This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 8.81 01:56:38.04 +59:15:33.8
131.18806 -2.56327 galactic Cas Second-epoch detections are separated by 0.6" and 4.3 pix
The object was found in VSX 0" X Cas
Type: M
# Max. Min./Amp. JD0 Period
9.450 V 13.200 V 2457020.00000 415.000000000000 C5,4e(N1e)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.04 +59:15:33.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.04 +59:15:33.8: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 56 38.04 +59 15 33.8 8.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
X Cas,2461199.8312,8.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
X Cas 20260608.3312 8.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 11.28 01:11:20.10 +61:17:57.0
125.31923 -1.48032 galactic Cas Second-epoch detections are separated by 0.5" and 4.2 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 | 01:11:20.10 +61:17:57.0 (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 01:11:20.10 +61:17:57.0: 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 01:11:20.10 +61:17:57.0: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 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 06 08.3312* 01 11 20.10 +61 17 57.0 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8312,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3312 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 11.24 01:35:41.73 +61:13:12.4
128.23450 -1.19516 galactic Cas Second-epoch detections are separated by 1.3" and 4.1 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 | 01:35:41.73 +61:13:12.4 (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 01:35:41.73 +61:13:12.4: 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 01:35:41.73 +61:13:12.4: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 35 41.73 +61 13 12.4 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,2461199.8312,11.24,0.05,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 20260608.3312 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 11.29 01:38:59.06 +61:08:53.5
128.63736 -1.19575 galactic Cas Second-epoch detections are separated by 1.3" and 4.0 pix
The object was found in VSX16" Gaia DR3 509947072000083840
Type: ROT
# Max. Min./Amp. JD0 Period
14.000 G 14.010 G 0.811910000000 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 01:38:59.06 +61:08:53.5: 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 01:38:59.06 +61:08:53.5: 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 06 08.3312* 01 38 59.06 +61 08 53.5 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509947072000083840,2461199.8312,11.29,0.05,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 509947072000083840 20260608.3312 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 06 08.3312 2461199.8312 11.28 01:36:37.01 +58:44:44.1
128.77590 -3.61259 galactic Cas Second-epoch detections are separated by 2.7" and 4.4 pix
The object was found in VSX 3" Gaia DR3 509123228550621568
Type: ROT
# Max. Min./Amp. JD0 Period
14.260 G 14.310 G 2.477030000000 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 01:36:37.01 +58:44:44.1: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:37.01 +58:44:44.1: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 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 06 08.3312* 01 36 37.01 +58 44 44.1 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 509123228550621568,2461199.8312,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509123228550621568 20260608.3312 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 11.30 01:45:15.24 +61:13:52.8
129.36205 -0.96675 galactic Cas Second-epoch detections are separated by 4.2" and 3.6 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 | 01:45:15.24 +61:13:52.8 (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 01:45:15.24 +61:13:52.8: 12.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:15.24 +61:13:52.8: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 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 06 08.3312* 01 45 15.24 +61 13 52.8 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,2461199.8312,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3312 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 11.15 01:25:01.17 +62:50:50.6
126.75242 0.22501 galactic Cas Second-epoch detections are separated by 1.3" and 3.8 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 | 01:25:01.17 +62:50:50.6 (user input) | T | P | (position from user input) J-Ks=0.981+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:01.17 +62:50:50.6: 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 01:25:01.17 +62:50:50.6: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 25 01.17 +62 50 50.6 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,2461199.8312,11.15,0.05,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 20260608.3312 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 06 08.3312 2461199.8312 11.02 01:34:58.00 +61:00:13.5
128.18440 -1.42331 galactic Cas Second-epoch detections are separated by 1.4" and 3.9 pix
The object was found in VSX11" Gaia DR3 509967443017642624
Type: RS
# Max. Min./Amp. JD0 Period
17.430 G 17.560 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 01:34:58.00 +61:00:13.5: 12.37 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:58.00 +61:00:13.5: 13.70 +/- 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 06 08.3312* 01 34 58.00 +61 00 13.5 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509967443017642624,2461199.8312,11.02,0.05,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 509967443017642624 20260608.3312 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 06 08.3312 2461199.8312 11.19 01:08:25.60 +59:48:03.5
125.06974 -3.00024 galactic Cas Second-epoch detections are separated by 3.4" and 3.7 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 | DocumentRef: VOTx3884615 | 01:08:25.60 +59:48:03.5 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.377+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:25.60 +59:48:03.5: 12.55 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:25.60 +59:48:03.5: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 08 25.60 +59 48 03.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3884615,2461199.8312,11.19,0.05,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
DocumentRef: VOTx3884615 20260608.3312 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 06 08.3312 2461199.8312 11.34 01:22:50.59 +58:12:41.5
127.07077 -4.40762 galactic Cas Second-epoch detections are separated by 3.2" and 4.0 pix
The object was found in VSX21" Gaia DR3 413816392424091520
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.040 G 13.070 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:50.59 +58:12:41.5: 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 01:22:50.59 +58:12:41.5: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.22 +/- 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 06 08.3312* 01 22 50.59 +58 12 41.5 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413816392424091520,2461199.8312,11.34,0.05,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 413816392424091520 20260608.3312 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 11.10 01:07:39.80 +61:12:43.6
124.88484 -1.59810 galactic Cas Second-epoch detections are separated by 3.7" and 4.7 pix
The object was found in VSX23" ASASSN-V J010737.80+611259.9
Type: EA
# Max. Min./Amp. JD0 Period
14.292 g Y 0.528 g 2458027.93600 1.349500000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.80 +61:12:43.6: 12.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.80 +61:12:43.6: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 07 39.80 +61 12 43.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J010737.80+611259.9,2461199.8312,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J010737.80+611259.9 20260608.3312 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 11.25 01:33:19.99 +62:33:20.4
127.73796 0.07550 galactic Cas Second-epoch detections are separated by 3.6" and 3.4 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 | DocumentRef: VOTx4127324 | 01:33:19.99 +62:33:20.4 (user input) | (GCVS) | (GCVS) | (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 01:33:19.99 +62:33:20.4: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:19.99 +62:33:20.4: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 33 19.99 +62 33 20.4 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
DocumentRef: VOTx4127324,2461199.8312,11.25,0.05,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
DocumentRef: VOTx4127324 20260608.3312 11.25CV 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 06 08.3312 2461199.8312 11.18 01:46:30.88 +57:52:14.0
130.22393 -4.21931 galactic Cas Second-epoch detections are separated by 1.6" and 4.2 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 | DocumentRef: VOTx3901772 | 01:46:30.88 +57:52:14.0 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.329+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:30.88 +57:52:14.0: 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 01:46:30.88 +57:52:14.0: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 46 30.88 +57 52 14.0 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
DocumentRef: VOTx3901772,2461199.8312,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3901772 20260608.3312 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.95 01:56:13.04 +59:33:50.1
131.06072 -2.28157 galactic Cas Second-epoch detections are separated by 1.0" and 4.2 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 | DocumentRef: VOTx3898611 | 01:56:13.04 +59:33:50.1 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.814+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:13.04 +59:33:50.1: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:13.04 +59:33:50.1: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 56 13.04 +59 33 50.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3898611,2461199.8312,10.95,0.05,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
DocumentRef: VOTx3898611 20260608.3312 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 11.10 01:12:00.99 +64:42:18.7
125.12892 1.92127 galactic Cas Second-epoch detections are separated by 1.4" and 4.0 pix
The object was found in VSX 3" 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 01:12:00.99 +64:42:18.7: 11.87 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:00.99 +64:42:18.7: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 12 00.99 +64 42 18.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J011201.03+644221.2,2461199.8312,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011201.03+644221.2 20260608.3312 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.90 02:12:46.81 +61:34:17.7
132.45475 0.21296 galactic Cas Second-epoch detections are separated by 1.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:12:46.81 +61:34:17.7 (user input) | T | P | (position from user input) J-Ks=0.914+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:12:46.81 +61:34:17.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:12:46.81 +61:34:17.7: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 02 12 46.81 +61 34 17.7 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8312,10.90,0.05,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
target 20260608.3312 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 06 08.3312 2461199.8312 11.08 01:40:18.31 +61:21:06.5
128.75559 -0.96617 galactic Cas Second-epoch detections are separated by 0.9" and 4.1 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 | DocumentRef: VOTx3902510 | 01:40:18.31 +61:21:06.5 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.970+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:18.31 +61:21:06.5: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:18.31 +61:21:06.5: 13.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 40 18.31 +61 21 06.5 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
DocumentRef: VOTx3902510,2461199.8312,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3902510 20260608.3312 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.96 01:19:42.17 +60:11:03.3
126.44195 -2.49473 galactic Cas Second-epoch detections are separated by 1.8" and 3.9 pix
The object was found in VSX19" Gaia DR3 510351108161907840
Type: ROT
# Max. Min./Amp. JD0 Period
13.910 G 13.940 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 01:19:42.17 +60:11:03.3: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:42.17 +60:11:03.3: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 19 42.17 +60 11 03.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510351108161907840,2461199.8312,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510351108161907840 20260608.3312 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.88 01:43:27.46 +58:38:06.2
129.67131 -3.55435 galactic Cas Second-epoch detections are separated by 1.6" and 4.3 pix
The object was found in VSX 1" Gaia DR3 506084487648397824
Type: ROT
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:27.46 +58:38:06.2: 12.67 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:27.46 +58:38:06.2: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 43 27.46 +58 38 06.2 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
Gaia DR3 506084487648397824,2461199.8312,10.88,0.05,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
Gaia DR3 506084487648397824 20260608.3312 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 06 08.3312 2461199.8312 10.80 01:17:15.17 +58:35:35.8
126.29850 -4.10963 galactic Cas Second-epoch detections are separated by 2.6" and 4.0 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 J019.3185+58.5958 | 01:17:15.17 +58:35:35.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.437+/-0.037 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:15.17 +58:35:35.8: 12.42 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:15.17 +58:35:35.8: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 17 15.17 +58 35 35.8 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
ATO J019.3185+58.5958,2461199.8312,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J019.3185+58.5958 20260608.3312 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.87 01:11:44.74 +61:13:57.2
125.37365 -1.54288 galactic Cas Second-epoch detections are separated by 2.4" and 4.5 pix
The object was found in VSX 0" ZTF J011144.73+611356.9
Type: RS
# Max. Min./Amp. JD0 Period
13.552 r Y 0.107 r 2458423.79830 1.359407700000
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 01:11:44.74 +61:13:57.2: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:44.74 +61:13:57.2: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 11 44.74 +61 13 57.2 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
ZTF J011144.73+611356.9,2461199.8312,10.87,0.05,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 J011144.73+611356.9 20260608.3312 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 06 08.3312 2461199.8312 10.90 01:24:55.09 +59:41:48.4
127.14945 -2.90053 galactic Cas Second-epoch detections are separated by 3.0" and 3.8 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 | 01:24:55.09 +59:41:48.4 (user input) | T | P | (position from user input) J-Ks=0.217+/-0.043 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:55.09 +59:41:48.4: 12.88 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:55.09 +59:41:48.4: 13.99 +/- 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 06 08.3312* 01 24 55.09 +59 41 48.4 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
target,2461199.8312,10.90,0.05,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
target 20260608.3312 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 06 08.3312 2461199.8312 10.95 01:08:59.63 +60:47:23.6
125.07352 -2.00884 galactic Cas Second-epoch detections are separated by 3.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 522440066710315904 | 01:08:58.80 +60:47:45.5 (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 01:08:59.63 +60:47:23.6: 13.10 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:59.63 +60:47:23.6: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 08 59.63 +60 47 23.6 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 522440066710315904,2461199.8312,10.95,0.05,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
