This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd
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 20.4189 2461211.9189 12.03 00:10:18.81 +64:39:19.4
118.54723 2.13432 galactic Cas Second-epoch detections are separated by 2.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:10:18.81 +64:39:19.4 (user input) | T | P | (position from user input) J-Ks=0.934+/- (M)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:10:18.81 +64:39:19.4: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:10:18.81 +64:39:19.4: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 10 18.81 +64 39 19.4 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 12.24 00:11:14.79 +64:53:31.2
118.68270 2.35236 galactic Cas Second-epoch detections are separated by 2.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:11:14.79 +64:53:31.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:11:14.79 +64:53:31.2: 14.74 +/- 0.13 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:11:14.79 +64:53:31.2: 15.26 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 11 14.79 +64 53 31.2 12.2 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,2461211.9189,12.24,0.05,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 20260620.4189 12.24CV 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 20.4189 2461211.9189 14.91 00:16:47.03 +64:42:55.0
119.24065 2.09218 galactic Cas Second-epoch detections are separated by 5.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:16:47.03 +64:42:55.0 (user input) | T | P | (position from user input) J-Ks=0.711+/-0.174 (K)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:16:47.03 +64:42:55.0: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:16:47.03 +64:42:55.0: 16.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 16 47.03 +64 42 55.0 14.9 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,2461211.9189,14.91,0.05,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 20260620.4189 14.91CV 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 20.4189 2461211.9189 14.96 00:04:33.49 +58:31:26.0
116.83016 -3.79137 galactic Cas Second-epoch detections are separated by 2.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.1350+58.5231 | 00:04:33.49 +58:31:26.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:04:33.49 +58:31:26.0: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:04:33.49 +58:31:26.0: 15.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 04 33.49 +58 31 26.0 15.0 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 J001.1350+58.5231,2461211.9189,14.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.1350+58.5231 20260620.4189 14.96CV 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 20.4189 2461211.9189 14.84 23:55:08.88 +62:13:12.1
116.42481 0.06155 galactic Cas Second-epoch detections are separated by 5.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:55:08.88 +62:13:12.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:55:08.88 +62:13:12.1: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:55:08.88 +62:13:12.1: 15.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 55 08.88 +62 13 12.1 14.8 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,2461211.9189,14.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.82 00:06:31.54 +62:21:03.3
117.74769 -0.06791 galactic Cas Second-epoch detections are separated by 2.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:06:31.54 +62:21:03.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:06:31.54 +62:21:03.3: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:06:31.54 +62:21:03.3: 16.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 06 31.54 +62 21 03.3 14.8 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,2461211.9189,14.82,0.05,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
target 20260620.4189 14.82CV 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 20.4189 2461211.9189 14.63 00:14:55.02 +58:40:52.3
118.18997 -3.85390 galactic Cas Second-epoch detections are separated by 5.8" and 7.5 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 | 00:14:55.02 +58:40:52.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:14:55.02 +58:40:52.3: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:14:55.02 +58:40:52.3: 15.79 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.79 +/- 0.27
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 20.4189* 00 14 55.02 +58 40 52.3 14.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.63,0.05,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 20260620.4189 14.63CV 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 20.4189 2461211.9189 14.87 00:29:41.19 +62:45:12.3
120.44531 -0.01327 galactic Cas Second-epoch detections are separated by 2.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:29:41.19 +62:45:12.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:29:41.19 +62:45:12.3: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:29:41.19 +62:45:12.3: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 29 41.19 +62 45 12.3 14.9 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,2461211.9189,14.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.87CV 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 20.4189 2461211.9189 14.68 00:18:06.59 +63:05:08.4
119.17082 0.45756 galactic Cas Second-epoch detections are separated by 8.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:06.59 +63:05:08.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:18:06.59 +63:05:08.4: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:18:06.59 +63:05:08.4: 16.15 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 18 06.59 +63 05 08.4 14.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.64 00:24:08.36 +62:24:35.2
119.77695 -0.29463 galactic Cas Second-epoch detections are separated by 1.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:24:08.36 +62:24:35.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:24:08.36 +62:24:35.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:24:08.36 +62:24:35.2: 15.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 24 08.36 +62 24 35.2 14.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.64CV 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 20.4189 2461211.9189 14.46 00:15:46.09 +64:49:40.7
119.14871 2.21856 galactic Cas Second-epoch detections are separated by 4.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:15:46.09 +64:49:40.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:15:46.09 +64:49:40.7: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:15:46.09 +64:49:40.7: 16.11 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 15 46.09 +64 49 40.7 14.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.56 00:27:25.45 +62:36:32.8
120.17396 -0.13398 galactic Cas Second-epoch detections are separated by 1.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:25.45 +62:36:32.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:27:25.45 +62:36:32.8: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:27:25.45 +62:36:32.8: 16.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 27 25.45 +62 36 32.8 14.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.57 23:25:18.12 +57:37:12.1
111.57601 -3.34016 galactic Cas Second-epoch detections are separated by 4.4" and 7.2 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 | 23:25:18.12 +57:37:12.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:25:18.12 +57:37:12.1: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:25:18.12 +57:37:12.1: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 25 18.12 +57 37 12.1 14.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.57CV 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 20.4189 2461211.9189 14.36 00:24:21.98 +59:46:31.8
119.52653 -2.91713 galactic Cas Second-epoch detections are separated by 2.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:24:21.98 +59:46:31.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:24:21.98 +59:46:31.8: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:24:21.98 +59:46:31.8: 15.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 24 21.98 +59 46 31.8 14.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.46 23:34:14.94 +65:40:48.1
115.09070 3.99024 galactic Cep Second-epoch detections are separated by 6.8" and 6.6 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 | 23:34:14.94 +65:40:48.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:34:14.94 +65:40:48.1: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:34:14.94 +65:40:48.1: 16.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461211.9189,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.42 00:24:52.06 +58:40:49.6
119.47621 -4.01291 galactic Cas Second-epoch detections are separated by 2.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 428160449319151488 | 00:24:57.33 +58:40:57.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:24:52.06 +58:40:49.6: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:24:52.06 +58:40:49.6: 15.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 24 52.06 +58 40 49.6 14.4 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 428160449319151488,2461211.9189,14.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 428160449319151488 20260620.4189 14.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.08 23:54:02.91 +64:01:04.1
116.69642 1.84304 galactic Cas Second-epoch detections are separated by 5.3" and 7.6 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 | 23:54:02.91 +64:01:04.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:54:02.91 +64:01:04.1: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:54:02.91 +64:01:04.1: 15.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 54 02.91 +64 01 04.1 14.1 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,2461211.9189,14.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.08CV 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 20.4189 2461211.9189 14.19 23:24:39.94 +64:41:36.4
113.82498 3.36707 galactic Cep Second-epoch detections are separated by 4.4" and 7.1 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 | 23:24:39.94 +64:41:36.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:24:39.94 +64:41:36.4: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:24:39.94 +64:41:36.4: 16.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461211.9189,14.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.19CV 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 20.4189 2461211.9189 14.11 23:44:16.65 +61:58:50.3
115.13275 0.13013 galactic Cas Second-epoch detections are separated by 7.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:44:16.65 +61:58:50.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:44:16.65 +61:58:50.3: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:44:16.65 +61:58:50.3: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 44 16.65 +61 58 50.3 14.1 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,2461211.9189,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.09 23:30:23.33 +64:09:25.2
114.23977 2.66163 galactic Cep Second-epoch detections are separated by 4.1" and 7.1 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 | 23:30:23.33 +64:09:25.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:30:23.33 +64:09:25.2: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:30:23.33 +64:09:25.2: 16.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461211.9189,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.99 00:18:49.80 +59:41:44.4
