: 15.7292 x 10.539 degrees
Field rotation angle: up is -2.30082 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.new"...
renamed 'wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.new' -> 'wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits'
renamed 'wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.new' -> 'wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits'
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits was not found.
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Generating wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat from image00004.cat
Generating wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat from image00003.cat
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits created.
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits created.
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Image size: 938.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:44.302 +61:59:29.90 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 938.9'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:43.310 +61:59:33.46 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 17121 stars ###
### Converted positions of 17919 stars ###
'wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/correct_sextractor_wcs_catalog_usingxy2sky2269262.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/correct_sextractor_wcs_catalog_usingxy2sky2269264.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
Image size: 938.9'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:43.310 +61:59:33.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:43.310 +61:59:33.46
Angular distance between the image centers 0.0295 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Image size: 938.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:44.302 +61:59:29.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:44.302 +61:59:29.90
Angular distance between the image centers 0.0312 deg.
###################################
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=N/A worst_q_ratio=N/A
ref2=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=N/A worst_q_ratio=N/A
new1=wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits sigma_overall=N/A worst_q_ratio=N/A
new2=wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits sigma_overall=N/A worst_q_ratio=N/A
reference average sigma_overall=N/A worst_q_ratio=N/A
warn-on-ratio threshold: 2.0x reference
###################################
INFO: WCS quality sigma_overall_arcsec not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality sigma_overall_arcsec not available for comparison (2nd new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (2nd new image new=N/A ref_avg=N/A)
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:42:43.310 +61:59:33.46
Second-epoch second image center 01:42:44.302 +61:59:29.90
Angular distance between the image centers 0.00218 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.LQecnadzPy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.SZpWWQCYqn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits &> /tmp/tmp.HMWsQXo8CD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits &> /tmp/tmp.C4macFC1cR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929150
a=0.000000 b=1.000000 c=22.929150
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=5.8)
Read 31681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.0659 to 45.7628 deg, Dec +55.3336 to +67.4023 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.0659 to 45.7628 deg, Dec 55.3336 to 67.4023 deg
Loaded 26179 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 14497 out of 16269 total matches.
Matched with Tycho-2 16269 out of 31681 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
14.4 mag. fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
14.5 mag. fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.LQecnadzPy (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, passed=31559
Got 31559 stars (including 27744 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 31559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 280 matched stars entering correct_measured_positions(), 228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 266 matched stars entering correct_measured_positions(), 9996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 403 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 337 matched stars entering correct_measured_positions(), 10041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.88"
Excluding outliers - 331 stars left (next iteration limit 292)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=331 sigma_overall_arcsec=7.729 sigma_q1_arcsec=31.346 sigma_q2_arcsec=12.794 sigma_q3_arcsec=22.422 sigma_q4_arcsec=4.202 n_q1=16 n_q2=97 n_q3=37 n_q4=181 worst_quadrant_to_overall_ratio=4.055
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.SZpWWQCYqn (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, passed=31681
Got 31681 stars (including 27947 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 31681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=973 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.346 n_q1=119 n_q2=244 n_q3=303 n_q4=307 worst_quadrant_to_overall_ratio=1.316
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.HMWsQXo8CD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1343, passed=17121
Got 17121 stars (including 15774 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat
util/solve_plate_with_UCAC5 got 17121 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 16758 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 16758 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 16758 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
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=fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits N_match=973 sigma_overall_arcsec=0.644 sigma_q1_arcsec=0.538 sigma_q2_arcsec=0.582 sigma_q3_arcsec=0.742 sigma_q4_arcsec=0.880 n_q1=268 n_q2=330 n_q3=208 n_q4=167 worst_quadrant_to_overall_ratio=1.366
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.C4macFC1cR (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1315, passed=17919
Got 17919 stars (including 16601 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat
util/solve_plate_with_UCAC5 got 17919 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
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: 973 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 17586 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
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(), 17587 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 17587 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 972 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits N_match=972 sigma_overall_arcsec=0.693 sigma_q1_arcsec=0.679 sigma_q2_arcsec=0.651 sigma_q3_arcsec=0.574 sigma_q4_arcsec=0.863 n_q1=276 n_q2=330 n_q3=198 n_q4=168 worst_quadrant_to_overall_ratio=1.246
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52684_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 52684_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:19:46.45 +58:12:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 08339_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:20:32.48 +62:32:01.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
Entering WCS image calibration mode.
Entering WCS image calibration mode.
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits was not set. Trying to guess...
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits was not set. Trying to guess...
The guess is 605 arcmin.
The guess is 605 arcmin.
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits was not found.
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
It's a known telescope with plate solutions that are supposed to be good.
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits was not set. Trying to guess...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits was not set. Trying to guess...
The guess is 570 arcmin.
The guess is 569 arcmin.
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits was not found.
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Generating wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat from image00003.cat
Generating wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat from image00004.cat
Generating wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat from image00001.cat
Generating wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat from image00002.cat
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits created.
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits created.
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Image size: 938.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:44.302 +61:59:29.90 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 938.9'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:43.310 +61:59:33.46 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits created.
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits created.
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:54.565 +61:59:40.70 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 120804 stars ###
### Converted positions of 121572 stars ###
'wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/correct_sextractor_wcs_catalog_usingxy2sky2448338.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/correct_sextractor_wcs_catalog_usingxy2sky2448334.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
### Converted positions of 222556 stars ###
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
### Converted positions of 218998 stars ###
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/correct_sextractor_wcs_catalog_usingxy2sky2448912.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/correct_sextractor_wcs_catalog_usingxy2sky2448929.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
Image size: 938.9'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:43.310 +61:59:33.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:43.310 +61:59:33.46
Angular distance between the image centers 0.0295 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Image size: 938.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:44.302 +61:59:29.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:44.302 +61:59:29.90
Angular distance between the image centers 0.0312 deg.
###################################
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=N/A worst_q_ratio=N/A
ref2=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=N/A worst_q_ratio=N/A
new1=wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits sigma_overall=N/A worst_q_ratio=N/A
new2=wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits sigma_overall=N/A worst_q_ratio=N/A
reference average sigma_overall=N/A worst_q_ratio=N/A
warn-on-ratio threshold: 2.0x reference
###################################
INFO: WCS quality sigma_overall_arcsec not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality sigma_overall_arcsec not available for comparison (2nd new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (2nd new image new=N/A ref_avg=N/A)
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:42:43.310 +61:59:33.46
Second-epoch second image center 01:42:44.302 +61:59:29.90
Angular distance between the image centers 0.00218 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.mf5O96koSV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.qoThMV1hYD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits &> /tmp/tmp.jenXaEtNQi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits &> /tmp/tmp.fy3IOiCR1c
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.035150
a=0.000000 b=1.000000 c=20.035150
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 12.76
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 12.76
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=4.4)
Read 218998 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9707 to 45.8168 deg, Dec +55.3262 to +67.4140 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 6.9707 to 45.8168 deg, Dec 55.3262 to 67.4140 deg
Loaded 26295 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10859 out of 16691 total matches.