Gaia DR3 522440066710315904 20260608.3312 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.80 01:13:27.33 +59:57:17.7
125.68798 -2.79896 galactic Cas Second-epoch detections are separated by 0.6" and 4.2 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 | 01:13:27.33 +59:57:17.7 (user input) | T | P | (position from user input) J-Ks=0.257+/-0.049 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:27.33 +59:57:17.7: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:27.33 +59:57:17.7: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 13 27.33 +59 57 17.7 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,2461199.8312,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3312 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.74 01:26:38.97 +59:41:39.3
127.36653 -2.87397 galactic Cas Second-epoch detections are separated by 3.7" and 4.1 pix
The object was found in VSX 3" Gaia DR3 510083239641442688
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.660 G 13.680 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:38.97 +59:41:39.3: 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 01:26:38.97 +59:41:39.3: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 26 38.97 +59 41 39.3 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510083239641442688,2461199.8312,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510083239641442688 20260608.3312 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.74 01:29:37.00 +60:44:46.8
127.58199 -1.78025 galactic Cas Second-epoch detections are separated by 3.5" and 3.7 pix
The object was found in VSX 1" ZTF J012937.04+604447.6
Type: SR
# Max. Min./Amp. JD0 Period
13.685 r Y 0.379 r 2458434.63690 57.409238500000
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 01:29:37.00 +60:44:46.8: 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 01:29:37.00 +60:44:46.8: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 29 37.00 +60 44 46.8 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J012937.04+604447.6,2461199.8312,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J012937.04+604447.6 20260608.3312 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.57 01:22:28.42 +61:07:37.9
126.67098 -1.51904 galactic Cas Second-epoch detections are separated by 0.8" and 4.2 pix
The object was found in VSX20" Gaia DR3 510501328936368640
Type: RS
# Max. Min./Amp. JD0 Period
13.970 G 14.040 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:28.42 +61:07:37.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:28.42 +61:07:37.9: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 22 28.42 +61 07 37.9 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510501328936368640,2461199.8312,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510501328936368640 20260608.3312 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.57 01:19:08.74 +60:33:59.4
126.33194 -2.12220 galactic Cas Second-epoch detections are separated by 0.6" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510378080556092032 | 01:19:06.00 +60:34:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.265+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:08.74 +60:33:59.4: 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 01:19:08.74 +60:33:59.4: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 19 08.74 +60 33 59.4 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510378080556092032,2461199.8312,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510378080556092032 20260608.3312 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.65 01:30:34.30 +59:44:32.4
127.84948 -2.75525 galactic Cas Second-epoch detections are separated by 0.8" and 4.2 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 | ATO J022.6525+59.7408 | 01:30:34.30 +59:44:32.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.454+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:34.30 +59:44:32.4: 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 01:30:34.30 +59:44:32.4: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 30 34.30 +59 44 32.4 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
ATO J022.6525+59.7408,2461199.8312,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.6525+59.7408 20260608.3312 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.43 01:32:19.11 +59:45:27.6
128.06470 -2.70605 galactic Cas Second-epoch detections are separated by 1.3" and 4.2 pix
The object was found in VSX21" ZTF J013221.77+594532.2
Type: SR
# Max. Min./Amp. JD0 Period
12.583 r Y 0.243 r 2458304.52380 52.926856300000
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 01:32:19.11 +59:45:27.6: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:19.11 +59:45:27.6: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 32 19.11 +59 45 27.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J013221.77+594532.2,2461199.8312,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J013221.77+594532.2 20260608.3312 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.13 01:49:03.84 +61:04:19.1
129.84517 -1.02392 galactic Cas Second-epoch detections are separated by 1.5" and 4.1 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 | 01:49:03.84 +61:04:19.1 (user input) | T | P | (position from user input) J-Ks=0.226+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:03.84 +61:04:19.1: 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 01:49:03.84 +61:04:19.1: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 49 03.84 +61 04 19.1 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8312,10.13,0.05,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 20260608.3312 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.07 01:46:55.24 +59:54:51.5
129.83935 -2.21126 galactic Cas Second-epoch detections are separated by 2.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506617853860840320 | 01:46:52.59 +59:54:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1955ApJS....2..123F LF 5 +59 210 J-Ks=0.866+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:55.24 +59:54:51.5: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:55.24 +59:54:51.5: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 46 55.24 +59 54 51.5 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506617853860840320,2461199.8312,10.07,0.05,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 506617853860840320 20260608.3312 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 9.95 01:25:26.53 +60:57:44.9
127.04828 -1.63721 galactic Cas Second-epoch detections are separated by 1.1" and 4.0 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 510670688089089920 | 01:25:28.22 +60:57:27.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1960IzKry..24..160B [B60] +60 212
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:26.53 +60:57:44.9: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:26.53 +60:57:44.9: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 25 26.53 +60 57 44.9 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510670688089089920,2461199.8312,9.95,0.05,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
Gaia DR3 510670688089089920 20260608.3312 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 9.82 01:35:24.97 +60:39:16.4
128.29742 -1.75823 galactic Cas Second-epoch detections are separated by 1.5" and 3.9 pix
The object was found in VSX 6" Gaia DR3 509819081975016960
Type: S
# Max. Min./Amp. JD0 Period
17.140 G 17.450 G O
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:24.97 +60:39:16.4: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:24.97 +60:39:16.4: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 35 24.97 +60 39 16.4 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509819081975016960,2461199.8312,9.82,0.05,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 509819081975016960 20260608.3312 9.82CV 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 06 08.3312 2461199.8312 8.14 01:47:13.06 +57:44:19.2
130.34394 -4.32813 galactic Cas Second-epoch detections are separated by 0.5" and 4.3 pix
The object was found in VSX 4" Gaia DR3 505962471920178944
Type: VAR
# Max. Min./Amp. JD0 Period
13.440 G 13.470 G 0.024984900000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:13.06 +57:44:19.2: 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 01:47:13.06 +57:44:19.2: 10.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.70 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 47 13.06 +57 44 19.2 8.1 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 505962471920178944,2461199.8312,8.14,0.05,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 505962471920178944 20260608.3312 8.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.20 02:03:46.69 +57:53:08.4
132.45014 -3.64301 galactic Per Second-epoch detections are separated by 1.7" and 4.2 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 505424815032880768 | 02:03:48.26 +57:52:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1932MeUpp..55....1S [S32] 85
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:46.69 +57:53:08.4: 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 02:03:46.69 +57:53:08.4: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 02 03 46.69 +57 53 08.4 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505424815032880768,2461199.8312,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505424815032880768 20260608.3312 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.55 01:15:09.86 +60:09:05.4
125.88316 -2.58422 galactic Cas Second-epoch detections are separated by 1.0" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J018.7866+60.1445 | 01:15:09.86 +60:09:05.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: B6V 1992AJ....103.1596B Cl* NGC 433 BCN 38 J-Ks=0.312+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:09.86 +60:09:05.4: 11.00 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:09.86 +60:09:05.4: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 15 09.86 +60 09 05.4 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J018.7866+60.1445,2461199.8312,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J018.7866+60.1445 20260608.3312 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.41 01:46:13.84 +57:54:08.7
130.18018 -4.19617 galactic Cas Second-epoch detections are separated by 1.3" and 4.2 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 505968386090030336 | 01:46:16.02 +57:53:41.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.694+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:13.84 +57:54:08.7: 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 01:46:13.84 +57:54:08.7: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 46 13.84 +57 54 08.7 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505968386090030336,2461199.8312,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505968386090030336 20260608.3312 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.57 02:15:48.92 +59:33:05.6
133.44479 -1.58690 galactic Cas Second-epoch detections are separated by 0.4" and 4.4 pix
The object was found in VSX 2" Gaia DR3 507250790304191744
Type: ROT
# Max. Min./Amp. JD0 Period
13.200 G 13.220 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 02:15:48.92 +59:33:05.6: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:48.92 +59:33:05.6: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 02 15 48.92 +59 33 05.6 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 507250790304191744,2461199.8312,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507250790304191744 20260608.3312 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.71 01:36:16.27 +60:12:25.4
128.47818 -2.18102 galactic Cas Second-epoch detections are separated by 2.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 01:36:16.27 +60:12:25.4: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:16.27 +60:12:25.4: 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 06 08.3312* 01 36 16.27 +60 12 25.4 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
Gaia DR3 509768332640107392,2461199.8312,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509768332640107392 20260608.3312 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 06 08.3312 2461199.8312 10.64 01:46:38.47 +60:07:34.0
129.76007 -2.01175 galactic Cas Second-epoch detections are separated by 1.2" and 4.2 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 | 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 01:46:38.47 +60:07:34.0: 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 01:46:38.47 +60:07:34.0: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 46 38.47 +60 07 34.0 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.6591+60.1406,2461199.8312,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.6591+60.1406 20260608.3312 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.80 01:28:07.81 +58:50:39.4
127.67272 -3.68932 galactic Cas Second-epoch detections are separated by 3.9" and 4.9 pix
The object was found in VSX24" Gaia DR3 509266886619110144
Type: ROT
# Max. Min./Amp. JD0 Period
15.900 G 15.940 G 6.018600000000 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 01:28:07.81 +58:50:39.4: 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 01:28:07.81 +58:50:39.4: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 28 07.81 +58 50 39.4 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509266886619110144,2461199.8312,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509266886619110144 20260608.3312 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.80 01:46:23.18 +61:12:57.3
129.49856 -0.95331 galactic Cas Second-epoch detections are separated by 0.2" and 4.1 pix
The object was found in VSX21" Gaia DR3 511217282805374208
Type: ROT
# Max. Min./Amp. JD0 Period
18.220 G 18.350 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 01:46:23.18 +61:12:57.3: 12.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:23.18 +61:12:57.3: 13.83 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 46 23.18 +61 12 57.3 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 511217282805374208,2461199.8312,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511217282805374208 20260608.3312 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.74 01:50:26.25 +59:39:00.7
130.32952 -2.37147 galactic Cas Second-epoch detections are separated by 2.8" and 4.0 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 | DocumentRef: VOTx134384 | 01:50:26.25 +59:39:00.7 (user input) | (GCVS) | (GCVS) | (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 01:50:26.25 +59:39:00.7: 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 01:50:26.25 +59:39:00.7: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 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 06 08.3312* 01 50 26.25 +59 39 00.7 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
DocumentRef: VOTx134384,2461199.8312,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx134384 20260608.3312 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.95 01:06:55.33 +59:18:56.3
124.90992 -3.49663 galactic Cas Second-epoch detections are separated by 2.1" and 4.0 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 | 01:06:55.33 +59:18:56.3 (user input) | T | P | (position from user input) J-Ks=0.785+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.33 +59:18:56.3: 13.02 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.33 +59:18:56.3: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 06 55.33 +59 18 56.3 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
target,2461199.8312,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3312 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.88 01:32:05.77 +61:59:26.0
127.68601 -0.50532 galactic Cas Second-epoch detections are separated by 1.0" and 4.0 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 510798197068398848 | 01:32:04.51 +61:59:00.7 (Gaia DR3) | DSCT/GDOR (local) | A (local) | Gaia3var=VARIABLE SpType: F5 1960IzKry..24..160B [B60] +61 281 J-Ks=0.127+/-0.036 (A)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:05.77 +61:59:26.0: 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 01:32:05.77 +61:59:26.0: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 32 05.77 +61 59 26.0 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
Gaia DR3 510798197068398848,2461199.8312,10.88,0.05,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