118.82352 -2.91572 galactic Cas Second-epoch detections are separated by 1.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:49.80 +59:41:44.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:18:49.80 +59:41:44.4: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:18:49.80 +59:41:44.4: 16.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 18 49.80 +59 41 44.4 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.70 00:22:06.77 +63:58:51.2
119.72218 1.29205 galactic Cas Second-epoch detections are separated by 3.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:06.77 +63:58:51.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:22:06.77 +63:58:51.2: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:22:06.77 +63:58:51.2: 16.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 22 06.77 +63 58 51.2 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.66 00:06:39.88 +63:07:45.2
117.89804 0.69591 galactic Cas Second-epoch detections are separated by 2.5" and 6.8 pix
The object was found in VSX21" Gaia DR3 431522755881344128
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.640 G 13.670 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:06:39.88 +63:07:45.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:06:39.88 +63:07:45.2: 15.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 06 39.88 +63 07 45.2 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 431522755881344128,2461211.9189,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 431522755881344128 20260620.4189 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.61 00:03:34.67 +63:34:49.5
117.63810 1.20166 galactic Cas Second-epoch detections are separated by 7.7" and 6.6 pix
The object was found in VSX10" Gaia DR3 431611197851413248
Type: ROT
# Max. Min./Amp. JD0 Period
15.190 G 15.220 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:03:34.67 +63:34:49.5: 15.15 +/- 0.21 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:03:34.67 +63:34:49.5: 15.21 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.18 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 03 34.67 +63 34 49.5 13.6 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 431611197851413248,2461211.9189,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 431611197851413248 20260620.4189 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.48 23:44:26.64 +61:51:10.5
115.11890 0.00166 galactic Cas Second-epoch detections are separated by 8.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:44:26.64 +61:51:10.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:44:26.64 +61:51:10.5: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:44:26.64 +61:51:10.5: 16.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 44 26.64 +61 51 10.5 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.48,0.05,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 20260620.4189 13.48CV 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 20.4189 2461211.9189 13.38 23:23:11.05 +63:45:18.2
113.36083 2.53543 galactic Cep Second-epoch detections are separated by 4.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:23:11.05 +63:45:18.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:23:11.05 +63:45:18.2: 15.13 +/- 0.16 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:23:11.05 +63:45:18.2: 14.32 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.47 +/- 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!
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,2461211.9189,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.36 00:00:30.07 +65:48:26.1
117.73971 3.45031 galactic Cas Second-epoch detections are separated by 5.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 432301068366547584 | 00:00:36.30 +65:48:49.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:00:30.07 +65:48:26.1: 14.41 +/- 0.09 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:00:30.07 +65:48:26.1: 14.37 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.39 +/- 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 20.4189* 00 00 30.07 +65 48 26.1 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 432301068366547584,2461211.9189,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 432301068366547584 20260620.4189 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.24 23:50:13.48 +61:49:47.5
115.77431 -0.18825 galactic Cas Second-epoch detections are separated by 8.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:50:13.48 +61:49:47.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:50:13.48 +61:49:47.5: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:50:13.48 +61:49:47.5: 15.85 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 50 13.48 +61 49 47.5 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.24,0.05,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 20260620.4189 13.24CV 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 20.4189 2461211.9189 13.11 00:21:17.66 +58:09:09.5
118.95161 -4.48596 galactic Cas Second-epoch detections are separated by 0.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 422130212156048384 | 00:21:15.45 +58:09:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:21:17.66 +58:09:09.5: 14.27 +/- 0.07 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:21:17.66 +58:09:09.5: 14.04 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.12 +/- 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 20.4189* 00 21 17.66 +58 09 09.5 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 422130212156048384,2461211.9189,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 422130212156048384 20260620.4189 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.04 00:11:38.65 +62:49:32.6
118.40651 0.30415 galactic Cas Second-epoch detections are separated by 2.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:11:38.65 +62:49:32.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:11:38.65 +62:49:32.6: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:11:38.65 +62:49:32.6: 14.64 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 11 38.65 +62 49 32.6 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.04 00:32:04.74 +63:10:05.9
120.74942 0.37862 galactic Cas Second-epoch detections are separated by 0.7" and 6.2 pix
The object was found in VSX 8" Gaia DR3 430789381625648896
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.970 G 12.990 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:32:04.74 +63:10:05.9: 14.90 +/- 0.20 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:32:04.74 +63:10:05.9: 15.48 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.06 +/- 0.17
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 20.4189* 00 32 04.74 +63 10 05.9 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430789381625648896,2461211.9189,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430789381625648896 20260620.4189 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.02 00:17:26.19 +61:52:46.3
118.93659 -0.72817 galactic Cas Second-epoch detections are separated by 2.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 429714334129313024 | 00:17:21.78 +61:52:29.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.687+/- (K)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:17:26.19 +61:52:46.3: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:17:26.19 +61:52:46.3: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 17 26.19 +61 52 46.3 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 429714334129313024,2461211.9189,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 429714334129313024 20260620.4189 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 12.54 00:22:02.50 +62:11:52.6
119.51142 -0.47842 galactic Cas Second-epoch detections are separated by 1.9" and 6.3 pix
The object was found in VSX 6" Gaia DR3 430488523456178304
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.490 G 12.550 G 0.113726600000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:22:02.50 +62:11:52.6: 14.90 +/- 0.14 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:22:02.50 +62:11:52.6: 14.18 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.34 +/- 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 20.4189* 00 22 02.50 +62 11 52.6 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430488523456178304,2461211.9189,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430488523456178304 20260620.4189 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.02 00:35:15.80 +63:00:42.3
121.09808 0.19761 galactic Cas Second-epoch detections are separated by 3.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 430819721271142272 | 00:35:14.88 +63:00:41.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:35:15.80 +63:00:42.3: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:35:15.80 +63:00:42.3: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 35 15.80 +63 00 42.3 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430819721271142272,2461211.9189,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430819721271142272 20260620.4189 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.02 00:21:56.58 +61:46:06.5
119.45093 -0.90377 galactic Cas Second-epoch detections are separated by 1.6" and 6.5 pix
The object was found in VSX16" Gaia DR3 430450968254479872
Type: ROT
# Max. Min./Amp. JD0 Period
18.040 G 18.150 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:21:56.58 +61:46:06.5: 15.24 +/- 0.21 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:21:56.58 +61:46:06.5: 14.86 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 21 56.58 +61 46 06.5 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430450968254479872,2461211.9189,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430450968254479872 20260620.4189 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.28 23:52:13.16 +65:38:35.1
116.87152 3.47053 galactic Cas Second-epoch detections are separated by 5.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:52:13.16 +65:38:35.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:52:13.16 +65:38:35.1: 15.85 +/- 0.36 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:52:13.16 +65:38:35.1: 15.76 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.80 +/- 0.23
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 20.4189* 23 52 13.16 +65 38 35.1 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.28,0.05,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 20260620.4189 13.28CV 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 20.4189 2461211.9189 13.22 00:10:44.24 +59:41:51.2
117.81206 -2.76899 galactic Cas Second-epoch detections are separated by 1.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:10:44.24 +59:41:51.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:10:44.24 +59:41:51.2: 14.92 +/- 0.14 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:10:44.24 +59:41:51.2: 14.48 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 10 44.24 +59 41 51.2 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.32 00:10:45.53 +63:25:28.5