Matched with Tycho-2 16691 out of 218998 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 195 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.0 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
2.0 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.0 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
12.8 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
12.7 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
11.8 mag. fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
11.8 mag. fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
All-image limiting magnitude estimate: 11.8 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.mf5O96koSV (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=35398, passed=222522
Got 222522 stars (including 186791 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 222522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 368 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 275 matched stars entering correct_measured_positions(), 212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.82"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 264 matched stars entering correct_measured_positions(), 49591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 434 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 49636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
Accuracy estimation diagnostic: 344 matched stars entering correct_measured_positions(), 64908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.78"
Excluding outliers - 344 stars left (next iteration limit 290)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=344 sigma_overall_arcsec=7.924 sigma_q1_arcsec=24.049 sigma_q2_arcsec=13.165 sigma_q3_arcsec=21.493 sigma_q4_arcsec=4.815 n_q1=16 n_q2=127 n_q3=29 n_q4=172 worst_quadrant_to_overall_ratio=3.035
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qoThMV1hYD (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=35098, passed=218974
Got 218974 stars (including 183551 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 218974 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=974 sigma_overall_arcsec=0.370 sigma_q1_arcsec=0.448 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.374 sigma_q4_arcsec=0.313 n_q1=145 n_q2=246 n_q3=288 n_q4=295 worst_quadrant_to_overall_ratio=1.210
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.jenXaEtNQi (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=13086, passed=121549
Got 121549 stars (including 108334 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat
util/solve_plate_with_UCAC5 got 121549 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
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: 973 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 119717 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 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(), 119715 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 119716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 972 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits N_match=972 sigma_overall_arcsec=0.623 sigma_q1_arcsec=0.563 sigma_q2_arcsec=0.544 sigma_q3_arcsec=0.652 sigma_q4_arcsec=0.792 n_q1=269 n_q2=317 n_q3=209 n_q4=177 worst_quadrant_to_overall_ratio=1.272
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fy3IOiCR1c (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=12995, passed=120786
Got 120786 stars (including 107667 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat
util/solve_plate_with_UCAC5 got 120786 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 118337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 118339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 118341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits N_match=968 sigma_overall_arcsec=0.651 sigma_q1_arcsec=0.634 sigma_q2_arcsec=0.610 sigma_q3_arcsec=0.545 sigma_q4_arcsec=0.795 n_q1=278 n_q2=294 n_q3=222 n_q4=174 worst_quadrant_to_overall_ratio=1.222
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-41-23_20.00sec_-4.90C_LIGHT_0420.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cas-03-Q2b1x1_054103_TTUQ2b1x1_1230446_Cm9Qt5fZ/wcs_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421.fits
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:56.88 +62:15:29.3: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:20.08 +61:29:38.6: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:35.27 +63:50:26.2: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:15.88 +58:53:23.0: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:41.28 +61:18:08.3: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:41.40 +59:04:48.2: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:54.96 +65:15:24.2: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:12.61 +61:16:56.8: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:18.30 +63:15:50.2: 12.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:45.50 +58:34:14.5: 12.61 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:15.88 +58:53:23.0: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:35.27 +63:50:26.2: 14.74 +/- 0.09 detection
Forced photometry filter KEPT candidate at 01:39:15.88 +58:53:23.0: ref_mag=13.92 +/- 0.05 new_mean_mag=10.9804 delta=2.94 (need > 0.90)
Forced photometry reference-image weighted average: 14.74 +/- 0.09
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:41.40 +59:04:48.2: 14.14 +/- 0.06 detection
Forced photometry filter KEPT candidate at 01:18:35.27 +63:50:26.2: ref_mag=14.74 +/- 0.09 new_mean_mag=11.4052 delta=3.33 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:56.88 +62:15:29.3: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.06
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:20.08 +61:29:38.6: 14.02 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:41.28 +61:18:08.3: 13.96 +/- 0.06 detection
Forced photometry filter KEPT candidate at 01:27:41.40 +59:04:48.2: ref_mag=14.14 +/- 0.06 new_mean_mag=11.1011 delta=3.03 (need > 0.90)
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Forced photometry reference-image weighted average: 14.02 +/- 0.06
Forced photometry filter KEPT candidate at 01:23:56.88 +62:15:29.3: ref_mag=14.17 +/- 0.06 new_mean_mag=11.3349 delta=2.83 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:54.96 +65:15:24.2: 13.99 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:12.61 +61:16:56.8: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.06
Forced photometry filter KEPT candidate at 01:13:20.08 +61:29:38.6: ref_mag=14.02 +/- 0.06 new_mean_mag=11.1800 delta=2.84 (need > 0.90)
Forced photometry filter KEPT candidate at 01:12:41.28 +61:18:08.3: ref_mag=13.96 +/- 0.06 new_mean_mag=11.1907 delta=2.77 (need > 0.90)
Forced photometry reference-image weighted average: 13.99 +/- 0.05
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Forced photometry filter KEPT candidate at 01:33:12.61 +61:16:56.8: ref_mag=13.99 +/- 0.05 new_mean_mag=11.3412 delta=2.65 (need > 0.90)
Forced photometry filter KEPT candidate at 02:09:54.96 +65:15:24.2: ref_mag=13.99 +/- 0.06 new_mean_mag=11.3906 delta=2.60 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:45.50 +58:34:14.5: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Forced photometry filter KEPT candidate at 01:21:45.50 +58:34:14.5: ref_mag=13.84 +/- 0.05 new_mean_mag=11.0857 delta=2.76 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:18.30 +63:15:50.2: 13.61 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.06
Forced photometry filter KEPT candidate at 01:29:18.30 +63:15:50.2: ref_mag=13.61 +/- 0.06 new_mean_mag=11.1460 delta=2.46 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:47.78 +57:25:43.5: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:47.78 +57:25:43.5: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.06
Forced photometry filter KEPT candidate at 01:17:47.78 +57:25:43.5: ref_mag=13.96 +/- 0.06 new_mean_mag=11.0921 delta=2.87 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:40.89 +60:51:26.3: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:40.89 +60:51:26.3: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.05
Forced photometry filter KEPT candidate at 01:13:40.89 +60:51:26.3: ref_mag=13.77 +/- 0.05 new_mean_mag=10.9969 delta=2.77 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:33.14 +60:44:42.2: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:08.00 +58:54:08.3: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:33.14 +60:44:42.2: 14.10 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.06
Forced photometry filter KEPT candidate at 01:22:33.14 +60:44:42.2: ref_mag=14.10 +/- 0.06 new_mean_mag=11.1711 delta=2.93 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:01.08 +64:42:20.0: 11.65 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.52 +59:01:15.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:08.00 +58:54:08.3: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Forced photometry filter KEPT candidate at 01:43:08.00 +58:54:08.3: ref_mag=13.67 +/- 0.04 new_mean_mag=10.9358 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:01.08 +64:42:20.0: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.04
Forced photometry filter KEPT candidate at 01:12:01.08 +64:42:20.0: ref_mag=13.22 +/- 0.04 new_mean_mag=11.0977 delta=2.13 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.52 +59:01:15.6: 13.94 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.06
Forced photometry filter KEPT candidate at 01:26:05.52 +59:01:15.6: ref_mag=13.94 +/- 0.06 new_mean_mag=10.9904 delta=2.95 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.43 +59:59:17.3: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.43 +59:59:17.3: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Forced photometry filter KEPT candidate at 01:07:39.43 +59:59:17.3: ref_mag=13.70 +/- 0.04 new_mean_mag=11.0119 delta=2.69 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:05:21.38 +64:15:22.1: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:21.38 +64:15:22.1: 13.80 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.06