Gaia DR3 510798197068398848 20260608.3312 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 06 08.3312 2461199.8312 10.96 01:38:04.35 +58:10:24.7
129.06544 -4.14178 galactic Cas Second-epoch detections are separated by 3.3" and 3.9 pix
The object was found in VSX21" Gaia DR3 508962699851411840
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
16.190 G 16.240 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:04.35 +58:10:24.7: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:04.35 +58:10:24.7: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 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 06 08.3312* 01 38 04.35 +58 10 24.7 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 508962699851411840,2461199.8312,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508962699851411840 20260608.3312 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.98 01:12:27.47 +59:58:25.4
125.56185 -2.79065 galactic Cas Second-epoch detections are separated by 2.3" and 3.9 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 | DocumentRef: VOTx114600 | 01:12:22.31 +59:58:45.1 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:27.47 +59:58:25.4: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:27.47 +59:58:25.4: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 12 27.47 +59 58 25.4 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
DocumentRef: VOTx114600,2461199.8312,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx114600 20260608.3312 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.81 01:07:24.23 +60:56:07.7
124.87080 -1.87616 galactic Cas Second-epoch detections are separated by 3.9" and 3.6 pix
The object was found in VSX 3" ZTF J010724.50+605605.2
Type: SR
# Max. Min./Amp. JD0 Period
15.599 g Y 0.213 g 2458370.54470 225.773534500000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:24.23 +60:56:07.7: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:24.23 +60:56:07.7: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 07 24.23 +60 56 07.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J010724.50+605605.2,2461199.8312,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J010724.50+605605.2 20260608.3312 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 10.91 01:54:06.37 +61:05:11.8
130.43498 -0.86891 galactic Cas Second-epoch detections are separated by 6.4" and 3.5 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 | 01:54:06.37 +61:05:11.8 (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 01:54:06.37 +61:05:11.8: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:06.37 +61:05:11.8: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 54 06.37 +61 05 11.8 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,2461199.8312,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3312 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 06 08.3312 2461199.8312 11.01 02:02:23.60 +59:42:14.9
131.77845 -1.94333 galactic Cas Second-epoch detections are separated by 4.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J030.6164+59.6920 | 02:02:24.46 +59:41:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:23.60 +59:42:14.9: 13.17 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:23.60 +59:42:14.9: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 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 06 08.3312* 02 02 23.60 +59 42 14.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J030.6164+59.6920,2461199.8312,11.01,0.05,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
ATO J030.6164+59.6920 20260608.3312 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 06 08.3312 2461199.8312 11.20 01:33:24.96 +59:30:24.8
128.24201 -2.93137 galactic Cas Second-epoch detections are separated by 4.2" and 3.6 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 | 01:33:24.96 +59:30:24.8 (user input) | T | P | (position from user input) J-Ks=0.520+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:24.96 +59:30:24.8: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:24.96 +59:30:24.8: 13.89 +/- 0.05 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 06 08.3312* 01 33 24.96 +59 30 24.8 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,2461199.8312,11.20,0.05,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 20260608.3312 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 06 08.3312 2461199.8312 11.06 01:28:07.19 +59:53:49.4
127.52161 -2.64740 galactic Cas Second-epoch detections are separated by 3.4" and 4.3 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 510182298766565376 | 01:28:11.24 +59:54:05.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.571+/-0.041 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:07.19 +59:53:49.4: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:07.19 +59:53:49.4: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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 06 08.3312* 01 28 07.19 +59 53 49.4 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 510182298766565376,2461199.8312,11.06,0.05,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
Gaia DR3 510182298766565376 20260608.3312 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 06 08.3312 2461199.8312 11.15 01:21:45.69 +58:34:13.7
126.88654 -4.06825 galactic Cas Second-epoch detections are separated by 0.8" and 4.4 pix
The object was found in VSX23" 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 01:21:45.69 +58:34:13.7: 12.59 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:45.69 +58:34:13.7: 13.99 +/- 0.05 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 06 08.3312* 01 21 45.69 +58 34 13.7 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
ZTF J012144.11+583432.6,2461199.8312,11.15,0.05,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
ZTF J012144.11+583432.6 20260608.3312 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 06 08.3312 2461199.8312 11.07 01:22:24.10 +61:13:51.9
126.64988 -1.41694 galactic Cas Second-epoch detections are separated by 2.1" and 4.3 pix
The object was found in VSX 2" NSVS J0122238+611352
Type: M
# Max. Min./Amp. JD0 Period
14.871 r Y 3.740 r 2458328.87710 325.120339600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:24.10 +61:13:51.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:24.10 +61:13:51.9: 15.83 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.83 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 22 24.10 +61 13 51.9 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0122238+611352,2461199.8312,11.07,0.05,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 J0122238+611352 20260608.3312 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 11.16 01:09:22.99 +57:26:30.2
125.35505 -5.34557 galactic Cas Second-epoch detections are separated by 1.4" and 4.2 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 | 01:09:22.99 +57:26:30.2 (user input) | T | P | (position from user input) 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 01:09:22.99 +57:26:30.2: 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 01:09:22.99 +57:26:30.2: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 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 06 08.3312* 01 09 22.99 +57 26 30.2 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,2461199.8312,11.16,0.05,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 20260608.3312 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 11.07 02:11:12.52 +62:21:13.4
132.03926 0.90088 galactic Cas Second-epoch detections are separated by 3.8" and 3.9 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 | 02:11:12.52 +62:21:13.4 (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 02:11:12.52 +62:21:13.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:12.52 +62:21:13.4: 14.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 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 06 08.3312* 02 11 12.52 +62 21 13.4 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,2461199.8312,11.07,0.05,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 20260608.3312 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 11.32 01:35:35.59 +61:15:46.6
128.21506 -1.15506 galactic Cas Second-epoch detections are separated by 1.8" and 4.4 pix
The object was found in VSX 1" Gaia DR3 509978133204810624
Type: RS
# Max. Min./Amp. JD0 Period
14.210 G 14.320 G 2.136390000000 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 01:35:35.59 +61:15:46.6: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:35.59 +61:15:46.6: 14.26 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 35 35.59 +61 15 46.6 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 509978133204810624,2461199.8312,11.32,0.05,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
Gaia DR3 509978133204810624 20260608.3312 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3312 2461199.8312 11.44 01:43:51.64 +61:52:51.2
129.06683 -0.36483 galactic Cas Second-epoch detections are separated by 8.6" and 2.7 pix
The object was found in VSX10" Gaia DR3 511486250835935744
Type: RS
# Max. Min./Amp. JD0 Period
18.000 G 18.150 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 01:43:51.64 +61:52:51.2: 11.55 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:51.64 +61:52:51.2: 14.54 +/- 0.26 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3312* 01 43 51.64 +61 52 51.2 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
Gaia DR3 511486250835935744,2461199.8312,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511486250835935744 20260608.3312 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461199.83144934 08.06.2026 07:57:07.223 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 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): 24936
Objects passed selection criteria: 24774
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 16946.8
Average stars matched: 15673 (92.4838 %)
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 Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 03:16:38 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: 2461199.83144934 08.06.2026 07:57:07.223 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 246
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: 78 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): 184791
Objects passed selection criteria: 184290
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: 133875
Average stars matched: 123145 (91.9851 %)
Memory usage VmPeak: 2131264 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 03:22:53 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.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: 2461199.83097074
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'
Plate-solving the images
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits'
wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
Image size: 938.8'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: 01:42:49.867 +62:00:14.27 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 01:42:49.867 +62:00:14.27
Angular distance between the image centers 0.0455 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
Image size: 938.8'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: 01:42:53.155 +62:00:18.53 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 01:42:53.155 +62:00:18.53
Angular distance between the image centers 0.0518 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:42:49.867 +62:00:14.27
Second-epoch second image center 01:42:53.155 +62:00:18.53
Angular distance between the image centers 0.00654 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.cwkXtiauX8
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.oVjlpzbpvm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits &> /tmp/tmp.CwmXt8gSzG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits &> /tmp/tmp.UpG5y253jl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.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
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.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 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.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
14.1 mag. fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
14.1 mag. fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.3 (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.cwkXtiauX8 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/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.oVjlpzbpvm (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/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.CwmXt8gSzG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=950, passed=13137
Got 13137 stars (including 12176 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat
util/solve_plate_with_UCAC5 got 13137 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (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 55.8 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(), 941 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(), 12891 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 55.8 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(), 12891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 12891 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_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits N_match=972 sigma_overall_arcsec=0.638 sigma_q1_arcsec=0.525 sigma_q2_arcsec=0.619 sigma_q3_arcsec=0.703 sigma_q4_arcsec=0.710 n_q1=282 n_q2=314 n_q3=219 n_q4=157 worst_quadrant_to_overall_ratio=1.113
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.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.UpG5y253jl (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat
SExtractor catalog parsing summary: zero_flux=6, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=966, passed=13091
Got 13091 stars (including 12116 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat
util/solve_plate_with_UCAC5 got 13091 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (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 55.8 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: 972 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 12608 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 55.8 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: 971 matched stars entering correct_measured_positions(), 12609 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 12609 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 971 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits N_match=971 sigma_overall_arcsec=0.604 sigma_q1_arcsec=0.533 sigma_q2_arcsec=0.533 sigma_q3_arcsec=0.743 sigma_q4_arcsec=0.554 n_q1=286 n_q2=319 n_q3=221 n_q4=145 worst_quadrant_to_overall_ratio=1.229
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=7.729 worst_q_ratio=4.055
ref2=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=0.405 worst_q_ratio=1.316
new1=fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits sigma_overall=0.638 worst_q_ratio=1.113
new2=fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits sigma_overall=0.604 worst_q_ratio=1.229
reference average sigma_overall=4.067 worst_q_ratio=2.6855
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290_astrometric_residuals.png (see messages above)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:24.43 +60:39:45.8: 12.87 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.04 +59:15:33.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:24.43 +60:39:45.8: 11.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.19 +/- 0.01
Forced photometry filter REJECTED candidate at 01:33:24.43 +60:39:45.8: ref_mag=11.19 +/- 0.01 new_mean_mag=10.9613 delta=0.23 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.04 +59:15:33.8: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter KEPT candidate at 01:56:38.04 +59:15:33.8: ref_mag=9.75 +/- 0.00 new_mean_mag=8.8134 delta=0.94 (need > 0.90)
Adding exclusion_list_local.txt__out20109.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52793_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 52793_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:19:46.42 +58:12:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53210_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 53210_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20109_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 20109_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 08339_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:20:32.57 +62:32:01.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:56:38.04 +59:15:33.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