118.40077 0.91128 galactic Cas Second-epoch detections are separated by 0.7" and 6.6 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 431453241826796032 | 00:10:38.95 +63:25:24.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:10:45.53 +63:25:28.5: 15.30 +/- 0.24 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:10:45.53 +63:25:28.5: 14.74 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 10 45.53 +63 25 28.5 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 431453241826796032,2461211.9189,13.32,0.05,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 431453241826796032 20260620.4189 13.32CV 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 20.4189 2461211.9189 13.29 00:10:26.03 +60:01:06.4
117.82514 -2.44611 galactic Cas Second-epoch detections are separated by 1.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:10:26.03 +60:01:06.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:10:26.03 +60:01:06.4: 14.66 +/- 0.10 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:10:26.03 +60:01:06.4: 14.56 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.61 +/- 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 20.4189* 00 10 26.03 +60 01 06.4 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.29 00:30:23.15 +60:12:42.8
120.31745 -2.55295 galactic Cas Second-epoch detections are separated by 1.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 428618086677459456 | 00:30:24.38 +60:12:17.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B3V 1960AAHam...5..215H Cl* NGC 129 Har 38
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:30:23.15 +60:12:42.8: 14.56 +/- 0.12 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:30:23.15 +60:12:42.8: 14.34 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 30 23.15 +60 12 42.8 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 428618086677459456,2461211.9189,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 428618086677459456 20260620.4189 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.39 00:22:14.89 +61:43:13.6
119.48136 -0.95559 galactic Cas Second-epoch detections are separated by 2.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 430450182288672000 | 00:22:11.56 +61:42:49.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:22:14.89 +61:43:13.6: 14.29 +/- 0.09 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:22:14.89 +61:43:13.6: 14.39 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 22 14.89 +61 43 13.6 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430450182288672000,2461211.9189,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430450182288672000 20260620.4189 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.42 00:23:54.03 +60:22:48.1
119.53279 -2.30985 galactic Cas Second-epoch detections are separated by 1.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:23:54.03 +60:22:48.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:23:54.03 +60:22:48.1: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:23:54.03 +60:22:48.1: 15.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 23 54.03 +60 22 48.1 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.45 00:36:08.60 +62:39:27.6
121.17672 -0.16195 galactic Cas Second-epoch detections are separated by 2.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:36:08.60 +62:39:27.6 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.088 (G)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:36:08.60 +62:39:27.6: 14.29 +/- 0.10 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:36:08.60 +62:39:27.6: 14.74 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 36 08.60 +62 39 27.6 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.45,0.05,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 20260620.4189 13.45CV 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 20.4189 2461211.9189 13.55 23:59:12.50 +63:48:15.4
117.20612 1.51468 galactic Cas Second-epoch detections are separated by 8.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:59:12.50 +63:48:15.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:59:12.50 +63:48:15.4: 14.67 +/- 0.11 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:59:12.50 +63:48:15.4: 14.93 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 59 12.50 +63 48 15.4 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.55,0.05,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
target 20260620.4189 13.55CV 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 20.4189 2461211.9189 13.51 00:15:02.46 +61:26:05.2
118.59432 -1.13006 galactic Cas Second-epoch detections are separated by 2.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 429599538245809280 | 00:14:59.83 +61:26:29.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:15:02.46 +61:26:05.2: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:15:02.46 +61:26:05.2: 15.70 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 15 02.46 +61 26 05.2 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 429599538245809280,2461211.9189,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 429599538245809280 20260620.4189 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.55 00:21:47.25 +61:02:51.3
119.34984 -1.61778 galactic Cas Second-epoch detections are separated by 2.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:21:47.25 +61:02:51.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:21:47.25 +61:02:51.3: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:21:47.25 +61:02:51.3: 15.91 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 21 47.25 +61 02 51.3 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.55,0.05,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
target 20260620.4189 13.55CV 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 20.4189 2461211.9189 13.55 23:27:44.47 +57:32:13.4
111.85916 -3.52423 galactic Cas Second-epoch detections are separated by 3.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J351.9323+57.5275 | 23:27:44.47 +57:32:13.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:27:44.47 +57:32:13.4: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:27:44.47 +57:32:13.4: 15.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 27 44.47 +57 32 13.4 13.6 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 J351.9323+57.5275,2461211.9189,13.55,0.05,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 J351.9323+57.5275 20260620.4189 13.55CV 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 20.4189 2461211.9189 13.64 00:11:16.41 +59:58:35.0
117.92230 -2.50412 galactic Cas Second-epoch detections are separated by 1.1" and 6.7 pix
The object was found in VSX11" ASASSN-V J001114.97+595833.6
Type: ROT
# Max. Min./Amp. JD0 Period
14.320 g Y 0.240 g 2459082.75700 84.170000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:11:16.41 +59:58:35.0: 15.09 +/- 0.16 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:11:16.41 +59:58:35.0: 14.50 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 11 16.41 +59 58 35.0 13.6 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
ASASSN-V J001114.97+595833.6,2461211.9189,13.64,0.05,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
ASASSN-V J001114.97+595833.6 20260620.4189 13.64CV 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 20.4189 2461211.9189 13.65 00:40:45.62 +64:16:36.7
121.77332 1.42914 galactic Cas Second-epoch detections are separated by 5.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:40:45.62 +64:16:36.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:40:45.62 +64:16:36.7: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:40:45.62 +64:16:36.7: 15.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 40 45.62 +64 16 36.7 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 13.65CV 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 20.4189 2461211.9189 13.69 00:23:45.07 +59:32:01.1
119.42344 -3.14937 galactic Cas Second-epoch detections are separated by 0.5" and 6.4 pix
The object was found in VSX 8" Mis V1302
Type: M
# Max. Min./Amp. JD0 Period
14.231 r Y 4.383 r 2458514.64480 308.827887100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:23:45.07 +59:32:01.1: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:23:45.07 +59:32:01.1: 15.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 23 45.07 +59 32 01.1 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1302,2461211.9189,13.69,0.05,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
Mis V1302 20260620.4189 13.69CV 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 20.4189 2461211.9189 13.80 00:23:31.32 +65:19:48.0
120.02187 2.61610 galactic Cas Second-epoch detections are separated by 5.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:23:31.32 +65:19:48.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:23:31.32 +65:19:48.0: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:23:31.32 +65:19:48.0: 15.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 23 31.32 +65 19 48.0 13.8 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,2461211.9189,13.80,0.05,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 20260620.4189 13.80CV 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 20.4189 2461211.9189 13.81 00:02:05.43 +63:18:21.2
117.42333 0.96315 galactic Cas Second-epoch detections are separated by 8.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:02:05.43 +63:18:21.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:02:05.43 +63:18:21.2: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:02:05.43 +63:18:21.2: 15.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 02 05.43 +63 18 21.2 13.8 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,2461211.9189,13.81,0.05,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
target 20260620.4189 13.81CV 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 20.4189 2461211.9189 13.80 00:36:20.85 +62:40:04.6
121.20072 -0.15307 galactic Cas Second-epoch detections are separated by 2.7" and 6.0 pix
The object was found in VSX14" Gaia DR3 430712239707921664
Type: ROT
# Max. Min./Amp. JD0 Period
15.980 G 16.020 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:36:20.85 +62:40:04.6: 15.13 +/- 0.25 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:36:20.85 +62:40:04.6: 14.78 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 36 20.85 +62 40 04.6 13.8 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 430712239707921664,2461211.9189,13.80,0.05,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 430712239707921664 20260620.4189 13.80CV 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 20.4189 2461211.9189 13.78 00:01:54.79 +63:10:51.2
117.37992 0.84424 galactic Cas Second-epoch detections are separated by 6.6" and 6.5 pix
The object was found in VSX 9" Gaia DR3 430085900345681152
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.900 G 13.930 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:01:54.79 +63:10:51.2: 15.16 +/- 0.25 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:01:54.79 +63:10:51.2: 14.78 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 01 54.79 +63 10 51.2 13.8 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 430085900345681152,2461211.9189,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430085900345681152 20260620.4189 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.89 00:34:36.24 +62:38:19.3