Forced photometry filter KEPT candidate at 01:05:21.38 +64:15:22.1: ref_mag=13.80 +/- 0.06 new_mean_mag=10.9867 delta=2.81 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:38.91 +59:41:40.1: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:45.74 +59:01:23.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:38.91 +59:41:40.1: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Forced photometry filter KEPT candidate at 01:26:38.91 +59:41:40.1: ref_mag=13.46 +/- 0.04 new_mean_mag=10.6657 delta=2.79 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:45.74 +59:01:23.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Forced photometry filter KEPT candidate at 01:25:45.74 +59:01:23.4: ref_mag=13.59 +/- 0.04 new_mean_mag=10.6997 delta=2.89 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:07.81 +59:42:42.9: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:07.81 +59:42:42.9: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter KEPT candidate at 01:39:07.81 +59:42:42.9: ref_mag=12.84 +/- 0.02 new_mean_mag=10.3182 delta=2.52 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:25.50 +63:41:28.0: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:25.50 +63:41:28.0: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter KEPT candidate at 01:37:25.50 +63:41:28.0: ref_mag=13.27 +/- 0.03 new_mean_mag=10.2849 delta=2.98 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:14.86 +61:08:19.1: 12.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:14.86 +61:08:19.1: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Forced photometry filter KEPT candidate at 01:11:14.86 +61:08:19.1: ref_mag=12.71 +/- 0.02 new_mean_mag=9.9328 delta=2.78 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:30.66 +63:53:02.2: 9.54 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:30.66 +63:53:02.2: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.07 +/- 0.01
Forced photometry filter KEPT candidate at 01:15:30.66 +63:53:02.2: ref_mag=11.07 +/- 0.01 new_mean_mag=9.4177 delta=1.66 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:56.63 +59:35:12.1: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:56.63 +59:35:12.1: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter KEPT candidate at 01:25:56.63 +59:35:12.1: ref_mag=11.99 +/- 0.01 new_mean_mag=9.2463 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:21.64 +64:56:38.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:21.64 +64:56:38.6: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Forced photometry filter KEPT candidate at 02:00:21.64 +64:56:38.6: ref_mag=13.47 +/- 0.04 new_mean_mag=10.5913 delta=2.88 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:41.74 +62:51:06.7: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:41.74 +62:51:06.7: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Forced photometry filter KEPT candidate at 01:19:41.74 +62:51:06.7: ref_mag=13.53 +/- 0.03 new_mean_mag=10.6815 delta=2.85 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.59 +60:07:34.5: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:38.59 +60:07:34.5: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 01:46:38.59 +60:07:34.5: ref_mag=13.35 +/- 0.03 new_mean_mag=10.5319 delta=2.82 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:16.40 +60:12:25.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:16.40 +60:12:25.5: 13.54 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:21.46 +61:44:14.8: 12.77 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.54 +/- 0.04
Forced photometry filter KEPT candidate at 01:36:16.40 +60:12:25.5: ref_mag=13.54 +/- 0.04 new_mean_mag=10.7492 delta=2.79 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:21.46 +61:44:14.8: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Forced photometry filter KEPT candidate at 01:29:21.46 +61:44:14.8: ref_mag=13.61 +/- 0.04 new_mean_mag=10.7813 delta=2.83 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.52 +59:18:56.0: 13.08 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.52 +59:18:56.0: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.05
Forced photometry filter KEPT candidate at 01:06:55.52 +59:18:56.0: ref_mag=13.83 +/- 0.05 new_mean_mag=10.8872 delta=2.95 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:48.52 +64:12:23.2: 11.79 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:48.52 +64:12:23.2: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.05
Forced photometry filter KEPT candidate at 01:18:48.52 +64:12:23.2: ref_mag=13.43 +/- 0.05 new_mean_mag=10.8586 delta=2.57 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:03.34 +61:54:44.9: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:03.34 +61:54:44.9: 13.94 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.12
Forced photometry filter KEPT candidate at 01:44:03.34 +61:54:44.9: ref_mag=13.94 +/- 0.12 new_mean_mag=10.9051 delta=3.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:11.02 +59:09:04.3: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:11.02 +59:09:04.3: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.05
Forced photometry filter KEPT candidate at 01:22:11.02 +59:09:04.3: ref_mag=13.75 +/- 0.05 new_mean_mag=10.9328 delta=2.82 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:39.80 +62:00:55.7: 13.28 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:39.80 +62:00:55.7: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Forced photometry filter KEPT candidate at 01:50:39.80 +62:00:55.7: ref_mag=13.93 +/- 0.05 new_mean_mag=10.9987 delta=2.93 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:41.59 +58:46:46.7: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:41.59 +58:46:46.7: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.05
Forced photometry filter KEPT candidate at 01:14:41.59 +58:46:46.7: ref_mag=13.83 +/- 0.05 new_mean_mag=10.8901 delta=2.94 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:40.44 +61:07:36.9: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:40.44 +61:07:36.9: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.06
Forced photometry filter KEPT candidate at 01:32:40.44 +61:07:36.9: ref_mag=13.76 +/- 0.06 new_mean_mag=10.8663 delta=2.89 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:05.89 +61:04:13.2: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:05.89 +61:04:13.2: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.06
Forced photometry filter KEPT candidate at 01:38:05.89 +61:04:13.2: ref_mag=13.87 +/- 0.06 new_mean_mag=10.9941 delta=2.88 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:50.76 +59:55:50.2: 12.64 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:11.25 +60:52:42.7: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:22.71 +57:26:31.0: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:50.76 +59:55:50.2: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Forced photometry filter KEPT candidate at 01:36:50.76 +59:55:50.2: ref_mag=13.89 +/- 0.05 new_mean_mag=11.0372 delta=2.85 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:11.25 +60:52:42.7: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.07
Forced photometry filter KEPT candidate at 01:15:11.25 +60:52:42.7: ref_mag=14.01 +/- 0.07 new_mean_mag=11.0333 delta=2.98 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.71 +57:26:31.0: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Forced photometry filter KEPT candidate at 01:09:22.71 +57:26:31.0: ref_mag=13.90 +/- 0.05 new_mean_mag=11.0814 delta=2.82 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:32.86 +59:40:05.4: 11.56 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.86 +59:40:05.4: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.05
Forced photometry filter KEPT candidate at 02:00:32.86 +59:40:05.4: ref_mag=12.95 +/- 0.05 new_mean_mag=10.8596 delta=2.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.61 +64:22:27.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.61 +64:22:27.5: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Forced photometry filter KEPT candidate at 01:31:48.61 +64:22:27.5: ref_mag=13.99 +/- 0.06 new_mean_mag=11.0856 delta=2.90 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:34.22 +63:37:08.3: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:34.22 +63:37:08.3: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.05
Forced photometry filter KEPT candidate at 01:59:34.22 +63:37:08.3: ref_mag=13.88 +/- 0.05 new_mean_mag=11.0903 delta=2.79 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:15.55 +61:53:39.0: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:15.55 +61:53:39.0: 14.03 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.15
Forced photometry filter KEPT candidate at 01:44:15.55 +61:53:39.0: ref_mag=14.03 +/- 0.15 new_mean_mag=11.0433 delta=2.98 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:25.11 +64:38:23.6: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:25.11 +64:38:23.6: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Forced photometry filter KEPT candidate at 02:02:25.11 +64:38:23.6: ref_mag=14.03 +/- 0.06 new_mean_mag=10.9949 delta=3.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:35.72 +64:48:50.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:35.72 +64:48:50.3: 14.23 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.07
Forced photometry filter KEPT candidate at 01:38:35.72 +64:48:50.3: ref_mag=14.23 +/- 0.07 new_mean_mag=11.2858 delta=2.94 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:22.27 +60:45:17.6: 11.86 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:22.27 +60:45:17.6: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.07
Forced photometry filter KEPT candidate at 01:40:22.27 +60:45:17.6: ref_mag=13.25 +/- 0.07 new_mean_mag=11.2289 delta=2.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:26.87 +61:39:56.3: 13.22 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:26.87 +61:39:56.3: 14.42 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.07
Forced photometry filter KEPT candidate at 01:23:26.87 +61:39:56.3: ref_mag=14.36 +/- 0.07 new_mean_mag=11.4582 delta=2.90 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:06.89 +64:35:49.8: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:06.89 +64:35:49.8: 14.25 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.07
Forced photometry filter KEPT candidate at 02:01:06.89 +64:35:49.8: ref_mag=14.25 +/- 0.07 new_mean_mag=11.4205 delta=2.83 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:40.27 +62:34:08.6: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:40.27 +62:34:08.6: 14.61 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.08
Forced photometry filter KEPT candidate at 01:41:40.27 +62:34:08.6: ref_mag=14.61 +/- 0.08 new_mean_mag=11.7540 delta=2.86 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:06.79 +61:26:14.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:06.79 +61:26:14.9: 14.76 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.14