Image size: 938.8'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: 01:42:49.867 +62:00:14.27 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 01:42:49.867 +62:00:14.27
Angular distance between the image centers 0.0455 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
Image size: 938.8'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: 01:42:53.155 +62:00:18.53 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 01:42:53.155 +62:00:18.53
Angular distance between the image centers 0.0518 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:42:49.867 +62:00:14.27
Second-epoch second image center 01:42:53.155 +62:00:18.53
Angular distance between the image centers 0.00654 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.hyD962HiVQ
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.2QiMdO1olQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits &> /tmp/tmp.cWefeYcFaV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits &> /tmp/tmp.lvfC5HcCh0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.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
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.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 216 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
2.2 pix fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
2.2 pix fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.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
11.6 mag. fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
11.6 mag. fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
All-image limiting magnitude estimate: 11.6 (SNR ) 11.1 (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.hyD962HiVQ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/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.2QiMdO1olQ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/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.cWefeYcFaV (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=8885, passed=103112
Got 103112 stars (including 94118 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat
util/solve_plate_with_UCAC5 got 103112 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (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: 971 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 101946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 101945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 101944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 970 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits N_match=970 sigma_overall_arcsec=0.612 sigma_q1_arcsec=0.549 sigma_q2_arcsec=0.584 sigma_q3_arcsec=0.701 sigma_q4_arcsec=0.600 n_q1=273 n_q2=321 n_q3=204 n_q4=172 worst_quadrant_to_overall_ratio=1.145
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.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.lvfC5HcCh0 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=24, blended=8937, passed=103556
Got 103556 stars (including 94504 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat
util/solve_plate_with_UCAC5 got 103556 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (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 55.8 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: 971 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 101028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 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: 971 matched stars entering correct_measured_positions(), 101026 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 101026 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits N_match=971 sigma_overall_arcsec=0.629 sigma_q1_arcsec=0.578 sigma_q2_arcsec=0.541 sigma_q3_arcsec=0.680 sigma_q4_arcsec=0.632 n_q1=271 n_q2=328 n_q3=217 n_q4=155 worst_quadrant_to_overall_ratio=1.082
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-56-25_20.00sec_5.00C_LIGHT_0289.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q2b1x1_031129_TTUQ2b1x1_2001928_Do15stRm/wcs_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290.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 01:35:41.73 +61:13:12.4: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:37.01 +58:44:44.1: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:01.17 +62:50:50.6: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:20.10 +61:17:57.0: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:15.24 +61:13:52.8: 12.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:25.60 +59:48:03.5: 12.55 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:50.59 +58:12:41.5: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.80 +61:12:43.6: 12.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:59.06 +61:08:53.5: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:58.00 +61:00:13.5: 12.37 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:41.73 +61:13:12.4: 13.64 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:01.17 +62:50:50.6: 13.74 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.80 +61:12:43.6: 13.79 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:15.24 +61:13:52.8: 14.18 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:50.59 +58:12:41.5: 14.22 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:20.10 +61:17:57.0: 13.97 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:37.01 +58:44:44.1: 14.07 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:25.60 +59:48:03.5: 13.80 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:59.06 +61:08:53.5: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Forced photometry reference-image weighted average: 13.97 +/- 0.06
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry reference-image weighted average: 14.22 +/- 0.07
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Forced photometry reference-image weighted average: 14.07 +/- 0.06
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:58.00 +61:00:13.5: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry filter KEPT candidate at 01:35:41.73 +61:13:12.4: ref_mag=13.64 +/- 0.04 new_mean_mag=11.1921 delta=2.44 (need > 0.90)
Forced photometry filter KEPT candidate at 01:11:20.10 +61:17:57.0: ref_mag=13.97 +/- 0.06 new_mean_mag=11.2015 delta=2.77 (need > 0.90)
Forced photometry filter KEPT candidate at 01:07:39.80 +61:12:43.6: ref_mag=13.79 +/- 0.05 new_mean_mag=11.0547 delta=2.74 (need > 0.90)
Forced photometry filter KEPT candidate at 01:25:01.17 +62:50:50.6: ref_mag=13.74 +/- 0.04 new_mean_mag=11.1034 delta=2.64 (need > 0.90)
Forced photometry filter KEPT candidate at 01:22:50.59 +58:12:41.5: ref_mag=14.22 +/- 0.07 new_mean_mag=11.3232 delta=2.90 (need > 0.90)
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Forced photometry filter KEPT candidate at 01:45:15.24 +61:13:52.8: ref_mag=14.18 +/- 0.06 new_mean_mag=11.2988 delta=2.88 (need > 0.90)
Forced photometry filter KEPT candidate at 01:36:37.01 +58:44:44.1: ref_mag=14.07 +/- 0.06 new_mean_mag=11.2817 delta=2.78 (need > 0.90)
Forced photometry filter KEPT candidate at 01:08:25.60 +59:48:03.5: ref_mag=13.73 +/- 0.04 new_mean_mag=11.1830 delta=2.54 (need > 0.90)
Forced photometry filter KEPT candidate at 01:38:59.06 +61:08:53.5: ref_mag=13.99 +/- 0.06 new_mean_mag=11.2856 delta=2.70 (need > 0.90)
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Forced photometry filter KEPT candidate at 01:34:58.00 +61:00:13.5: ref_mag=13.59 +/- 0.04 new_mean_mag=10.9352 delta=2.66 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:19.99 +62:33:20.4: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:30.88 +57:52:14.0: 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 01:33:19.99 +62:33:20.4: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter KEPT candidate at 01:33:19.99 +62:33:20.4: ref_mag=13.79 +/- 0.04 new_mean_mag=11.2448 delta=2.55 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:30.88 +57:52:14.0: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Forced photometry filter KEPT candidate at 01:46:30.88 +57:52:14.0: ref_mag=13.72 +/- 0.04 new_mean_mag=11.1756 delta=2.54 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:13.04 +59:33:50.1: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:13.04 +59:33:50.1: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter KEPT candidate at 01:56:13.04 +59:33:50.1: ref_mag=13.65 +/- 0.04 new_mean_mag=10.9497 delta=2.70 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:00.99 +64:42:18.7: 11.87 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:12:46.81 +61:34:17.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:00.99 +64:42:18.7: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.04
Forced photometry filter KEPT candidate at 01:12:00.99 +64:42:18.7: ref_mag=13.43 +/- 0.04 new_mean_mag=11.0958 delta=2.34 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:12:46.81 +61:34:17.7: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter KEPT candidate at 02:12:46.81 +61:34:17.7: ref_mag=13.65 +/- 0.04 new_mean_mag=10.9007 delta=2.75 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:18.31 +61:21:06.5: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:18.31 +61:21:06.5: 13.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Forced photometry filter KEPT candidate at 01:40:18.31 +61:21:06.5: ref_mag=13.90 +/- 0.04 new_mean_mag=11.0683 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 01:19:42.17 +60:11:03.3: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:42.17 +60:11:03.3: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Forced photometry filter KEPT candidate at 01:19:42.17 +60:11:03.3: ref_mag=13.82 +/- 0.04 new_mean_mag=10.9560 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 01:05:06.51 +62:48:52.4: 10.41 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:06.51 +62:48:52.4: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.54 +/- 0.02
Forced photometry filter REJECTED candidate at 01:05:06.51 +62:48:52.4: ref_mag=11.54 +/- 0.02 new_mean_mag=11.0872 delta=0.45 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:27.46 +58:38:06.2: 12.67 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:27.46 +58:38:06.2: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Forced photometry filter KEPT candidate at 01:43:27.46 +58:38:06.2: ref_mag=13.68 +/- 0.04 new_mean_mag=10.8830 delta=2.80 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:15.17 +58:35:35.8: 12.42 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:15.17 +58:35:35.8: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter KEPT candidate at 01:17:15.17 +58:35:35.8: ref_mag=13.40 +/- 0.03 new_mean_mag=10.7903 delta=2.61 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:44.74 +61:13:57.2: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:44.74 +61:13:57.2: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter KEPT candidate at 01:11:44.74 +61:13:57.2: ref_mag=13.36 +/- 0.03 new_mean_mag=10.8670 delta=2.49 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:55.09 +59:41:48.4: 12.88 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:55.09 +59:41:48.4: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.06
Forced photometry filter KEPT candidate at 01:24:55.09 +59:41:48.4: ref_mag=13.94 +/- 0.06 new_mean_mag=10.8866 delta=3.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:59.63 +60:47:23.6: 13.10 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:59.63 +60:47:23.6: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Forced photometry filter KEPT candidate at 01:08:59.63 +60:47:23.6: ref_mag=13.57 +/- 0.04 new_mean_mag=10.8990 delta=2.67 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:27.33 +59:57:17.7: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:27.33 +59:57:17.7: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Forced photometry filter KEPT candidate at 01:13:27.33 +59:57:17.7: ref_mag=13.57 +/- 0.04 new_mean_mag=10.7686 delta=2.80 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:38.97 +59:41:39.3: 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 01:26:38.97 +59:41:39.3: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Forced photometry filter KEPT candidate at 01:26:38.97 +59:41:39.3: ref_mag=13.48 +/- 0.04 new_mean_mag=10.7391 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:37.00 +60:44:46.8: 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 01:29:37.00 +60:44:46.8: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Forced photometry filter KEPT candidate at 01:29:37.00 +60:44:46.8: ref_mag=13.80 +/- 0.05 new_mean_mag=10.7138 delta=3.09 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:28.42 +61:07:37.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:28.42 +61:07:37.9: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 01:22:28.42 +61:07:37.9: ref_mag=13.23 +/- 0.02 new_mean_mag=10.5723 delta=2.65 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:08.74 +60:33:59.4: 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 01:30:34.30 +59:44:32.4: 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 01:19:08.74 +60:33:59.4: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Forced photometry filter KEPT candidate at 01:19:08.74 +60:33:59.4: ref_mag=13.17 +/- 0.03 new_mean_mag=10.5716 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 01:30:34.30 +59:44:32.4: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Forced photometry filter KEPT candidate at 01:30:34.30 +59:44:32.4: ref_mag=13.39 +/- 0.04 new_mean_mag=10.6258 delta=2.76 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:10.45 +60:37:30.1: 7.60 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:10.45 +60:37:30.1: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 7.89 +/- 0.01
Forced photometry filter REJECTED candidate at 01:33:10.45 +60:37:30.1: ref_mag=7.89 +/- 0.01 new_mean_mag=10.5809 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 01:09:29.78 +61:47:03.4: 10.05 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:29.78 +61:47:03.4: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.02
Forced photometry filter REJECTED candidate at 01:09:29.78 +61:47:03.4: ref_mag=11.12 +/- 0.02 new_mean_mag=10.5402 delta=0.58 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:19.11 +59:45:27.6: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:19.11 +59:45:27.6: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 01:32:19.11 +59:45:27.6: ref_mag=13.06 +/- 0.02 new_mean_mag=10.4192 delta=2.65 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:03.84 +61:04:19.1: 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 01:49:03.84 +61:04:19.1: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Forced photometry filter KEPT candidate at 01:49:03.84 +61:04:19.1: ref_mag=12.75 +/- 0.02 new_mean_mag=10.1219 delta=2.63 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:55.24 +59:54:51.5: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:55.24 +59:54:51.5: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 01:46:55.24 +59:54:51.5: ref_mag=12.68 +/- 0.01 new_mean_mag=10.0524 delta=2.63 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:26.53 +60:57:44.9: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:26.53 +60:57:44.9: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 01:25:26.53 +60:57:44.9: ref_mag=12.67 +/- 0.01 new_mean_mag=9.9494 delta=2.73 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:24.97 +60:39:16.4: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:24.97 +60:39:16.4: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Forced photometry filter KEPT candidate at 01:35:24.97 +60:39:16.4: ref_mag=12.70 +/- 0.02 new_mean_mag=9.8150 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 01:47:13.06 +57:44:19.2: 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 01:47:13.06 +57:44:19.2: 10.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.70 +/- 0.00