120.99906 -0.16986 galactic Cas Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:34:36.24 +62:38:19.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:34:36.24 +62:38:19.3: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:34:36.24 +62:38:19.3: 15.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 34 36.24 +62 38 19.3 13.9 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,2461211.9189,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.98 23:44:59.54 +61:59:31.2
115.21680 0.11965 galactic Cas Second-epoch detections are separated by 8.8" and 6.9 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 | 23:44:59.54 +61:59:31.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:44:59.54 +61:59:31.2: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:44:59.54 +61:59:31.2: 16.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 44 59.54 +61 59 31.2 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 13.98CV 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 20.4189 2461211.9189 13.96 00:27:06.32 +61:13:07.6
120.00629 -1.51467 galactic Cas Second-epoch detections are separated by 1.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 428874994440134144 | 00:27:06.75 +61:12:23.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1956PMcCO..13a....B AG+60 51
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:27:06.32 +61:13:07.6: 15.76 +/- 0.31 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:27:06.32 +61:13:07.6: 15.38 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.51 +/- 0.18
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 20.4189* 00 27 06.32 +61 13 07.6 14.0 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 428874994440134144,2461211.9189,13.96,0.05,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 428874994440134144 20260620.4189 13.96CV 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 20.4189 2461211.9189 14.03 00:28:27.63 +63:43:01.9
120.39138 0.95885 galactic Cas Second-epoch detections are separated by 3.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:28:27.63 +63:43:01.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:28:27.63 +63:43:01.9: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:28:27.63 +63:43:01.9: 15.92 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 28 27.63 +63 43 01.9 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.00 00:20:42.27 +58:20:31.5
118.89679 -4.28867 galactic Cas Second-epoch detections are separated by 3.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 422180377375790592 | 00:20:39.15 +58:20:49.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:20:42.27 +58:20:31.5: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:20:42.27 +58:20:31.5: 15.24 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.18
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 20.4189* 00 20 42.27 +58 20 31.5 14.0 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 422180377375790592,2461211.9189,14.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 422180377375790592 20260620.4189 14.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.98 00:09:15.91 +59:38:43.9
117.62006 -2.79057 galactic Cas Second-epoch detections are separated by 1.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J002.3361+59.6510 | 00:09:20.90 +59:38:31.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:09:15.91 +59:38:43.9: 14.98 +/- 0.16 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:09:15.91 +59:38:43.9: 14.99 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 09 15.91 +59 38 43.9 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J002.3361+59.6510,2461211.9189,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J002.3361+59.6510 20260620.4189 13.98CV 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 20.4189 2461211.9189 13.99 00:23:26.38 +62:17:45.0
119.68405 -0.39922 galactic Cas Second-epoch detections are separated by 1.0" and 6.5 pix
The object was found in VSX15" ZTF J002328.10+621735.6
Type: BY
# Max. Min./Amp. JD0 Period
15.949 r Y 0.044 r 2458347.92660 7.690530500000
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:23:26.38 +62:17:45.0: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:23:26.38 +62:17:45.0: 15.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 23 26.38 +62 17 45.0 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J002328.10+621735.6,2461211.9189,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J002328.10+621735.6 20260620.4189 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.07 00:24:10.80 +62:20:28.7
119.77440 -0.36322 galactic Cas Second-epoch detections are separated by 1.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:24:10.80 +62:20:28.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:24:10.80 +62:20:28.7: 15.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:24:10.80 +62:20:28.7: 15.30 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 24 10.80 +62 20 28.7 14.1 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,2461211.9189,14.07,0.05,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 20260620.4189 14.07CV 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 20.4189 2461211.9189 14.04 23:46:28.29 +63:40:33.6
115.80418 1.70692 galactic Cas Second-epoch detections are separated by 4.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:46:28.29 +63:40:33.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:46:28.29 +63:40:33.6: 15.28 +/- 0.16 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:46:28.29 +63:40:33.6: 16.00 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.42 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 46 28.29 +63 40 33.6 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.20 00:21:54.61 +64:21:30.0
119.74328 1.66955 galactic Cas Second-epoch detections are separated by 2.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:21:54.61 +64:21:30.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:21:54.61 +64:21:30.0: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:21:54.61 +64:21:30.0: 15.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 21 54.61 +64 21 30.0 14.2 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,2461211.9189,14.20,0.05,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 20260620.4189 14.20CV 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 20.4189 2461211.9189 14.10 23:48:52.99 +61:40:27.3
115.58317 -0.30173 galactic Cas Second-epoch detections are separated by 7.1" and 7.1 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 | 23:48:52.99 +61:40:27.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:48:52.99 +61:40:27.3: 15.22 +/- 0.22 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:48:52.99 +61:40:27.3: 15.31 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.17
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 20.4189* 23 48 52.99 +61 40 27.3 14.1 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,2461211.9189,14.10,0.05,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
target 20260620.4189 14.10CV 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 20.4189 2461211.9189 14.18 00:17:56.90 +59:09:20.5
118.64288 -3.43688 galactic Cas Second-epoch detections are separated by 2.5" and 6.3 pix
The object was found in VSX 7" V0659 Cas
Type: M
# Max. Min./Amp. JD0 Period
13.500 V < 17.000 V 2442638.00000 344.000000000000 M5/7e
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:17:56.90 +59:09:20.5: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:17:56.90 +59:09:20.5: 15.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 17 56.90 +59 09 20.5 14.2 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
V0659 Cas,2461211.9189,14.18,0.05,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
V0659 Cas 20260620.4189 14.18CV 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 20.4189 2461211.9189 14.13 00:12:01.75 +57:56:55.7
117.70582 -4.52251 galactic Cas Second-epoch detections are separated by 2.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J002.9861+57.9471 | 00:12:01.75 +57:56:55.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:12:01.75 +57:56:55.7: 15.12 +/- 0.18 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:12:01.75 +57:56:55.7: 15.12 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 12 01.75 +57 56 55.7 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J002.9861+57.9471,2461211.9189,14.13,0.05,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
ATO J002.9861+57.9471 20260620.4189 14.13CV 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 20.4189 2461211.9189 14.15 00:07:55.37 +63:41:10.3
118.13172 1.22074 galactic Cas Second-epoch detections are separated by 2.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 431648134564246656 | 00:07:57.70 +63:40:43.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: Ae 1956BOTT....2o..16G GGR 169
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:07:55.37 +63:41:10.3: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:07:55.37 +63:41:10.3: 15.55 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.55 +/- 0.27
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 20.4189* 00 07 55.37 +63 41 10.3 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 431648134564246656,2461211.9189,14.15,0.05,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
Gaia DR3 431648134564246656 20260620.4189 14.15CV 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 20.4189 2461211.9189 14.17 00:05:33.91 +62:32:06.1
117.67056 0.13281 galactic Cas Second-epoch detections are separated by 2.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:05:33.91 +62:32:06.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:05:33.91 +62:32:06.1: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:05:33.91 +62:32:06.1: 15.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 05 33.91 +62 32 06.1 14.2 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,2461211.9189,14.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.14 00:28:42.73 +63:24:32.8
120.39198 0.64949 galactic Cas Second-epoch detections are separated by 3.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:28:42.73 +63:24:32.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:28:42.73 +63:24:32.8: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:28:42.73 +63:24:32.8: 15.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 28 42.73 +63 24 32.8 14.1 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,2461211.9189,14.14,0.05,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
target 20260620.4189 14.14CV 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 20.4189 2461211.9189 14.16 00:32:03.42 +58:44:20.9
120.41349 -4.03781 galactic Cas Second-epoch detections are separated by 4.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 428023766280107648 | 00:32:00.73 +58:44:58.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.526+/-0.139 (K)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:32:03.42 +58:44:20.9: 15.46 +/- 0.24 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:32:03.42 +58:44:20.9: 15.30 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.37 +/- 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 20.4189* 00 32 03.42 +58 44 20.9 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 428023766280107648,2461211.9189,14.16,0.05,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
Gaia DR3 428023766280107648 20260620.4189 14.16CV 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 20.4189 2461211.9189 14.17 00:20:28.24 +63:28:45.2
119.48310 0.81503 galactic Cas Second-epoch detections are separated by 3.4" and 6.1 pix