Forced photometry filter KEPT candidate at 01:27:06.79 +61:26:14.9: ref_mag=14.76 +/- 0.14 new_mean_mag=11.7300 delta=3.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:18.16 +61:15:41.0: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:18.16 +61:15:41.0: 14.88 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.15
Forced photometry filter KEPT candidate at 01:17:18.16 +61:15:41.0: ref_mag=14.88 +/- 0.15 new_mean_mag=11.8209 delta=3.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:47.36 +63:11:26.1: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:47.36 +63:11:26.1: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Forced photometry filter KEPT candidate at 02:13:47.36 +63:11:26.1: ref_mag=13.95 +/- 0.05 new_mean_mag=10.1579 delta=3.79 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:23.54 +65:01:38.2: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:23.54 +65:01:38.2: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Forced photometry filter KEPT candidate at 02:15:23.54 +65:01:38.2: ref_mag=12.62 +/- 0.02 new_mean_mag=8.9109 delta=3.70 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:44.46 +60:46:16.7: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:44.46 +60:46:16.7: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter KEPT candidate at 01:33:44.46 +60:46:16.7: ref_mag=13.42 +/- 0.03 new_mean_mag=10.7800 delta=2.64 (need > 0.90)
Adding exclusion_list_local.txt__out125111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out272395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out272400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out273512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out274365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out276505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out276591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out276792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58464.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 85s
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: 36s
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Considering the candidate 247637_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247637_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247660_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247660_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247662_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247662_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247665_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247665_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:30:06.68 +61:51:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247667_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247667_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247672_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247672_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247675_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247675_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:45:21.33 +65:13:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247676_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247676_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247681_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247681_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247682_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247682_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247686_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247686_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247697_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247697_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247700_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247700_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247702_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247702_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247704_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247704_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247707_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247707_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247710_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247710_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 247727_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247727_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247728_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247728_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247729_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247729_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247736_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247736_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247746_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247746_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:07:41.90 +60:54:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247753_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247753_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247755_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247755_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 247756_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247756_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247758_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247758_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:39:24.08 +58:23:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247760_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247760_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:33:35.35 +59:56:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247761_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247761_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247767_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247767_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247771_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247771_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:05:57.23 +63:03:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247775_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247775_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:32:21.94 +60:27:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247783_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247783_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247787_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247787_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:14:45.20 +60:30:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247790_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247790_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:25:15.38 +64:40:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247796_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247796_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247799_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247799_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247802_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247802_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:55:14.52 +59:32:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247807_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247807_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247808_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247808_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:19:48.72 +61:38:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247809_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 247809_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 247811_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247811_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247813_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247813_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:16:01.05 +62:41:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247814_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 247814_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:22:08.34 +60:22:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250799_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 250799_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 251840_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 251840_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:44:02.01 +61:53:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252481_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 252481_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 252545_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 252545_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 252602_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 252602_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 252666_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 252666_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 252712_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 252712_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:38:00.49 +57:56:46.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253407_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 253407_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:17:59.22 +57:47:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253663_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 253663_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 254601_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 254601_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 254690_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 254690_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:26:41.17 +60:46:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256051_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 256051_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:58:16.35 +59:38:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256329_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 256329_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:18:14.21 +61:44:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257097_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 257097_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:20:10.92 +58:12:10.