Forced photometry filter KEPT candidate at 01:47:13.06 +57:44:19.2: ref_mag=10.70 +/- 0.00 new_mean_mag=8.1412 delta=2.56 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:46.69 +57:53:08.4: 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 02:03:46.69 +57:53:08.4: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Forced photometry filter KEPT candidate at 02:03:46.69 +57:53:08.4: ref_mag=13.10 +/- 0.03 new_mean_mag=10.1947 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 01:15:09.86 +60:09:05.4: 11.00 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:09.86 +60:09:05.4: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.04
Forced photometry filter KEPT candidate at 01:15:09.86 +60:09:05.4: ref_mag=12.35 +/- 0.04 new_mean_mag=10.5473 delta=1.80 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:13.84 +57:54:08.7: 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 01:46:13.84 +57:54:08.7: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Forced photometry filter KEPT candidate at 01:46:13.84 +57:54:08.7: ref_mag=13.19 +/- 0.03 new_mean_mag=10.4123 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 02:15:48.92 +59:33:05.6: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:48.92 +59:33:05.6: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Forced photometry filter KEPT candidate at 02:15:48.92 +59:33:05.6: ref_mag=13.22 +/- 0.03 new_mean_mag=10.5569 delta=2.66 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:16.27 +60:12:25.4: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:16.27 +60:12:25.4: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.04
Forced photometry filter KEPT candidate at 01:36:16.27 +60:12:25.4: ref_mag=13.54 +/- 0.04 new_mean_mag=10.7000 delta=2.84 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.47 +60:07:34.0: 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 01:46:38.47 +60:07:34.0: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.04
Forced photometry filter KEPT candidate at 01:46:38.47 +60:07:34.0: ref_mag=13.38 +/- 0.04 new_mean_mag=10.6393 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:07.81 +58:50:39.4: 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 01:28:07.81 +58:50:39.4: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter KEPT candidate at 01:28:07.81 +58:50:39.4: ref_mag=13.65 +/- 0.04 new_mean_mag=10.7897 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 01:46:23.18 +61:12:57.3: 12.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:23.18 +61:12:57.3: 13.83 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.19
Forced photometry filter KEPT candidate at 01:46:23.18 +61:12:57.3: ref_mag=13.83 +/- 0.19 new_mean_mag=10.7944 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 01:50:26.25 +59:39:00.7: 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 01:50:26.25 +59:39:00.7: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.05
Forced photometry filter KEPT candidate at 01:50:26.25 +59:39:00.7: ref_mag=13.68 +/- 0.05 new_mean_mag=10.7425 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 01:06:55.33 +59:18:56.3: 13.02 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.33 +59:18:56.3: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry filter KEPT candidate at 01:06:55.33 +59:18:56.3: ref_mag=13.82 +/- 0.05 new_mean_mag=10.9302 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 01:32:05.77 +61:59:26.0: 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 01:32:05.77 +61:59:26.0: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Forced photometry filter KEPT candidate at 01:32:05.77 +61:59:26.0: ref_mag=13.46 +/- 0.03 new_mean_mag=10.8752 delta=2.58 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:04.35 +58:10:24.7: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:04.35 +58:10:24.7: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.06
Forced photometry filter KEPT candidate at 01:38:04.35 +58:10:24.7: ref_mag=13.82 +/- 0.06 new_mean_mag=10.9326 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 01:12:27.47 +59:58:25.4: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:27.47 +59:58:25.4: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.06
Forced photometry filter KEPT candidate at 01:12:27.47 +59:58:25.4: ref_mag=13.84 +/- 0.06 new_mean_mag=10.9712 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 01:07:24.23 +60:56:07.7: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:24.23 +60:56:07.7: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Forced photometry filter KEPT candidate at 01:07:24.23 +60:56:07.7: ref_mag=13.68 +/- 0.04 new_mean_mag=10.8001 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 01:54:06.37 +61:05:11.8: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:06.37 +61:05:11.8: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Forced photometry filter KEPT candidate at 01:54:06.37 +61:05:11.8: ref_mag=13.86 +/- 0.05 new_mean_mag=10.9118 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 02:02:23.60 +59:42:14.9: 13.17 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:23.60 +59:42:14.9: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.05
Forced photometry filter KEPT candidate at 02:02:23.60 +59:42:14.9: ref_mag=13.63 +/- 0.05 new_mean_mag=11.0002 delta=2.63 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:24.96 +59:30:24.8: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:24.96 +59:30:24.8: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Forced photometry filter KEPT candidate at 01:33:24.96 +59:30:24.8: ref_mag=13.89 +/- 0.05 new_mean_mag=11.1201 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 01:28:07.19 +59:53:49.4: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:07.19 +59:53:49.4: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Forced photometry filter KEPT candidate at 01:28:07.19 +59:53:49.4: ref_mag=13.94 +/- 0.05 new_mean_mag=11.0656 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 01:21:45.69 +58:34:13.7: 12.59 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:45.69 +58:34:13.7: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Forced photometry filter KEPT candidate at 01:21:45.69 +58:34:13.7: ref_mag=13.89 +/- 0.05 new_mean_mag=11.1424 delta=2.75 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:24.10 +61:13:51.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:24.10 +61:13:51.9: 15.83 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.83 +/- 0.26
Forced photometry filter KEPT candidate at 01:22:24.10 +61:13:51.9: ref_mag=15.83 +/- 0.26 new_mean_mag=11.0633 delta=4.76 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:22.99 +57:26:30.2: 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 01:09:22.99 +57:26:30.2: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.06
Forced photometry filter KEPT candidate at 01:09:22.99 +57:26:30.2: ref_mag=13.97 +/- 0.06 new_mean_mag=11.1602 delta=2.80 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:12.52 +62:21:13.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:12.52 +62:21:13.4: 14.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.07
Forced photometry filter KEPT candidate at 02:11:12.52 +62:21:13.4: ref_mag=14.10 +/- 0.07 new_mean_mag=11.0221 delta=3.07 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:35.59 +61:15:46.6: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:35.59 +61:15:46.6: 14.26 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.10
Forced photometry filter KEPT candidate at 01:35:35.59 +61:15:46.6: ref_mag=14.26 +/- 0.10 new_mean_mag=11.3242 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 01:43:51.64 +61:52:51.2: 11.55 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:51.64 +61:52:51.2: 14.54 +/- 0.26 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.16
Forced photometry filter KEPT candidate at 01:43:51.64 +61:52:51.2: ref_mag=12.61 +/- 0.16 new_mean_mag=11.4387 delta=1.18 (need > 0.90)
Adding exclusion_list_local.txt__out247635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out261199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out261415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out261931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271959.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 757s
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: 61s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247635_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247635_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247636_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247636_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247645_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247645_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247646_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247646_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247647_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247647_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247648_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247648_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247654_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247654_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247656_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247656_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247658_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247658_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247662_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247662_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247663_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247663_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247665_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247665_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247678_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247678_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:30:06.70 +61:51:06.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247679_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247679_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:12:30.94 +61:17:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247682_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247682_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247687_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247687_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247691_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247691_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247692_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247692_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247695_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247695_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247696_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247696_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247703_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247703_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247707_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247707_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:13:41.16 +60:51:26.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247714_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247714_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247716_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247716_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:07:35.07 +57:33:09.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247721_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247721_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:16:59.23 +59:52:02.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247724_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247724_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:14:01.42 +57:40:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247725_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247725_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247728_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247728_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247731_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247731_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247737_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247737_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:33:35.46 +59:56:23.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247738_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247738_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:39:24.27 +58:23:04.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247743_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247743_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247744_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247744_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247746_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247746_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247747_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247747_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247751_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247751_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247753_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247753_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247754_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247754_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247756_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247756_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247759_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247759_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:19:24.03 +58:26:40.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247761_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247761_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:32:22.04 +60:27:29.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247763_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247763_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:01:30.75 +65:05:38.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247767_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247767_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:05:57.28 +63:03:35.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247768_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247768_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247773_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247773_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:39:04.33 +61:53:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247775_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247775_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:14:45.23 +60:30:04.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247776_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247776_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:10:37.58 +57:22:41.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247777_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247777_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247783_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247783_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:12:40.97 +61:20:38.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247784_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247784_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247786_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247786_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247787_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247787_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:07:08.05 +57:44:35.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247789_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247789_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:55:14.60 +59:32:02.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247790_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247790_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247792_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247792_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:43:59.23 +61:55:18.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247793_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247793_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:16:20.72 +62:42:27.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247794_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247794_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:15:55.96 +58:23:30.