The object was found in VSX13" ZTF J002026.38+632848.1
Type: RS
# Max. Min./Amp. JD0 Period
14.643 r Y 0.044 r 2458456.67850 1.717188500000
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:20:28.24 +63:28:45.2: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:20:28.24 +63:28:45.2: 16.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 20 28.24 +63 28 45.2 14.2 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 J002026.38+632848.1,2461211.9189,14.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J002026.38+632848.1 20260620.4189 14.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.28 00:13:40.51 +62:31:06.5
118.59093 -0.03457 galactic Cas Second-epoch detections are separated by 1.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:13:40.51 +62:31:06.5 (user input) | T | P | (position from user input) J-Ks=0.831+/-0.123 (M)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:13:40.51 +62:31:06.5: 15.82 +/- 0.36 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:13:40.51 +62:31:06.5: 15.82 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.82 +/- 0.36
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 13 40.51 +62 31 06.5 14.3 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,2461211.9189,14.28,0.05,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 20260620.4189 14.28CV 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 20.4189 2461211.9189 14.07 23:24:49.11 +57:25:54.6
111.45273 -3.49663 galactic Cas Second-epoch detections are separated by 6.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2009366025277335936 | 23:24:44.02 +57:25:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:24:49.11 +57:25:54.6: 15.22 +/- 0.18 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:24:49.11 +57:25:54.6: 15.42 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.30 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 24 49.11 +57 25 54.6 14.1 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 2009366025277335936,2461211.9189,14.07,0.05,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 2009366025277335936 20260620.4189 14.07CV 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 20.4189 2461211.9189 14.22 00:19:13.59 +63:35:39.0
119.35958 0.94606 galactic Cas Second-epoch detections are separated by 5.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:13.59 +63:35:39.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:19:13.59 +63:35:39.0: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:19:13.59 +63:35:39.0: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 19 13.59 +63 35 39.0 14.2 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,2461211.9189,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.20 00:05:21.04 +63:24:15.2
117.80075 0.99255 galactic Cas Second-epoch detections are separated by 3.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:05:21.04 +63:24:15.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:05:21.04 +63:24:15.2: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:05:21.04 +63:24:15.2: 15.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 05 21.04 +63 24 15.2 14.2 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,2461211.9189,14.20,0.05,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 20260620.4189 14.20CV 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 20.4189 2461211.9189 14.32 00:19:24.93 +59:23:46.2
118.85966 -3.22215 galactic Cas Second-epoch detections are separated by 2.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:24.93 +59:23:46.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:19:24.93 +59:23:46.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:19:24.93 +59:23:46.2: 16.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 19 24.93 +59 23 46.2 14.3 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,2461211.9189,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.32CV 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 20.4189 2461211.9189 14.29 00:12:19.82 +60:34:41.4
118.14415 -1.92953 galactic Cas Second-epoch detections are separated by 2.1" and 6.6 pix
The object was found in VSX10" ZTF J001218.47+603439.1
Type: RS
# Max. Min./Amp. JD0 Period
14.158 r Y 0.065 r 2458493.36760 6.999803100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:12:19.82 +60:34:41.4: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:12:19.82 +60:34:41.4: 15.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 12 19.82 +60 34 41.4 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J001218.47+603439.1,2461211.9189,14.29,0.05,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
ZTF J001218.47+603439.1 20260620.4189 14.29CV 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 20.4189 2461211.9189 14.26 00:30:54.68 +63:26:03.2
120.63922 0.65389 galactic Cas Second-epoch detections are separated by 5.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 430890261815554304 | 00:30:49.14 +63:25:50.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:30:54.68 +63:26:03.2: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:30:54.68 +63:26:03.2: 15.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 30 54.68 +63 26 03.2 14.3 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
Large-amplitude variable Gaia DR2 430890261815554304,2461211.9189,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 430890261815554304 20260620.4189 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.32 00:22:10.68 +64:32:05.5
119.79210 1.84164 galactic Cas Second-epoch detections are separated by 2.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:10.68 +64:32:05.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:22:10.68 +64:32:05.5: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:22:10.68 +64:32:05.5: 15.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 22 10.68 +64 32 05.5 14.3 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,2461211.9189,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.32CV 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 20.4189 2461211.9189 14.36 00:28:07.31 +63:12:32.5
120.30809 0.45612 galactic Cas Second-epoch detections are separated by 2.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 430978154028648576 | 00:28:01.88 +63:12:56.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1966UppAn...5d...1O [O66] 8:1097
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:28:07.31 +63:12:32.5: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:28:07.31 +63:12:32.5: 16.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 28 07.31 +63 12 32.5 14.4 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 430978154028648576,2461211.9189,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430978154028648576 20260620.4189 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.28 00:16:22.75 +61:54:20.3
118.81665 -0.68566 galactic Cas Second-epoch detections are separated by 1.9" and 6.5 pix
The object was found in VSX 4" Gaia DR3 429726772354547200
Type: ROT
# Max. Min./Amp. JD0 Period
16.500 G 16.610 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:16:22.75 +61:54:20.3: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:16:22.75 +61:54:20.3: 15.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 16 22.75 +61 54 20.3 14.3 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 429726772354547200,2461211.9189,14.28,0.05,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 429726772354547200 20260620.4189 14.28CV 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 20.4189 2461211.9189 14.35 00:41:22.76 +64:38:36.1
121.85477 1.79265 galactic Cas Second-epoch detections are separated by 3.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:41:22.76 +64:38:36.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:41:22.76 +64:38:36.1: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:41:22.76 +64:38:36.1: 15.54 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.54 +/- 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 20.4189* 00 41 22.76 +64 38 36.1 14.3 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,2461211.9189,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.32 00:05:24.33 +57:58:25.5
116.84103 -4.35259 galactic Cas Second-epoch detections are separated by 0.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.3637+57.9625 | 00:05:24.33 +57:58:25.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:05:24.33 +57:58:25.5: 15.79 +/- 0.30 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:05:24.33 +57:58:25.5: 15.27 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.42 +/- 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 20.4189* 00 05 24.33 +57 58 25.5 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.3637+57.9625,2461211.9189,14.32,0.05,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
ATO J001.3637+57.9625 20260620.4189 14.32CV 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 20.4189 2461211.9189 14.31 00:22:22.12 +59:28:19.3
119.24204 -3.19130 galactic Cas Second-epoch detections are separated by 3.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:22.12 +59:28:19.3 (user input) | T | P | (position from user input) J-Ks=1.216+/- (M)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:22:22.12 +59:28:19.3: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:22:22.12 +59:28:19.3: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 22 22.12 +59 28 19.3 14.3 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,2461211.9189,14.31,0.05,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 20260620.4189 14.31CV 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 20.4189 2461211.9189 14.37 00:09:20.47 +58:03:30.0
117.37051 -4.35813 galactic Cas Second-epoch detections are separated by 4.2" and 6.3 pix
The object was found in VSX11" Gaia DR3 422492432519415808
Type: ROT
# Max. Min./Amp. JD0 Period
14.400 G 14.440 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:09:20.47 +58:03:30.0: 15.39 +/- 0.22 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:09:20.47 +58:03:30.0: 15.45 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.42 +/- 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 20.4189* 00 09 20.47 +58 03 30.0 14.4 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 422492432519415808,2461211.9189,14.37,0.05,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 422492432519415808 20260620.4189 14.37CV 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 20.4189 2461211.9189 14.38 00:11:48.28 +61:45:47.8
118.26190 -0.74858 galactic Cas Second-epoch detections are separated by 1.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:11:48.28 +61:45:47.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:11:48.28 +61:45:47.8: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:11:48.28 +61:45:47.8: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 11 48.28 +61 45 47.8 14.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.37 00:05:11.91 +60:11:01.0
117.20940 -2.17338 galactic Cas Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:05:11.91 +60:11:01.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:05:11.91 +60:11:01.0: 15.66 +/- 0.26 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:05:11.91 +60:11:01.0: 15.33 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.45 +/- 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 20.4189* 00 05 11.91 +60 11 01.0 14.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.37,0.05,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 20260620.4189 14.37CV 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 20.4189 2461211.9189 14.43 23:26:59.12 +64:37:21.5