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 257324_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 257324_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:43:53.07 +61:53:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257730_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 257730_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:21:28.15 +57:48:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257756_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 257756_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:19:12.49 +65:36:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257857_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 257857_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:16:08.73 +58:49:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257885_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 257885_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:46:33.66 +61:16:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258125_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 258125_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:44:17.76 +61:53:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258552_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 258552_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:51:02.56 +64:49:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258830_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 258830_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 259171_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 259171_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:15:58.89 +63:12:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259944_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 259944_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:11:23.01 +61:21:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260294_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 260294_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:19:22.28 +58:19:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260517_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 260517_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:02:54.86 +64:24:59.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 260629_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 260629_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 260876_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 260876_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:13:30.52 +58:34:25.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 260972_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 260972_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:33:23.23 +57:44:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261333_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 261333_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:15:11.64 +60:07:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261482_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 261482_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:17:00.85 +61:40:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261837_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 261837_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:37:44.72 +64:45:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262147_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 262147_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:06:23.53 +62:44:02.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262178_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 262178_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:16:05.01 +58:49:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262183_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 262183_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:35:54.24 +60:13:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262248_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 262248_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:19:03.75 +63:57:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262274_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 262274_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:04:26.76 +65:05:53.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262529_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 262529_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:43:06.98 +58:57:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262558_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 262558_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:27:02.28 +58:03:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262651_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 262651_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:58:40.07 +59:15:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262829_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 262829_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:13:36.10 +57:52:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262830_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 262830_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 262870_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 262870_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:06:45.45 +59:50:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262881_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 262881_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 262885_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 262885_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:35:50.57 +61:27:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263203_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 263203_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:11:50.24 +59:02:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263273_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 263273_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 263274_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 263274_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:10:23.71 +60:01:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263302_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 263302_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 263309_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 263309_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:48:38.15 +61:49:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263409_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 263409_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:47:19.01 +63:38:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263472_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 263472_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:38:08.26 +61:03:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263744_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 263744_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 263754_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 263754_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 263806_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 263806_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:39:56.84 +60:52:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263852_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 263852_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:44:56.69 +59:46:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264018_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 264018_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:34:10.35 +62:09:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264441_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 264441_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 264573_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 264573_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 264574_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 264574_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 264725_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 264725_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:38:33.81 +60:47:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264778_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 264778_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 264804_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 264804_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:33:24.69 +58:21:30.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 265038_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 265038_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:31:32.47 +61:02:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265133_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 265133_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:02:53.92 +60:15:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265143_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 265143_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:55:52.96 +64:15:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265233_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 265233_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 265256_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 265256_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:31:29.27 +58:12:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265544_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 265544_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 265592_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 265592_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:38:07.65 +61:01:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265642_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 265642_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:20:40.68 +60:23:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265680_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 265680_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:16:24.24 +58:04:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265800_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 265800_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 266037_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 266037_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:16:36.95 +64:56:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266080_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 266080_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:42:55.06 +64:01:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266133_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 266133_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 266166_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 266166_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:46:18.23 +60:59:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266179_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 266179_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:38:12.04 +61:01:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266287_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 266287_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 266528_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 266528_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:10:32.51 +59:59:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266640_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 266640_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 267114_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 267114_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:33:46.57 +62:31:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267196_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 267196_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:23:07.66 +61:11:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267214_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 267214_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 267220_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 267220_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 267288_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 267288_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 267311_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 267311_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:18:04.37 +65:36:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267379_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 267379_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:14:00.32 +61:42:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267662_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 267662_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 267760_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 267760_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 267838_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 267838_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:02:50.48 +60:14:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267841_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 267841_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 267842_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 267842_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:42:26.67 +59:34:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267862_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 267862_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:43:03.32 +58:57:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268038_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 268038_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 268199_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 268199_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:56:25.56 +62:05:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268283_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 268283_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 268308_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 268308_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:14:00.69 +59:02:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268350_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 268350_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 268427_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 268427_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:59:06.09 +59:55:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268451_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 268451_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:27:56.49 +62:46:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268469_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 268469_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 268497_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 268497_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:34:34.67 +65:48:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268543_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 268543_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 268594_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 268594_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 268890_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 268890_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 269039_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 269039_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 269106_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 269106_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:20:49.51 +64:40:20.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 269349_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 269349_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
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Considering the candidate 269366_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 269366_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269377_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 269377_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269455_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 269455_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269505_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 269505_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:32:54.21 +60:17:24.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269576_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 269576_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:34:42.39 +58:42:16.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269804_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 269804_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:44:32.42 +61:36:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270316_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 270316_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:36:13.69 +60:49:01.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270357_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 270357_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:49:06.22 +65:23:43.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270396_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 270396_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270462_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 270462_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:38:57.03 +63:28:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271081_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 271081_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271381_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 271381_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271532_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 271532_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:27:03.94 +64:43:36.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271588_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 271588_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:14:21.88 +59:59:52.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271808_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 271808_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:55:05.07 +59:57:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271898_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 271898_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271947_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 271947_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272266_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 272266_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272395_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 272395_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272399_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 272399_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272400_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 272400_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272516_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 272516_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272696_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 272696_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272911_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 272911_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 273512_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 273512_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 273563_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 273563_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:41:41.28 +57:56:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 273579_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 273579_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:17:01.79 +63:21:39.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 274365_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 274365_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 274939_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 274939_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 276505_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 276505_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 276591_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 276591_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 276792_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 276792_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 39378_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:47:55.71 +64:32:55.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 70271_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:20:32.45 +62:32:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 72532_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:45:35.77 +63:07:04.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189361_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 189361_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58464_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 58464_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21138_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 21138_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125111_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