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247795_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247795_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:20:24.32 +59:10:24.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247799_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247799_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:51:35.87 +57:52:55.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247800_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247800_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:23:56.38 +62:06:40.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247801_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247801_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:25:56.63 +59:35:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247804_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247804_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:22:08.42 +60:22:44.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247806_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 247806_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:13:07.27 +58:04:48.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247807_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 247807_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249445_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 249445_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251477_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 251477_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:28:00.51 +61:19:58.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251784_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 251784_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:44:01.86 +61:53:56.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251817_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 251817_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:46:08.74 +61:12:17.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252034_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 252034_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:26:41.04 +60:46:45.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252265_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 252265_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:38:00.50 +57:56:45.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253002_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 253002_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:19:11.11 +58:20:30.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253157_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 253157_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:17:59.17 +57:47:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254049_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 254049_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:26:46.72 +57:46:54.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254283_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 254283_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:28:15.48 +58:44:12.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255222_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 255222_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:58:16.30 +59:38:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255400_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 255400_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:08:42.38 +58:17:00.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255752_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 255752_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256525_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 256525_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:20:11.04 +58:12:08.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256542_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 256542_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:18:14.15 +61:44:37.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256567_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 256567_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:43:53.10 +61:53:16.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256617_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 256617_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:05:03.60 +64:21:51.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256693_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 256693_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257050_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 257050_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:51:02.59 +64:49:53.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257054_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 257054_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:46:33.62 +61:16:47.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257488_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 257488_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:16:08.64 +58:49:39.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257766_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 257766_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:06:39.05 +64:09:28.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257880_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 257880_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:20:18.48 +58:13:42.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257967_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 257967_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:00:51.90 +58:31:25.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258071_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 258071_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:44:17.71 +61:53:14.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258218_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 258218_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:44:32.33 +58:45:35.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258444_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 258444_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:33:59.45 +58:28:32.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258463_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 258463_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:43:03.41 +58:08:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258555_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 258555_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:15:58.91 +63:12:25.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258738_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 258738_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258980_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 258980_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:11:23.04 +61:21:06.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259616_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 259616_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:19:22.34 +58:19:18.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259702_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 259702_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:02:54.89 +64:24:59.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259891_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 259891_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:18:39.91 +58:25:50.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260009_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 260009_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:33:32.63 +60:40:04.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260253_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 260253_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:33:23.37 +57:44:24.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260309_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 260309_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:39:57.07 +60:52:22.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260344_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 260344_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:19:12.54 +65:35:58.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260422_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 260422_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:16:36.27 +64:57:47.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260467_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 260467_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:35:50.54 +61:27:34.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260579_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 260579_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:16:05.19 +58:49:40.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260738_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 260738_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:44:02.07 +61:52:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260837_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 260837_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:03:15.33 +62:12:12.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260866_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 260866_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:00:36.71 +58:30:22.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260957_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 260957_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:10:23.85 +60:01:13.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261021_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261021_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:07:34.16 +60:52:43.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261072_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261072_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:27:02.37 +58:03:16.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261158_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261158_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:13:30.35 +58:34:25.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261199_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 261199_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261206_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261206_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:01:36.93 +59:57:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261280_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261280_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:13:36.03 +57:52:29.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261373_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261373_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:48:38.34 +61:49:10.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261415_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 261415_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261476_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261476_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:37:44.71 +64:45:49.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261589_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261589_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:34:10.38 +62:09:38.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261593_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261593_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:39:00.26 +61:11:55.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261674_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261674_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:15:11.61 +60:07:04.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261751_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261751_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:04:26.91 +65:05:54.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261782_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261782_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:44:28.21 +60:41:23.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261828_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261828_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:24:58.21 +59:22:57.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261931_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 261931_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261976_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 261976_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:43:07.01 +58:57:28.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262010_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 262010_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:39:24.79 +63:23:53.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262107_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 262107_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:08:32.93 +63:34:29.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262258_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 262258_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:42:33.24 +63:52:58.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262564_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 262564_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:47:19.00 +63:38:12.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262594_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 262594_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:06:45.53 +59:50:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262631_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 262631_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:17:00.90 +61:40:43.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263112_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 263112_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:16:12.79 +62:42:26.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263195_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 263195_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:19:03.82 +63:57:44.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263228_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 263228_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263243_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 263243_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:06:23.34 +62:44:02.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263292_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 263292_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:02:54.09 +60:15:40.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263332_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 263332_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:17:21.68 +59:22:33.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263386_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 263386_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263392_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 263392_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:09:09.44 +61:37:27.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263432_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 263432_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:01:15.16 +59:23:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263455_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 263455_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:41:50.95 +61:02:07.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263515_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 263515_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263605_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 263605_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:01:38.77 +61:45:16.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263696_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 263696_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:48:39.95 +59:09:19.