114.03701 3.21937 galactic Cep Second-epoch detections are separated by 5.2" and 7.2 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 | 23:26:59.12 +64:37:21.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:26:59.12 +64:37:21.5: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:26:59.12 +64:37:21.5: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461211.9189,14.43,0.05,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
target 20260620.4189 14.43CV 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 20.4189 2461211.9189 14.45 00:31:04.23 +58:32:51.9
120.27038 -4.21871 galactic Cas Second-epoch detections are separated by 2.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 428003837631079040 | 00:31:01.83 +58:33:09.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.767+/-0.197 (K)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:31:04.23 +58:32:51.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:31:04.23 +58:32:51.9: 15.54 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.54 +/- 0.25
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 20.4189* 00 31 04.23 +58 32 51.9 14.4 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 428003837631079040,2461211.9189,14.45,0.05,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 428003837631079040 20260620.4189 14.45CV 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 20.4189 2461211.9189 14.45 23:58:29.51 +63:50:02.4
117.13472 1.55979 galactic Cas Second-epoch detections are separated by 4.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:29.51 +63:50:02.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:58:29.51 +63:50:02.4: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:58:29.51 +63:50:02.4: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 58 29.51 +63 50 02.4 14.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.45,0.05,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 20260620.4189 14.45CV 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 20.4189 2461211.9189 14.38 00:20:42.97 +62:52:57.8
119.43936 0.21949 galactic Cas Second-epoch detections are separated by 3.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:20:42.97 +62:52:57.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:20:42.97 +62:52:57.8: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:20:42.97 +62:52:57.8: 15.92 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 20 42.97 +62 52 57.8 14.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.53 23:42:11.08 +58:56:31.9
114.09016 -2.73558 galactic Cas Second-epoch detections are separated by 4.1" and 7.2 pix
The object was found in VSX 8" IRAS 23397+5839
Type: M
# Max. Min./Amp. JD0 Period
15.600 V < 17.900 V 2457749.00000 330.000000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:42:11.08 +58:56:31.9: 15.65 +/- 0.25 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:42:11.08 +58:56:31.9: 16.04 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.65 +/- 0.25
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 20.4189* 23 42 11.08 +58 56 31.9 14.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IRAS 23397+5839,2461211.9189,14.53,0.05,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
IRAS 23397+5839 20260620.4189 14.53CV 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 20.4189 2461211.9189 14.54 23:53:09.74 +62:18:07.4
116.21749 0.19243 galactic Cas Second-epoch detections are separated by 8.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:53:09.74 +62:18:07.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:53:09.74 +62:18:07.4: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:53:09.74 +62:18:07.4: 15.92 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 53 09.74 +62 18 07.4 14.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.63 23:49:37.36 +61:05:24.8
115.52984 -0.89002 galactic Cas Second-epoch detections are separated by 2.3" and 6.7 pix
The object was found in VSX12" NSVS J2349357+610521
Type: M
# Max. Min./Amp. JD0 Period
17.456 g Y 4.268 g 2458535.29910 375.860830000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:49:37.36 +61:05:24.8: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:49:37.36 +61:05:24.8: 16.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 49 37.36 +61 05 24.8 14.6 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
NSVS J2349357+610521,2461211.9189,14.63,0.05,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 J2349357+610521 20260620.4189 14.63CV 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 20.4189 2461211.9189 14.76 00:36:09.90 +62:54:05.0
121.19364 0.08120 galactic Cas Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:36:09.90 +62:54:05.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:36:09.90 +62:54:05.0: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:36:09.90 +62:54:05.0: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 36 09.90 +62 54 05.0 14.8 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,2461211.9189,14.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.68 00:15:05.59 +63:31:33.7
118.89445 0.93955 galactic Cas Second-epoch detections are separated by 2.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:15:05.59 +63:31:33.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:15:05.59 +63:31:33.7: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:15:05.59 +63:31:33.7: 15.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 15 05.59 +63 31 33.7 14.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,14.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.82 00:12:27.40 +60:10:24.0
118.09842 -2.33208 galactic Cas Second-epoch detections are separated by 1.8" and 6.6 pix
The object was found in VSX15" Gaia DR3 429180486875088512
Type: ROT
# Max. Min./Amp. JD0 Period
15.090 G 15.120 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:12:27.40 +60:10:24.0: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:12:27.40 +60:10:24.0: 16.11 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 12 27.40 +60 10 24.0 14.8 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 429180486875088512,2461211.9189,14.82,0.05,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 429180486875088512 20260620.4189 14.82CV 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 20.4189 2461211.9189 14.67 23:28:12.92 +63:48:23.1
113.90347 2.40309 galactic Cep Second-epoch detections are separated by 4.3" and 6.9 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 | 23:28:12.92 +63:48:23.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:28:12.92 +63:48:23.1: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:28:12.92 +63:48:23.1: 16.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461211.9189,14.67,0.05,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 20260620.4189 14.67CV 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 20.4189 2461211.9189 14.87 23:48:54.64 +64:22:28.6
116.23423 2.31902 galactic Cas Second-epoch detections are separated by 4.4" and 6.6 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 | 23:48:54.64 +64:22:28.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:48:54.64 +64:22:28.6: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:48:54.64 +64:22:28.6: 15.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 48 54.64 +64 22 28.6 14.9 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,2461211.9189,14.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.87CV 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 20.4189 2461211.9189 14.69 00:21:41.13 +62:06:54.0
119.46060 -0.55605 galactic Cas Second-epoch detections are separated by 1.8" and 6.4 pix
The object was found in VSX11" Gaia DR3 430463097249520640
Type: ROT
# Max. Min./Amp. JD0 Period
14.360 G 14.400 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:21:41.13 +62:06:54.0: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:21:41.13 +62:06:54.0: 15.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 21 41.13 +62 06 54.0 14.7 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 430463097249520640,2461211.9189,14.69,0.05,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 430463097249520640 20260620.4189 14.69CV 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 20.4189 2461211.9189 14.79 00:08:40.94 +63:50:28.9
118.24036 1.35976 galactic Cas Second-epoch detections are separated by 2.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:08:40.94 +63:50:28.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:08:40.94 +63:50:28.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:08:40.94 +63:50:28.9: 15.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 08 40.94 +63 50 28.9 14.8 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,2461211.9189,14.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.89 00:32:46.68 +59:50:59.1
120.58770 -2.93704 galactic Cas Second-epoch detections are separated by 3.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:32:46.68 +59:50:59.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:32:46.68 +59:50:59.1: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:32:46.68 +59:50:59.1: 16.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 32 46.68 +59 50 59.1 14.9 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,2461211.9189,14.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.79 23:24:47.03 +63:17:45.8
113.37678 2.04328 galactic Cas Second-epoch detections are separated by 5.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:24:47.03 +63:17:45.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:24:47.03 +63:17:45.8: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:24:47.03 +63:17:45.8: 15.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 24 47.03 +63 17 45.8 14.8 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,2461211.9189,14.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.85 23:30:17.78 +64:29:51.3
114.33552 2.98867 galactic Cep Second-epoch detections are separated by 4.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:30:17.78 +64:29:51.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:30:17.78 +64:29:51.3: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:30:17.78 +64:29:51.3: 16.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461211.9189,14.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.83 00:27:40.15 +64:55:42.0
120.41580 2.17277 galactic Cas Second-epoch detections are separated by 7.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:40.15 +64:55:42.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:27:40.15 +64:55:42.0: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:27:40.15 +64:55:42.0: 16.17 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 27 40.15 +64 55 42.0 14.8 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,2461211.9189,14.83,0.05,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 20260620.4189 14.83CV 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 20.4189 2461211.9189 14.84 00:10:35.06 +59:42:25.3