Preparing report for the candidate 125111_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 112593_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 01:21:55.14 +61:20:57.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95057_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 95057_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120880_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 120880_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76113_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421
The candidate 76113_fd_Cas-03-Q2b1x1_2026-05-12_04-44-37_20.00sec_-5.00C_LIGHT_0421 did not pass the final checks
**** FOUND 02:02:02.17 +62:41:31.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 124s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:33:44.46 +60:46:16.7
02:15:23.54 +65:01:38.2
02:09:54.96 +65:15:24.2
01:33:12.61 +61:16:56.8
01:12:41.28 +61:18:08.3
01:23:56.88 +62:15:29.3
01:13:20.08 +61:29:38.6
01:18:35.27 +63:50:26.2
01:39:15.88 +58:53:23.0
01:27:41.40 +59:04:48.2
01:29:18.30 +63:15:50.2
01:21:45.50 +58:34:14.5
01:17:47.78 +57:25:43.5
01:13:40.89 +60:51:26.3
01:22:33.14 +60:44:42.2
01:43:08.00 +58:54:08.3
01:12:01.08 +64:42:20.0
01:26:05.52 +59:01:15.6
01:07:39.43 +59:59:17.3
01:05:21.38 +64:15:22.1
01:26:38.91 +59:41:40.1
01:25:45.74 +59:01:23.4
01:39:07.81 +59:42:42.9
01:37:25.50 +63:41:28.0
01:11:14.86 +61:08:19.1
01:15:30.66 +63:53:02.2
01:25:56.63 +59:35:12.1
02:00:21.64 +64:56:38.6
01:19:41.74 +62:51:06.7
01:46:38.59 +60:07:34.5
01:36:16.40 +60:12:25.5
01:29:21.46 +61:44:14.8
01:06:55.52 +59:18:56.0
01:18:48.52 +64:12:23.2
01:44:03.34 +61:54:44.9
01:22:11.02 +59:09:04.3
01:50:39.80 +62:00:55.7
01:14:41.59 +58:46:46.7
01:32:40.44 +61:07:36.9
01:38:05.89 +61:04:13.2
01:36:50.76 +59:55:50.2
01:15:11.25 +60:52:42.7
01:09:22.71 +57:26:31.0
02:00:32.86 +59:40:05.4
01:31:48.61 +64:22:27.5
01:59:34.22 +63:37:08.3
01:44:15.55 +61:53:39.0
02:02:25.11 +64:38:23.6
01:38:35.72 +64:48:50.3
01:40:22.27 +60:45:17.6
01:23:26.87 +61:39:56.3
02:01:06.89 +64:35:49.8
01:41:40.27 +62:34:08.6
01:27:06.79 +61:26:14.9
01:17:18.16 +61:15:41.0
02:13:47.36 +63:11:26.1
########### Completed Cas-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
02:09:54.96 +65:15:24.2
01:33:12.61 +61:16:56.8
01:12:41.28 +61:18:08.3
01:23:56.88 +62:15:29.3
01:13:20.08 +61:29:38.6
01:18:35.27 +63:50:26.2
01:39:15.88 +58:53:23.0
01:27:41.40 +59:04:48.2
01:29:18.30 +63:15:50.2
01:21:45.50 +58:34:14.5
01:17:47.78 +57:25:43.5
01:13:40.89 +60:51:26.3
01:22:33.14 +60:44:42.2
01:43:08.00 +58:54:08.3
01:12:01.08 +64:42:20.0
01:26:05.52 +59:01:15.6
01:07:39.43 +59:59:17.3
01:05:21.38 +64:15:22.1
01:26:38.91 +59:41:40.1
01:25:45.74 +59:01:23.4
01:39:07.81 +59:42:42.9
01:37:25.50 +63:41:28.0
01:11:14.86 +61:08:19.1
01:15:30.66 +63:53:02.2
01:25:56.63 +59:35:12.1
02:00:21.64 +64:56:38.6
01:19:41.74 +62:51:06.7
01:46:38.59 +60:07:34.5
01:36:16.40 +60:12:25.5
01:29:21.46 +61:44:14.8
01:06:55.52 +59:18:56.0
01:18:48.52 +64:12:23.2
01:44:03.34 +61:54:44.9
01:22:11.02 +59:09:04.3
01:50:39.80 +62:00:55.7
01:14:41.59 +58:46:46.7
01:32:40.44 +61:07:36.9
01:38:05.89 +61:04:13.2
01:36:50.76 +59:55:50.2
01:15:11.25 +60:52:42.7
01:09:22.71 +57:26:31.0
02:00:32.86 +59:40:05.4
01:31:48.61 +64:22:27.5
01:59:34.22 +63:37:08.3
01:44:15.55 +61:53:39.0
02:02:25.11 +64:38:23.6
01:38:35.72 +64:48:50.3
01:40:22.27 +60:45:17.6
01:23:26.87 +61:39:56.3
02:01:06.89 +64:35:49.8
01:41:40.27 +62:34:08.6
01:27:06.79 +61:26:14.9
01:17:18.16 +61:15:41.0
02:13:47.36 +63:11:26.1
02:15:23.54 +65:01:38.2
01:33:44.46 +60:46:16.7
###################################################################################
02:09:54.96 +65:15:24.2 -- not an asteroid (will add it to exclusion list)
01:33:12.61 +61:16:56.8 -- not an asteroid (will add it to exclusion list)
01:12:41.28 +61:18:08.3 -- not an asteroid (will add it to exclusion list)
01:23:56.88 +62:15:29.3 -- not an asteroid (will add it to exclusion list)
01:13:20.08 +61:29:38.6 -- not an asteroid (will add it to exclusion list)
01:18:35.27 +63:50:26.2 -- not an asteroid (will add it to exclusion list)
01:39:15.88 +58:53:23.0 -- not an asteroid (will add it to exclusion list)
01:27:41.40 +59:04:48.2 -- not an asteroid (will add it to exclusion list)
01:29:18.30 +63:15:50.2 -- not an asteroid (will add it to exclusion list)
01:21:45.50 +58:34:14.5 -- not an asteroid (will add it to exclusion list)
01:17:47.78 +57:25:43.5 -- not an asteroid (will add it to exclusion list)
01:13:40.89 +60:51:26.3 -- not an asteroid (will add it to exclusion list)
01:22:33.14 +60:44:42.2 -- not an asteroid (will add it to exclusion list)
01:43:08.00 +58:54:08.3 -- not an asteroid (will add it to exclusion list)
01:12:01.08 +64:42:20.0 -- not an asteroid (will add it to exclusion list)
01:26:05.52 +59:01:15.6 -- not an asteroid (will add it to exclusion list)
01:07:39.43 +59:59:17.3 -- not an asteroid (will add it to exclusion list)
01:05:21.38 +64:15:22.1 -- not an asteroid (will add it to exclusion list)
01:26:38.91 +59:41:40.1 -- not an asteroid (will add it to exclusion list)
01:25:45.74 +59:01:23.4 -- not an asteroid (will add it to exclusion list)
01:39:07.81 +59:42:42.9 -- not an asteroid (will add it to exclusion list)
01:37:25.50 +63:41:28.0 -- not an asteroid (will add it to exclusion list)
01:11:14.86 +61:08:19.1 -- not an asteroid (will add it to exclusion list)
01:15:30.66 +63:53:02.2 -- not an asteroid (will add it to exclusion list)
01:25:56.63 +59:35:12.1 -- not an asteroid (will add it to exclusion list)
02:00:21.64 +64:56:38.6 -- not an asteroid (will add it to exclusion list)
01:19:41.74 +62:51:06.7 -- not an asteroid (will add it to exclusion list)
01:46:38.59 +60:07:34.5 -- not an asteroid (will add it to exclusion list)
01:36:16.40 +60:12:25.5 -- not an asteroid (will add it to exclusion list)
01:29:21.46 +61:44:14.8 -- not an asteroid (will add it to exclusion list)
01:06:55.52 +59:18:56.0 -- not an asteroid (will add it to exclusion list)
01:18:48.52 +64:12:23.2 -- not an asteroid (will add it to exclusion list)
01:44:03.34 +61:54:44.9 -- not an asteroid (will add it to exclusion list)
01:22:11.02 +59:09:04.3 -- not an asteroid (will add it to exclusion list)
01:50:39.80 +62:00:55.7 -- not an asteroid (will add it to exclusion list)
01:14:41.59 +58:46:46.7 -- not an asteroid (will add it to exclusion list)
01:32:40.44 +61:07:36.9 -- not an asteroid (will add it to exclusion list)
01:38:05.89 +61:04:13.2 -- not an asteroid (will add it to exclusion list)
01:36:50.76 +59:55:50.2 -- not an asteroid (will add it to exclusion list)
01:15:11.25 +60:52:42.7 -- not an asteroid (will add it to exclusion list)
01:09:22.71 +57:26:31.0 -- not an asteroid (will add it to exclusion list)
02:00:32.86 +59:40:05.4 -- not an asteroid (will add it to exclusion list)
01:31:48.61 +64:22:27.5 -- not an asteroid (will add it to exclusion list)
01:59:34.22 +63:37:08.3 -- not an asteroid (will add it to exclusion list)
01:44:15.55 +61:53:39.0 -- not an asteroid (will add it to exclusion list)
02:02:25.11 +64:38:23.6 -- not an asteroid (will add it to exclusion list)
01:38:35.72 +64:48:50.3 -- not an asteroid (will add it to exclusion list)
01:40:22.27 +60:45:17.6 -- not an asteroid (will add it to exclusion list)
01:23:26.87 +61:39:56.3 -- not an asteroid (will add it to exclusion list)
02:01:06.89 +64:35:49.8 -- not an asteroid (will add it to exclusion list)
01:41:40.27 +62:34:08.6 -- not an asteroid (will add it to exclusion list)
01:27:06.79 +61:26:14.9 -- not an asteroid (will add it to exclusion list)
01:17:18.16 +61:15:41.0 -- not an asteroid (will add it to exclusion list)
02:13:47.36 +63:11:26.1 -- not an asteroid (will add it to exclusion list)
02:15:23.54 +65:01:38.2 -- not an asteroid (will add it to exclusion list)
01:33:44.46 +60:46:16.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:05:21.38 +64:15:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:55.52 +59:18:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.43 +59:59:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:22.71 +57:26:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:14.86 +61:08:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:01.08 +64:42:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:41.28 +61:18:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:20.08 +61:29:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:40.89 +60:51:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:41.59 +58:46:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:11.25 +60:52:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:30.66 +63:53:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:18.16 +61:15:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:47.78 +57:25:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:35.27 +63:50:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:48.52 +64:12:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:41.74 +62:51:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:45.50 +58:34:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:11.02 +59:09:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:33.14 +60:44:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:26.87 +61:39:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:56.88 +62:15:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:45.74 +59:01:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:56.63 +59:35:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:05.52 +59:01:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:38.91 +59:41:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:06.79 +61:26:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:41.40 +59:04:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:18.30 +63:15:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:21.46 +61:44:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.61 +64:22:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:40.44 +61:07:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:12.61 +61:16:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:44.46 +60:46:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:16.40 +60:12:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:50.76 +59:55:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:25.50 +63:41:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:05.89 +61:04:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:35.72 +64:48:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:07.81 +59:42:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:15.88 +58:53:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:22.27 +60:45:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:40.27 +62:34:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:08.00 +58:54:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:03.34 +61:54:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:15.55 +61:53:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.59 +60:07:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:39.80 +62:00:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:34.22 +63:37:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:21.64 +64:56:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:32.86 +59:40:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:06.89 +64:35:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:25.11 +64:38:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:54.96 +65:15:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:47.36 +63:11:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:23.54 +65:01:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:05:21.38 +64:15:22.1 -- not a known variable star