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263978_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 263978_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264143_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 264143_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:16:02.30 +58:49:58.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264360_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 264360_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264454_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 264454_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264624_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 264624_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:58:04.40 +57:58:51.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264647_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 264647_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:38:12.13 +61:01:25.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264710_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 264710_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:21:29.10 +63:55:32.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264729_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 264729_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:19:41.53 +62:51:06.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264740_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 264740_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:37:41.62 +58:37:32.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264749_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 264749_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:42:28.20 +58:17:48.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264766_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 264766_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:14:29.89 +63:16:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264852_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 264852_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:49:34.28 +61:03:37.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265056_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265056_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:44:32.39 +61:36:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265067_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265067_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:38:07.71 +61:01:37.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265103_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265103_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:38:34.06 +58:07:23.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265145_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265145_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:38:33.82 +60:47:23.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265184_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 265184_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265242_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 265242_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265258_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265258_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:44:56.76 +59:46:23.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265302_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265302_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:58:40.04 +59:15:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265507_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265507_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:11:50.25 +59:02:57.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265550_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265550_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:38:06.41 +58:10:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265626_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265626_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:14:00.45 +61:42:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265677_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265677_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:46:18.22 +60:59:20.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265726_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265726_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:14:58.53 +60:30:22.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265760_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265760_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:31:32.42 +61:02:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265849_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265849_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:20:40.78 +60:23:48.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265890_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265890_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:42:54.69 +64:01:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265975_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 265975_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:58:05.11 +59:36:38.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265984_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 265984_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266026_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 266026_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266051_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 266051_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:14:21.87 +59:59:51.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266065_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 266065_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266430_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 266430_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:43:03.45 +58:57:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266617_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 266617_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:43:12.85 +64:00:48.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266650_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 266650_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:31:48.31 +64:22:24.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266857_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 266857_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:14:00.59 +59:02:36.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266948_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 266948_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:54:30.36 +59:06:33.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267244_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 267244_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267364_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 267364_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267515_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 267515_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:56:25.40 +62:05:29.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267635_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 267635_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:59:06.04 +59:55:35.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267852_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 267852_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267979_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 267979_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:42:26.69 +59:34:01.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268116_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 268116_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:34:42.69 +58:42:14.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268247_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 268247_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268378_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 268378_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:16:36.51 +64:56:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268439_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 268439_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:03:25.23 +57:50:12.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268514_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 268514_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:33:46.84 +62:31:24.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268662_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 268662_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269221_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 269221_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:49:06.31 +65:23:44.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269275_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 269275_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269366_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 269366_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:44:34.92 +62:36:57.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269492_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 269492_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269676_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 269676_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:27:56.45 +62:46:06.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269802_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 269802_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:48:35.05 +58:41:29.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269864_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 269864_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270425_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 270425_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:46:23.88 +59:12:44.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271094_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 271094_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271184_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 271184_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271959_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
Preparing report for the candidate 271959_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272404_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 272404_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:53:03.10 +60:26:38.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 39378_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:47:55.74 +64:32:54.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156692_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 156692_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:56:38.05 +59:15:33.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 70271_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:20:32.52 +62:32:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153703_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 153703_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:18:22.28 +58:47:12.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21138_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 21138_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:15:23.62 +65:01:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 112593_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:21:55.06 +61:20:58.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 72532_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:45:35.61 +63:07:06.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34158_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 34158_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 01:39:32.52 +64:53:04.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76113_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290
The candidate 76113_fd_Cas-03-Q2b1x1_2026-06-08_02-57-07_20.00sec_4.90C_LIGHT_0290 did not pass the final checks
**** FOUND 02:02:02.14 +62:41:30.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 824s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:56:38.04 +59:15:33.8
01:11:20.10 +61:17:57.0
01:35:41.73 +61:13:12.4
01:38:59.06 +61:08:53.5
01:36:37.01 +58:44:44.1
01:45:15.24 +61:13:52.8
01:25:01.17 +62:50:50.6
01:34:58.00 +61:00:13.5
01:08:25.60 +59:48:03.5
01:22:50.59 +58:12:41.5
01:07:39.80 +61:12:43.6
01:33:19.99 +62:33:20.4
01:46:30.88 +57:52:14.0
01:56:13.04 +59:33:50.1
01:12:00.99 +64:42:18.7
02:12:46.81 +61:34:17.7
01:40:18.31 +61:21:06.5
01:19:42.17 +60:11:03.3
01:43:27.46 +58:38:06.2
01:17:15.17 +58:35:35.8
01:11:44.74 +61:13:57.2
01:24:55.09 +59:41:48.4
01:08:59.63 +60:47:23.6
01:13:27.33 +59:57:17.7
01:26:38.97 +59:41:39.3
01:29:37.00 +60:44:46.8
01:22:28.42 +61:07:37.9
01:19:08.74 +60:33:59.4
01:30:34.30 +59:44:32.4
01:32:19.11 +59:45:27.6
01:49:03.84 +61:04:19.1
01:46:55.24 +59:54:51.5
01:25:26.53 +60:57:44.9
01:35:24.97 +60:39:16.4
01:47:13.06 +57:44:19.2
02:03:46.69 +57:53:08.4
01:15:09.86 +60:09:05.4
01:46:13.84 +57:54:08.7
02:15:48.92 +59:33:05.6
01:36:16.27 +60:12:25.4
01:46:38.47 +60:07:34.0
01:28:07.81 +58:50:39.4
01:46:23.18 +61:12:57.3
01:50:26.25 +59:39:00.7
01:06:55.33 +59:18:56.3
01:32:05.77 +61:59:26.0
01:38:04.35 +58:10:24.7
01:12:27.47 +59:58:25.4
01:07:24.23 +60:56:07.7
01:54:06.37 +61:05:11.8
02:02:23.60 +59:42:14.9
01:33:24.96 +59:30:24.8
01:28:07.19 +59:53:49.4
01:21:45.69 +58:34:13.7
01:22:24.10 +61:13:51.9
01:09:22.99 +57:26:30.2
02:11:12.52 +62:21:13.4
01:35:35.59 +61:15:46.6
01:43:51.64 +61:52:51.2
########### Completed Cas-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:56:38.04 +59:15:33.8
01:11:20.10 +61:17:57.0
01:35:41.73 +61:13:12.4
01:38:59.06 +61:08:53.5
01:36:37.01 +58:44:44.1
01:45:15.24 +61:13:52.8
01:25:01.17 +62:50:50.6
01:34:58.00 +61:00:13.5
01:08:25.60 +59:48:03.5
01:22:50.59 +58:12:41.5
01:07:39.80 +61:12:43.6
01:33:19.99 +62:33:20.4
01:46:30.88 +57:52:14.0
01:56:13.04 +59:33:50.1
01:12:00.99 +64:42:18.7
02:12:46.81 +61:34:17.7
01:40:18.31 +61:21:06.5
01:19:42.17 +60:11:03.3
01:43:27.46 +58:38:06.2
01:17:15.17 +58:35:35.8
01:11:44.74 +61:13:57.2
01:24:55.09 +59:41:48.4
01:08:59.63 +60:47:23.6
01:13:27.33 +59:57:17.7
01:26:38.97 +59:41:39.3
01:29:37.00 +60:44:46.8
01:22:28.42 +61:07:37.9
01:19:08.74 +60:33:59.4
01:30:34.30 +59:44:32.4
01:32:19.11 +59:45:27.6
01:49:03.84 +61:04:19.1
01:46:55.24 +59:54:51.5
01:25:26.53 +60:57:44.9
01:35:24.97 +60:39:16.4
01:47:13.06 +57:44:19.2
02:03:46.69 +57:53:08.4
01:15:09.86 +60:09:05.4
01:46:13.84 +57:54:08.7
02:15:48.92 +59:33:05.6
01:36:16.27 +60:12:25.4
01:46:38.47 +60:07:34.0
01:28:07.81 +58:50:39.4
01:46:23.18 +61:12:57.3
01:50:26.25 +59:39:00.7
01:06:55.33 +59:18:56.3
01:32:05.77 +61:59:26.0
01:38:04.35 +58:10:24.7
01:12:27.47 +59:58:25.4
01:07:24.23 +60:56:07.7
01:54:06.37 +61:05:11.8
02:02:23.60 +59:42:14.9
01:33:24.96 +59:30:24.8
01:28:07.19 +59:53:49.4
01:21:45.69 +58:34:13.7
01:22:24.10 +61:13:51.9
01:09:22.99 +57:26:30.2
02:11:12.52 +62:21:13.4
01:35:35.59 +61:15:46.6
01:43:51.64 +61:52:51.2
###################################################################################
01:56:38.04 +59:15:33.8 -- not an asteroid (will add it to exclusion list)
01:11:20.10 +61:17:57.0 -- not an asteroid (will add it to exclusion list)
01:35:41.73 +61:13:12.4 -- not an asteroid (will add it to exclusion list)
01:38:59.06 +61:08:53.5 -- not an asteroid (will add it to exclusion list)
01:36:37.01 +58:44:44.1 -- not an asteroid (will add it to exclusion list)
01:45:15.24 +61:13:52.8 -- not an asteroid (will add it to exclusion list)
01:25:01.17 +62:50:50.6 -- not an asteroid (will add it to exclusion list)
01:34:58.00 +61:00:13.5 -- not an asteroid (will add it to exclusion list)
01:08:25.60 +59:48:03.5 -- not an asteroid (will add it to exclusion list)
01:22:50.59 +58:12:41.5 -- not an asteroid (will add it to exclusion list)
01:07:39.80 +61:12:43.6 -- not an asteroid (will add it to exclusion list)
01:33:19.99 +62:33:20.4 -- not an asteroid (will add it to exclusion list)
01:46:30.88 +57:52:14.0 -- not an asteroid (will add it to exclusion list)
01:56:13.04 +59:33:50.1 -- not an asteroid (will add it to exclusion list)
01:12:00.99 +64:42:18.7 -- not an asteroid (will add it to exclusion list)