117.79448 -2.75659 galactic Cas Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:10:35.06 +59:42:25.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:10:35.06 +59:42:25.3: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:10:35.06 +59:42:25.3: 15.79 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 10 35.06 +59 42 25.3 14.8 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,2461211.9189,14.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.88 00:11:06.41 +63:53:48.0
118.51280 1.37150 galactic Cas Second-epoch detections are separated by 1.0" and 6.6 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 431490797020845440 | 00:11:10.30 +63:54:23.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:11:06.41 +63:53:48.0: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:11:06.41 +63:53:48.0: 15.91 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.91 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 11 06.41 +63 53 48.0 14.9 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 431490797020845440,2461211.9189,14.88,0.05,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 431490797020845440 20260620.4189 14.88CV 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 20.4189 2461211.9189 14.82 00:07:31.54 +62:23:56.3
117.87013 -0.04043 galactic Cas Second-epoch detections are separated by 1.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:07:31.54 +62:23:56.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:07:31.54 +62:23:56.3: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:07:31.54 +62:23:56.3: 15.85 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 07 31.54 +62 23 56.3 14.8 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,2461211.9189,14.82,0.05,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
target 20260620.4189 14.82CV 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 20.4189 2461211.9189 14.85 00:41:03.00 +65:48:58.1
121.86690 2.96587 galactic Cas Second-epoch detections are separated by 1.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:41:03.00 +65:48:58.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:41:03.00 +65:48:58.1: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:41:03.00 +65:48:58.1: 16.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 41 03.00 +65 48 58.1 14.8 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,2461211.9189,14.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.82 00:05:59.75 +64:46:53.0
118.11348 2.33562 galactic Cas Second-epoch detections are separated by 7.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:05:59.75 +64:46:53.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:05:59.75 +64:46:53.0: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:05:59.75 +64:46:53.0: 15.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 05 59.75 +64 46 53.0 14.8 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,2461211.9189,14.82,0.05,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
target 20260620.4189 14.82CV 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 20.4189 2461211.9189 14.77 23:44:00.19 +63:59:36.5
115.62139 2.08303 galactic Cas Second-epoch detections are separated by 7.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:44:00.19 +63:59:36.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:44:00.19 +63:59:36.5: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:44:00.19 +63:59:36.5: 16.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 44 00.19 +63 59 36.5 14.8 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,2461211.9189,14.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.93 00:01:08.45 +62:53:36.4
117.23872 0.57900 galactic Cas Second-epoch detections are separated by 8.7" and 6.8 pix
The object was found in VSX22" ZTF J000110.90+625322.0
Type: BY
# Max. Min./Amp. JD0 Period
17.044 r Y 0.063 r 2458285.90290 0.877201800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:01:08.45 +62:53:36.4: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:01:08.45 +62:53:36.4: 15.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 01 08.45 +62 53 36.4 14.9 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 J000110.90+625322.0,2461211.9189,14.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J000110.90+625322.0 20260620.4189 14.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.82 00:26:09.80 +66:06:26.9
120.37266 3.36140 galactic Cas Second-epoch detections are separated by 2.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:09.80 +66:06:26.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:26:09.80 +66:06:26.9: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:26:09.80 +66:06:26.9: 16.15 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 26 09.80 +66 06 26.9 14.8 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,2461211.9189,14.82,0.05,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
target 20260620.4189 14.82CV 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 20.4189 2461211.9189 14.87 00:07:23.74 +64:28:32.7
118.20844 2.00867 galactic Cas Second-epoch detections are separated by 5.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:07:23.74 +64:28:32.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:07:23.74 +64:28:32.7: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:07:23.74 +64:28:32.7: 16.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 07 23.74 +64 28 32.7 14.9 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,2461211.9189,14.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.87CV 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 20.4189 2461211.9189 14.84 23:21:47.31 +63:52:52.7
113.25835 2.70619 galactic Cep Second-epoch detections are separated by 6.4" and 7.2 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 | 23:21:47.31 +63:52:52.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:21:47.31 +63:52:52.7: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:21:47.31 +63:52:52.7: 15.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461211.9189,14.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.85 00:22:51.43 +66:01:51.6
120.03065 3.32038 galactic Cas Second-epoch detections are separated by 2.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:51.43 +66:01:51.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:22:51.43 +66:01:51.6: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:22:51.43 +66:01:51.6: 16.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 22 51.43 +66 01 51.6 14.8 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,2461211.9189,14.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.79 00:11:43.97 +61:21:08.7
118.19046 -1.15327 galactic Cas Second-epoch detections are separated by 4.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:11:43.97 +61:21:08.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:11:43.97 +61:21:08.7: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:11:43.97 +61:21:08.7: 16.22 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 11 43.97 +61 21 08.7 14.8 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,2461211.9189,14.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 14.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 14.90 23:28:06.19 +64:26:26.5
114.09294 3.00860 galactic Cep Second-epoch detections are separated by 4.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:06.19 +64:26:26.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:28:06.19 +64:26:26.5: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:28:06.19 +64:26:26.5: 15.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461211.9189,14.90,0.05,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 20260620.4189 14.90CV 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 20.4189 2461211.9189 13.51 00:29:27.82 +60:49:56.1
120.25615 -1.92528 galactic Cas Second-epoch detections are separated by 1.1" and 6.4 pix
The object was found in VSX 8" NSVS J0029273+604956
Type: M
# Max. Min./Amp. JD0 Period
16.607 g Y 2.044 g 2458522.52250 258.863730600000 M6.5
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:29:27.82 +60:49:56.1: 15.84 +/- 0.31 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:29:27.82 +60:49:56.1: 15.95 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.84 +/- 0.31
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 20.4189* 00 29 27.82 +60 49 56.1 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0029273+604956,2461211.9189,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0029273+604956 20260620.4189 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 10.89 23:29:21.47 +63:22:22.0
113.88779 1.95149 galactic Cas Second-epoch detections are separated by 4.0" and 7.1 pix
The object was found in VSX23" Gaia DR3 2016626822113759744
Type:
# Max. Min./Amp. JD0 Period
17.650 G 17.850 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:29:21.47 +63:22:22.0: 16.01 +/- 0.36 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:29:21.47 +63:22:22.0: 15.99 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 16.01 +/- 0.36
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 29 21.47 +63 22 22.0 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 2016626822113759744,2461211.9189,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2016626822113759744 20260620.4189 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 12.57 00:07:40.74 +64:42:27.6
118.27776 2.23208 galactic Cas Second-epoch detections are separated by 4.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:07:40.74 +64:42:27.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:07:40.74 +64:42:27.6: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:07:40.74 +64:42:27.6: 15.92 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 00 07 40.74 +64 42 27.6 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9189,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4189 12.57CV 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 20.4189 2461211.9189 13.32 23:58:36.89 +58:25:46.5
116.04801 -3.73438 galactic Cas Second-epoch detections are separated by 2.7" and 6.7 pix
The object was found in VSX 7" 2MASS J23583604+5825441
Type: SR
# Max. Min./Amp. JD0 Period
13.282 r Y 0.957 r 2458284.44080 313.397654500000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:58:36.89 +58:25:46.5: 14.40 +/- 0.07 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:58:36.89 +58:25:46.5: 14.52 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.45 +/- 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 20.4189* 23 58 36.89 +58 25 46.5 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
2MASS J23583604+5825441,2461211.9189,13.32,0.05,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
2MASS J23583604+5825441 20260620.4189 13.32CV 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 20.4189 2461211.9189 12.85 23:51:07.26 +62:08:50.7
115.95070 0.09601 galactic Cas Second-epoch detections are separated by 5.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2012974343265756928 | 23:51:07.09 +62:08:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:51:07.26 +62:08:50.7: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:51:07.26 +62:08:50.7: 15.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4189* 23 51 07.26 +62 08 50.7 12.8 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 2012974343265756928,2461211.9189,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2012974343265756928 20260620.4189 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4189 2461211.9189 13.47 23:29:38.03 +64:59:16.0