01:06:55.52 +59:18:56.0 -- not a known variable star
01:07:39.43 +59:59:17.3 -- not a known variable star
01:09:22.71 +57:26:31.0 -- not a known variable star
01:11:14.86 +61:08:19.1 -- a known variable star
01:12:01.08 +64:42:20.0 -- a known variable star
01:12:41.28 +61:18:08.3 -- not a known variable star
01:13:20.08 +61:29:38.6 -- a known variable star
01:13:40.89 +60:51:26.3 -- not a known variable star
01:14:41.59 +58:46:46.7 -- a known variable star
01:15:11.25 +60:52:42.7 -- not a known variable star
01:15:30.66 +63:53:02.2 -- not a known variable star
01:17:18.16 +61:15:41.0 -- not a known variable star
01:17:47.78 +57:25:43.5 -- not a known variable star
01:18:35.27 +63:50:26.2 -- not a known variable star
01:18:48.52 +64:12:23.2 -- not a known variable star
01:19:41.74 +62:51:06.7 -- not a known variable star
01:21:45.50 +58:34:14.5 -- a known variable star
01:22:11.02 +59:09:04.3 -- not a known variable star
01:22:33.14 +60:44:42.2 -- not a known variable star
01:23:26.87 +61:39:56.3 -- not a known variable star
01:23:56.88 +62:15:29.3 -- not a known variable star
01:25:45.74 +59:01:23.4 -- not a known variable star
01:25:56.63 +59:35:12.1 -- not a known variable star
01:26:05.52 +59:01:15.6 -- not a known variable star
01:26:38.91 +59:41:40.1 -- a known variable star
01:27:06.79 +61:26:14.9 -- not a known variable star
01:27:41.40 +59:04:48.2 -- not a known variable star
01:29:18.30 +63:15:50.2 -- not a known variable star
01:29:21.46 +61:44:14.8 -- not a known variable star
01:31:48.61 +64:22:27.5 -- not a known variable star
01:32:40.44 +61:07:36.9 -- not a known variable star
01:33:12.61 +61:16:56.8 -- not a known variable star
01:33:44.46 +60:46:16.7 -- not a known variable star
01:36:16.40 +60:12:25.5 -- not a known variable star
01:36:50.76 +59:55:50.2 -- a known variable star
01:37:25.50 +63:41:28.0 -- a known variable star
01:38:05.89 +61:04:13.2 -- not a known variable star
01:38:35.72 +64:48:50.3 -- not a known variable star
01:39:07.81 +59:42:42.9 -- not a known variable star
01:39:15.88 +58:53:23.0 -- not a known variable star
01:40:22.27 +60:45:17.6 -- not a known variable star
01:41:40.27 +62:34:08.6 -- not a known variable star
01:43:08.00 +58:54:08.3 -- not a known variable star
01:44:03.34 +61:54:44.9 -- not a known variable star
01:44:15.55 +61:53:39.0 -- not a known variable star
01:46:38.59 +60:07:34.5 -- not a known variable star
01:50:39.80 +62:00:55.7 -- not a known variable star
01:59:34.22 +63:37:08.3 -- not a known variable star
02:00:21.64 +64:56:38.6 -- not a known variable star
02:00:32.86 +59:40:05.4 -- a known variable star
02:01:06.89 +64:35:49.8 -- not a known variable star
02:02:25.11 +64:38:23.6 -- a known variable star
02:09:54.96 +65:15:24.2 -- not a known variable star
02:13:47.36 +63:11:26.1 -- a known variable star
02:15:23.54 +65:01:38.2 -- a known variable star
Found 44 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
56 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 56 (excluding asteroids and hot pixels, 44 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461172.90386410 -observatory V36
03:05:08.24 +17:08:57.1 Mercury (-2.1mag)
05:23:21.65 +24:32:12.7 Venus (-3.9mag)
01:32:41.84 +08:49:07.9 Mars (1.2mag)
07:27:54.39 +22:18:05.3 Jupiter (-2.0mag)
00:40:16.48 +01:56:34.1 Saturn (0.9mag)
03:53:43.46 +20:06:17.0 Uranus (5.8mag)
00:13:57.43 +00:03:57.0 Neptune (7.8mag)
20:34:13.60 -22:56:18.3 Pluto (14.5mag)
23:29:42.45 -02:37:13.2 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 May 12 06:40 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461172.90386410:
07:27:49.89 +22:18:18.1 Io (5.9mag)
07:27:58.12 +22:17:53.8 Europa (6.1mag)
07:27:55.65 +22:18:08.6 Ganymede (5.5mag)
07:27:25.63 +22:19:18.2 Callisto (6.7mag)
07:29:49.88 +21:56:29.7 Himalia (15.5mag)
07:27:54.27 +22:18:04.4 Thebe (16.4mag)
07:30:17.84 +22:23:04.8 Elara (17.4mag)
07:28:32.07 +22:44:12.8 Pasiphae (17.6mag)
07:35:30.81 +22:18:05.0 Carme (18.7mag)
00:40:26.78 +01:56:21.5 Titan (8.7mag)
00:40:12.84 +01:56:46.2 Rhea (10.0mag)
00:40:06.98 +01:54:41.3 Iapetus (11.4mag)
00:40:06.80 +01:56:56.8 Hyperion (14.7mag)
00:41:29.10 +02:02:12.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 12 06:40 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461172.90386410:
16:59:18.91 -29:37:56.2 JWST
08:25:30.01 +12:56:31.4 Chandra
09:15:21.10 -52:49:28.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 12 06:40 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461172.90386410 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
07:49:50.54 +25:13:58.5 17.7mag P/2009 WX51 (Catalina)
18:55:19.93 -30:34:46.9 13.7mag P/2010 H2 (Vales)
05:28:11.37 -68:37:21.2 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:39:41.48 +31:39:35.5 17.4mag C/2017 K2 (PANSTARRS)
17:24:42.94 +13:23:45.1 17.7mag C/2021 G2 (ATLAS)
23:14:38.93 +30:24:28.4 17.2mag C/2022 E2 (ATLAS)
05:01:00.66 +26:38:52.1 16.3mag C/2022 N2 (PANSTARRS)
09:13:08.21 +31:49:10.4 16.4mag C/2022 QE78 (ATLAS)
08:38:12.36 +02:15:48.5 17.5mag C/2022 R6 (PANSTARRS)
18:43:54.20 +20:29:32.7 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:30:19.65 -11:09:27.5 17.5mag P/2023 B1 (PANSTARRS)
09:00:15.64 -08:10:28.7 17.9mag C/2023 F3 (ATLAS)
22:13:01.43 +64:40:19.9 17.6mag C/2023 H5 (Lemmon)
18:44:40.93 -04:37:15.4 13.8mag C/2023 R1 (PANSTARRS)
15:48:29.17 +88:03:56.2 17.9mag C/2023 X2 (Lemmon)
06:38:00.44 +63:39:09.6 17.4mag C/2024 A1 (ATLAS)
06:03:48.06 +24:32:24.7 12.5mag C/2024 E1 (Wierzchos)
15:59:24.50 +10:27:29.0 17.3mag C/2024 G6 (ATLAS)
20:23:12.71 +22:56:13.0 14.3mag C/2024 J3 (ATLAS)
03:51:19.29 -18:45:51.7 16.2mag C/2024 T5 (ATLAS)
05:40:37.75 +39:26:52.9 17.8mag C/2025 J1 (Borisov)
12:09:32.30 +53:12:44.9 16.4mag C/2025 L1 (ATLAS)
05:41:27.65 -08:06:08.8 10.5mag C/2025 R3 (PANSTARRS)
12:44:08.79 +04:17:05.4 17.3mag C/2025 Y1 (ATLAS)
05:29:00.84 +01:20:25.5 17.9mag C/2026 A1 (MAPS)
01:06:52.48 +41:00:54.7 15.4mag C/2026 B2 (Sun-Gao)
19:33:45.20 -08:23:15.3 10.3mag 10P/Tempel
14:28:05.95 -00:21:40.8 16.4mag 24P/Schaumasse
10:59:01.18 -00:56:00.1 15.8mag 29P/Schwassmann-Wachmann
10:43:30.61 -02:43:04.3 17.5mag 43P/Wolf-Harrington
02:29:52.64 +21:46:49.3 17.5mag 47P/Ashbrook-Jackson
08:03:12.67 +30:55:13.7 16.9mag 63P/Wild
00:00:29.31 -08:33:37.6 15.7mag 65P/Gunn
05:18:49.40 +28:55:21.3 16.2mag 76P/West-Kohoutek-Ikemura
02:05:31.88 +13:08:46.0 14.0mag 78P/Gehrels
00:16:58.40 -01:46:26.9 15.0mag 88P/Howell
03:29:10.61 +26:43:36.9 15.1mag 93P/Lovas
05:48:57.02 +33:15:30.3 15.9mag 123P/West-Hartley
09:05:32.59 +26:21:21.4 16.3mag 124P/Mrkos
03:15:06.93 +17:05:23.5 16.4mag 128P/Shoemaker-Holt
03:39:58.15 +17:16:45.4 17.6mag 131P/Mueller
03:48:29.43 +19:13:44.0 11.5mag 141P/Machholz
03:52:37.57 +13:35:26.8 11.4mag 141P-A/Machholz
02:33:04.08 +09:50:35.7 10.5mag 141P-D/Machholz
02:37:46.07 -29:02:21.8 17.7mag 161P/Hartley-IRAS
02:18:01.26 +11:43:18.4 14.9mag 162P/SidingSpring
17:11:42.87 -10:44:19.5 16.1mag 235P/LINEAR
06:33:30.60 +35:52:27.2 17.2mag 240P/NEAT
07:55:07.93 -02:50:12.2 18.0mag 242P/Spahr
23:23:21.08 -12:51:26.6 17.1mag 260P/McNaught
02:56:12.48 +26:52:31.1 17.8mag 295P/LINEAR
15:29:26.46 +08:13:57.9 17.4mag 391P/Kowalski
07:47:50.49 +21:14:59.3 17.8mag 450P/LONEOS
06:16:31.15 +43:27:55.4 17.7mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K May 12 06:40 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
12:59:50.45 -10:58:38.80 2026-05-9.06 17.5
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
12:59:50.45 -10:58:38.80 2026-05-9.06 17.5
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
-rw-r--r-- 1 apache apache 5.8K May 12 06:40 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
-rw-r--r-- 1 apache apache 188K May 12 06:40 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:54:46.620 -08:22:24.75 AT 2026loc 2026-05-06.75 19.14
14:22:36.675 +74:50:21.87 AT 2026lob 2026-04-29.38 20.2009
17:03:04.538 +02:27:36.89 AT 2026loa 2026-04-28.46 20.2126
14:58:51.354 +75:57:44.68 AT 2026lnz 2026-04-29.40 19.9983
14:59:36.274 +47:45:03.39 AT 2026lny 2026-04-29.38 19.5987
11:06:29.182 +44:51:04.29 AT 2026lnx 2026-05-06.32 18.654
12:25:50.354 +05:38:12.16 AT 2026lnw 2026-05-02.22 19.7726
16:59:22.419 +01:38:47.05 AT 2026lnv 2026-05-07.34 19.2961
10:41:49.538 -18:22:59.53 AT 2026lnu 2026-05-05.37 19.94
15:55:05.718 +01:53:48.70 AT 2026lnt 2026-05-07.33 18.2083
13:29:49.691 -05:45:05.96 SN 2026lns 2026-05-07.21 19.2662
15:08:03.565 +59:43:20.93 AT 2026lnr 2026-05-07.24 19.8187
13:19:56.192 +04:42:46.60 AT 2026lnq 2026-05-07.23 19.7266
13:42:37.932 +03:25:31.87 AT 2026lnp 2026-05-07.23 19.3378
13:05:48.294 -23:51:09.88 AT 2026lno 2026-05-07.23 19.2731
13:28:10.220 -24:58:07.02 AT 2026lnn 2026-05-07.23 19.1862
13:01:10.346 -26:29:29.03 AT 2026lnm 2026-05-07.21 19.8458
13:06:44.896 +73:12:18.55 AT 2026lnl 2026-05-07.22 18.8585
16:53:20.972 +24:45:10.02 AT 2026lnk 2026-04-29.39 20.1096
15:20:12.330 +05:17:27.37 AT 2026lnj 2026-04-23.40 20.1549
-rw-r--r-- 1 apache apache 30K May 12 06:40 tns_transients_list.txt