02:12:46.81 +61:34:17.7 -- not an asteroid (will add it to exclusion list)
01:40:18.31 +61:21:06.5 -- not an asteroid (will add it to exclusion list)
01:19:42.17 +60:11:03.3 -- not an asteroid (will add it to exclusion list)
01:43:27.46 +58:38:06.2 -- not an asteroid (will add it to exclusion list)
01:17:15.17 +58:35:35.8 -- not an asteroid (will add it to exclusion list)
01:11:44.74 +61:13:57.2 -- not an asteroid (will add it to exclusion list)
01:24:55.09 +59:41:48.4 -- not an asteroid (will add it to exclusion list)
01:08:59.63 +60:47:23.6 -- not an asteroid (will add it to exclusion list)
01:13:27.33 +59:57:17.7 -- not an asteroid (will add it to exclusion list)
01:26:38.97 +59:41:39.3 -- not an asteroid (will add it to exclusion list)
01:29:37.00 +60:44:46.8 -- not an asteroid (will add it to exclusion list)
01:22:28.42 +61:07:37.9 -- not an asteroid (will add it to exclusion list)
01:19:08.74 +60:33:59.4 -- not an asteroid (will add it to exclusion list)
01:30:34.30 +59:44:32.4 -- not an asteroid (will add it to exclusion list)
01:32:19.11 +59:45:27.6 -- not an asteroid (will add it to exclusion list)
01:49:03.84 +61:04:19.1 -- not an asteroid (will add it to exclusion list)
01:46:55.24 +59:54:51.5 -- not an asteroid (will add it to exclusion list)
01:25:26.53 +60:57:44.9 -- not an asteroid (will add it to exclusion list)
01:35:24.97 +60:39:16.4 -- not an asteroid (will add it to exclusion list)
01:47:13.06 +57:44:19.2 -- not an asteroid (will add it to exclusion list)
02:03:46.69 +57:53:08.4 -- not an asteroid (will add it to exclusion list)
01:15:09.86 +60:09:05.4 -- not an asteroid (will add it to exclusion list)
01:46:13.84 +57:54:08.7 -- not an asteroid (will add it to exclusion list)
02:15:48.92 +59:33:05.6 -- not an asteroid (will add it to exclusion list)
01:36:16.27 +60:12:25.4 -- not an asteroid (will add it to exclusion list)
01:46:38.47 +60:07:34.0 -- not an asteroid (will add it to exclusion list)
01:28:07.81 +58:50:39.4 -- not an asteroid (will add it to exclusion list)
01:46:23.18 +61:12:57.3 -- not an asteroid (will add it to exclusion list)
01:50:26.25 +59:39:00.7 -- not an asteroid (will add it to exclusion list)
01:06:55.33 +59:18:56.3 -- not an asteroid (will add it to exclusion list)
01:32:05.77 +61:59:26.0 -- not an asteroid (will add it to exclusion list)
01:38:04.35 +58:10:24.7 -- not an asteroid (will add it to exclusion list)
01:12:27.47 +59:58:25.4 -- not an asteroid (will add it to exclusion list)
01:07:24.23 +60:56:07.7 -- not an asteroid (will add it to exclusion list)
01:54:06.37 +61:05:11.8 -- not an asteroid (will add it to exclusion list)
02:02:23.60 +59:42:14.9 -- not an asteroid (will add it to exclusion list)
01:33:24.96 +59:30:24.8 -- not an asteroid (will add it to exclusion list)
01:28:07.19 +59:53:49.4 -- not an asteroid (will add it to exclusion list)
01:21:45.69 +58:34:13.7 -- not an asteroid (will add it to exclusion list)
01:22:24.10 +61:13:51.9 -- not an asteroid (will add it to exclusion list)
01:09:22.99 +57:26:30.2 -- not an asteroid (will add it to exclusion list)
02:11:12.52 +62:21:13.4 -- not an asteroid (will add it to exclusion list)
01:35:35.59 +61:15:46.6 -- not an asteroid (will add it to exclusion list)
01:43:51.64 +61:52:51.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:06:55.33 +59:18:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:24.23 +60:56:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.80 +61:12:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:25.60 +59:48:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:59.63 +60:47:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:22.99 +57:26:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:20.10 +61:17:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:44.74 +61:13:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:00.99 +64:42:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:27.47 +59:58:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:27.33 +59:57:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:09.86 +60:09:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:15.17 +58:35:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:08.74 +60:33:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:42.17 +60:11:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:45.69 +58:34:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:24.10 +61:13:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:28.42 +61:07:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:50.59 +58:12:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:55.09 +59:41:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:01.17 +62:50:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:26.53 +60:57:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:38.97 +59:41:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:07.19 +59:53:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:07.81 +58:50:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:37.00 +60:44:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:34.30 +59:44:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:05.77 +61:59:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:19.11 +59:45:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:19.99 +62:33:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:24.96 +59:30:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:58.00 +61:00:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:24.97 +60:39:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:35.59 +61:15:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:41.73 +61:13:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:16.27 +60:12:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:37.01 +58:44:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:04.35 +58:10:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:59.06 +61:08:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:18.31 +61:21:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:27.46 +58:38:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:51.64 +61:52:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:15.24 +61:13:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:13.84 +57:54:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:23.18 +61:12:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:30.88 +57:52:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.47 +60:07:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:55.24 +59:54:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:13.06 +57:44:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:03.84 +61:04:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:26.25 +59:39:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:06.37 +61:05:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:13.04 +59:33:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:38.04 +59:15:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:23.60 +59:42:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:46.69 +57:53:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:12.52 +62:21:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:46.81 +61:34:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:48.92 +59:33:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:06:55.33 +59:18:56.3 -- not a known variable star
01:07:24.23 +60:56:07.7 -- a known variable star
01:07:39.80 +61:12:43.6 -- a known variable star
01:08:25.60 +59:48:03.5 -- not a known variable star
01:08:59.63 +60:47:23.6 -- not a known variable star
01:09:22.99 +57:26:30.2 -- not a known variable star
01:11:20.10 +61:17:57.0 -- not a known variable star
01:11:44.74 +61:13:57.2 -- a known variable star
01:12:00.99 +64:42:18.7 -- a known variable star
01:12:27.47 +59:58:25.4 -- not a known variable star
01:13:27.33 +59:57:17.7 -- not a known variable star
01:15:09.86 +60:09:05.4 -- not a known variable star
01:17:15.17 +58:35:35.8 -- not a known variable star
01:19:08.74 +60:33:59.4 -- not a known variable star
01:19:42.17 +60:11:03.3 -- a known variable star
01:21:45.69 +58:34:13.7 -- a known variable star
01:22:24.10 +61:13:51.9 -- a known variable star
01:22:28.42 +61:07:37.9 -- a known variable star
01:22:50.59 +58:12:41.5 -- a known variable star
01:24:55.09 +59:41:48.4 -- not a known variable star
01:25:01.17 +62:50:50.6 -- not a known variable star
01:25:26.53 +60:57:44.9 -- not a known variable star
01:26:38.97 +59:41:39.3 -- a known variable star
01:28:07.19 +59:53:49.4 -- not a known variable star
01:28:07.81 +58:50:39.4 -- a known variable star
01:29:37.00 +60:44:46.8 -- a known variable star
01:30:34.30 +59:44:32.4 -- not a known variable star
01:32:05.77 +61:59:26.0 -- not a known variable star
01:32:19.11 +59:45:27.6 -- a known variable star
01:33:19.99 +62:33:20.4 -- not a known variable star
01:33:24.96 +59:30:24.8 -- not a known variable star
01:34:58.00 +61:00:13.5 -- a known variable star
01:35:24.97 +60:39:16.4 -- a known variable star
01:35:35.59 +61:15:46.6 -- a known variable star
01:35:41.73 +61:13:12.4 -- not a known variable star
01:36:16.27 +60:12:25.4 -- not a known variable star
01:36:37.01 +58:44:44.1 -- a known variable star
01:38:04.35 +58:10:24.7 -- a known variable star
01:38:59.06 +61:08:53.5 -- a known variable star
01:40:18.31 +61:21:06.5 -- not a known variable star
01:43:27.46 +58:38:06.2 -- a known variable star
01:43:51.64 +61:52:51.2 -- a known variable star
01:45:15.24 +61:13:52.8 -- not a known variable star
01:46:13.84 +57:54:08.7 -- not a known variable star
01:46:23.18 +61:12:57.3 -- a known variable star
01:46:30.88 +57:52:14.0 -- not a known variable star
01:46:38.47 +60:07:34.0 -- not a known variable star
01:46:55.24 +59:54:51.5 -- not a known variable star
01:47:13.06 +57:44:19.2 -- a known variable star
01:49:03.84 +61:04:19.1 -- not a known variable star
01:50:26.25 +59:39:00.7 -- not a known variable star
01:54:06.37 +61:05:11.8 -- not a known variable star
01:56:13.04 +59:33:50.1 -- not a known variable star
01:56:38.04 +59:15:33.8 -- a known variable star
02:02:23.60 +59:42:14.9 -- not a known variable star
02:03:46.69 +57:53:08.4 -- not a known variable star
02:11:12.52 +62:21:13.4 -- not a known variable star
02:12:46.81 +61:34:17.7 -- not a known variable star
02:15:48.92 +59:33:05.6 -- a known variable star
Found 34 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
59 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 59 (excluding asteroids and hot pixels, 34 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)2461199.83097074 -observatory V36
06:44:34.51 +24:58:32.8 Mercury (0.1mag)
07:43:33.42 +23:21:06.6 Venus (-4.0mag)
02:50:01.00 +15:44:43.7 Mars (1.3mag)
07:48:33.22 +21:31:09.3 Jupiter (-1.9mag)
00:49:24.86 +02:48:53.9 Saturn (0.9mag)
04:00:14.42 +20:25:33.4 Uranus (5.8mag)
00:16:09.05 +00:16:51.0 Neptune (7.8mag)
20:33:20.95 -23:04:36.0 Pluto (14.5mag)
23:10:17.22 -04:53:09.4 Moon (-10.4mag)
-rw-r--r-- 1 apache apache 362 Jun 8 03:16 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461199.83097074:
07:48:37.53 +21:30:58.5 Io (6.0mag)
07:48:36.18 +21:31:02.6 Europa (6.2mag)
07:48:17.24 +21:31:57.8 Ganymede (5.6mag)
07:48:50.51 +21:30:13.0 Callisto (6.7mag)
07:48:50.09 +21:07:27.6 Himalia (15.6mag)
07:48:35.60 +21:31:01.5 Thebe (16.5mag)
07:48:49.30 +21:22:50.5 Elara (17.5mag)
07:50:44.36 +21:42:46.7 Pasiphae (17.7mag)
07:55:07.96 +21:32:52.4 Carme (18.9mag)
00:49:15.73 +02:48:51.1 Titan (8.7mag)
00:49:21.19 +02:49:05.7 Rhea (9.9mag)
00:49:57.06 +02:51:04.1 Iapetus (11.3mag)
00:49:21.34 +02:48:30.0 Hyperion (14.7mag)
00:50:06.94 +02:50:49.2 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 8 03:16 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461199.83097074:
17:26:00.74 -35:17:32.9 JWST
15:17:22.82 +54:00:23.6 Chandra
20:42:21.63 +36:53:57.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 8 03:16 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461199.83097074 -observatory V36
18:43:24.89 -32:39:51.2 13.6mag P/2010 H2 (Vales)
05:53:36.39 -68:03:45.2 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:49:06.61 +31:58:11.2 17.5mag C/2017 K2 (PANSTARRS)
17:14:40.59 +15:21:31.7 17.8mag C/2021 G2 (ATLAS)
21:13:31.43 -49:25:31.3 16.9mag P/2021 N1 (ZTF)
23:12:36.25 +31:35:50.7 17.2mag C/2022 E2 (ATLAS)
05:34:12.66 +26:58:34.6 16.5mag C/2022 N2 (PANSTARRS)
09:29:49.56 +31:04:39.9 16.6mag C/2022 QE78 (ATLAS)
08:50:37.16 +03:56:18.6 17.7mag C/2022 R6 (PANSTARRS)
18:28:07.96 +21:36:18.2 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:19:19.38 -11:00:31.8 17.6mag P/2023 B1 (PANSTARRS)
22:14:23.28 +66:32:14.3 17.7mag C/2023 H5 (Lemmon)
17:46:02.89 -06:42:09.2 13.7mag C/2023 R1 (PANSTARRS)
13:18:00.98 +82:57:43.6 17.9mag C/2023 X2 (Lemmon)
07:10:36.34 +64:18:48.4 17.7mag C/2024 A1 (ATLAS)
06:47:28.82 +27:50:47.3 13.6mag C/2024 E1 (Wierzchos)
15:37:10.84 +13:32:18.2 17.4mag C/2024 G6 (ATLAS)
20:12:57.31 +31:10:34.6 14.0mag C/2024 J3 (ATLAS)
04:18:09.85 -15:56:20.5 16.0mag C/2024 T5 (ATLAS)
06:06:02.42 +34:28:03.6 17.9mag C/2025 J1 (Borisov)
11:34:50.26 +52:44:26.9 17.4mag C/2025 L1 (ATLAS)
06:45:06.82 -10:52:33.2 14.1mag C/2025 R3 (PANSTARRS)
09:24:16.40 +23:20:17.1 17.9mag C/2025 V2 (Rankin)
12:39:41.82 +04:41:26.2 17.2mag C/2025 Y1 (ATLAS)
18:12:39.84 +75:09:44.5 17.9mag C/2026 A2 (Bok)
02:00:54.35 +43:25:31.0 16.1mag C/2026 B2 (Sun-Gao)
11:11:20.34 -03:41:06.2 16.5mag A/2026 E1
20:23:53.61 -08:34:46.3 8.7mag 10P/Tempel
11:02:02.21 -00:58:11.6 16.0mag 29P/Schwassmann-Wachmann
03:11:56.03 +25:39:50.5 17.7mag 47P/Ashbrook-Jackson
09:00:16.31 +23:43:47.8 16.9mag 63P/Wild
00:27:02.74 -06:21:31.4 15.7mag 65P/Gunn
06:43:53.09 +33:26:36.9 16.9mag 76P/West-Kohoutek-Ikemura
03:09:30.79 +17:14:03.0 13.8mag 78P/Gehrels
01:21:03.50 +04:52:44.8 15.6mag 88P/Howell
04:55:04.96 +30:18:47.9 15.3mag 93P/Lovas
02:43:20.33 +27:38:53.1 17.6mag 114P/Wiseman-Skiff
06:50:52.47 +33:01:59.2 15.6mag 123P/West-Hartley
09:50:24.98 +14:34:43.8 16.5mag 124P/Mrkos
03:59:15.74 +19:15:34.6 16.4mag 128P/Shoemaker-Holt
04:33:50.21 +19:05:26.8 17.7mag 131P/Mueller
05:58:54.03 +18:38:58.5 14.7mag 141P/Machholz
06:01:32.65 +17:40:56.6 14.6mag 141P-A/Machholz
04:54:46.86 +16:11:32.8 11.6mag 141P-D/Machholz
02:57:46.61 -24:40:50.5 16.8mag 161P/Hartley-IRAS
03:41:59.90 +23:51:51.7 14.9mag 162P/SidingSpring
19:36:37.20 +01:46:10.0 16.9mag 169P/NEAT
00:18:42.35 +02:29:31.9 17.9mag 220P/McNaught
16:52:04.42 -08:28:08.9 16.4mag 235P/LINEAR
07:34:58.01 +35:29:09.7 17.5mag 240P/NEAT
00:32:42.65 -02:24:40.5 16.4mag 260P/McNaught
04:04:35.84 +32:30:21.1 17.6mag 295P/LINEAR
23:53:08.47 -09:32:12.1 17.6mag 320P/McNaught
15:15:10.50 +08:05:42.6 17.4mag 391P/Kowalski
08:07:14.75 +20:44:37.7 17.9mag 450P/LONEOS
07:00:11.79 +41:41:12.1 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 8 03:16 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
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
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
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
-rw-r--r-- 1 apache apache 5.6K Jun 8 03:16 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
-rw-r--r-- 1 apache apache 189K Jun 8 03:16 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:39:35.110 +15:17:58.28 AT 2026nsc 2026-05-09.80 20.76
16:42:48.680 +20:27:18.30 AT 2026nsb 2026-05-09.80 20.54
13:34:03.440 +31:37:31.73 AT 2026nsa 2026-05-07.80 21.26
13:50:28.150 +02:34:54.72 AT 2026nrz 2026-05-22.72 21.54
13:43:59.750 +03:47:21.63 AT 2026nry 2026-05-22.69 22.05
13:17:26.150 -01:26:00.12 AT 2026nrx 2026-05-21.64 21.7
00:35:20.216 -08:28:38.64 AT 2026nrw 2026-05-19.42 18.74
23:50:43.016 -01:09:12.25 AT 2026nrv 2026-05-23.48 19.5028
22:36:47.715 +37:31:34.81 AT 2026nru 2026-05-22.43 19.4626
23:58:04.247 +20:56:44.66 AT 2026nrt 2026-05-23.48 20.1237
16:08:58.229 +36:53:23.76 AT 2026nrs 2026-05-21.36 20.3819
19:44:04.734 +84:44:44.91 SN 2026nrr 2026-05-25.47 17.808
21:42:24.388 -20:21:08.51 SN 2026nrq 2026-05-25.56 18.623
22:03:20.669 -84:55:27.45 AT 2026nrp 2026-05-22.30 19.244
23:07:53.376 -39:04:26.84 AT 2026nro 2026-05-22.38 19.567
00:40:07.848 -39:10:21.32 AT 2026nrn 2026-05-12.41 18.737
23:05:28.381 -21:25:50.28 AT 2026nrm 2026-05-25.58 18.887
19:27:28.750 -48:42:52.35 AT 2026nrl 2026-05-22.24 19.107
12:33:38.422 +12:02:05.88 AT 2026nrk 2026-05-25.29 21.322
12:32:27.199 +02:39:54.51 AT 2026nrj 2026-05-25.29 21.0728
-rw-r--r-- 1 apache apache 30K Jun 8 03:16 tns_transients_list.txt