114.42056 3.47660 galactic Cep Second-epoch detections are separated by 4.8" and 7.2 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 | 23:29:38.03 +64:59:16.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:29:38.03 +64:59:16.0: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:29:38.03 +64:59:16.0: 15.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461211.9189,13.47,0.05,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 20260620.4189 13.47CV 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 20.4189 2461211.9189 11.89 00:07:05.62 +61:48:59.6
117.72115 -0.60573 galactic Cas Second-epoch detections are separated by 1.9" and 6.5 pix
The object was found in VSX 4" V0658 Cas
Type: M
# Max. Min./Amp. JD0 Period
11.500 V 14.000 V 224.000000000000 M6.5
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:07:05.62 +61:48:59.6: 13.56 +/- 0.04 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:07:05.62 +61:48:59.6: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 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 20.4189* 00 07 05.62 +61 48 59.6 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0658 Cas,2461211.9189,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0658 Cas 20260620.4189 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.57276170 09.01.2026 01:44:36.611 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
First image: 2461049.57276170 09.01.2026 01:44:36.611 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
Last image: 2461211.91927029 20.06.2026 10:03:34.953 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 32
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
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: 7 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): 26512
Objects passed selection criteria: 26408
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 20688.8
Average stars matched: 18759 (90.6725 %)
Memory usage VmPeak: 127488 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jun 20 06:36:13 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: 2461049.57276170 09.01.2026 01:44:36.611 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
First image: 2461049.57276170 09.01.2026 01:44:36.611 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
Last image: 2461211.91927029 20.06.2026 10:03:34.953 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 520
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
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: 264 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): 204944
Objects passed selection criteria: 204247
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 163311
Average stars matched: 149470 (91.5249 %)
Memory usage VmPeak: 2002660 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jun 20 07:12:08 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-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
SExtractor catalog cache: saved Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.cat to cache
SExtractor catalog cache: saved Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.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-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.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: 2461211.91855711
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits exists and is non-empty
Saving wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits to local_wcs_cache/
'wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits' -> 'local_wcs_cache/wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits'
wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits exists and is non-empty
Saving wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits to local_wcs_cache/
'wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits' -> 'local_wcs_cache/wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits'
wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits exists and is non-empty
Saving wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits to local_wcs_cache/
'wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits' -> 'local_wcs_cache/wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits'
wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits exists and is non-empty
Saving wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits to local_wcs_cache/
'wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits' -> 'local_wcs_cache/wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits (1st reference image)
verification OK: wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
Image size: 943.5'x628.6' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 23:59:58.941 +61:59:19.93 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits (1st new image)
verification OK: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
Image size: 941.2'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:06.783 +61:59:56.88 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:58.941 +61:59:19.93
Second-epoch image center 00:00:06.783 +61:59:56.88
Angular distance between the image centers 0.0185 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits (2nd new image)
verification OK: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
Image size: 941.2'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:05.654 +62:00:35.74 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:58.941 +61:59:19.93
Second-epoch image center 00:00:05.654 +62:00:35.74
Angular distance between the image centers 0.0248 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 00:00:06.783 +61:59:56.88
Second-epoch second image center 00:00:05.654 +62:00:35.74
Angular distance between the image centers 0.01102 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-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits &> /tmp/tmp.5Etq7NrxWD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits &> /tmp/tmp.iZ25rHgfpR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits &> /tmp/tmp.jUKYYznrqr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits &> /tmp/tmp.Rd9R1LeLWT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.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-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits and wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits and wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat
Found non-empty wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits and wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat
The reference image (wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits) and catalog (wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat) found
'wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat' -> 'wcsmag.cat'
Read 28928 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9986 deg, Dec +55.3299 to +67.4085 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0003 to 359.9986 deg, Dec 55.3299 to 67.4085 deg
Loaded 133379 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): 1544 out of 1735 total matches.
Matched with Tycho-2 1735 out of 28928 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.943100
a=0.000000 b=1.000000 c=22.943100
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.24
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.24
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 28928 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9986 deg, Dec +55.3299 to +67.4085 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0003 to 359.9986 deg, Dec 55.3299 to 67.4085 deg
Loaded 133379 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): 1544 out of 1735 total matches.
Matched with Tycho-2 1735 out of 28928 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits:
Forced-photometry filter: calibrated wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits -> calib.txt_param_ref_wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits (aperture=5.8)
Read 30191 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9985 deg, Dec +55.2732 to +67.4066 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0001 to 359.9985 deg, Dec 55.2732 to 67.4066 deg
Loaded 134187 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): 2225 out of 2505 total matches.
Matched with Tycho-2 2505 out of 30191 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits:
Forced-photometry filter: calibrated wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits -> calib.txt_param_ref_wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 31 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
2.1 pix Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits
2.4 pix fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
2.4 pix fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
2.0 pix wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
2.1 pix wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits
Limiting magnitude estimates:
15.2 mag. Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
15.2 mag. Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits
15.0 mag. fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
15.0 mag. fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (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.5Etq7NrxWD (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-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.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_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.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-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.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-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits' -> 'wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
Checking if the catalog wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat corresponding to the image wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat corresponding to the image wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits
WCS catalog name: wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3732, passed=28928
Got 28928 stars (including 25166 good ones) from the SExtractor catalog wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat
util/solve_plate_with_UCAC5 got 28928 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.5'
Seting catalog search parameters based on the expected field of view 943.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013104 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010483 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 341.1650 through 0 to 19.9061, gap 19.9061 to 341.1650
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 26071 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 341.1694 through 0 to 19.9054, gap 19.9054 to 341.1694
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 26086 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.47"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 26929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.29"
Excluding outliers - 968 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits N_match=968 sigma_overall_arcsec=2.004 sigma_q1_arcsec=1.709 sigma_q2_arcsec=1.480 sigma_q3_arcsec=1.550 sigma_q4_arcsec=1.402 n_q1=148 n_q2=275 n_q3=232 n_q4=313 worst_quadrant_to_overall_ratio=0.853
The image catalog is written to wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits -region wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.iZ25rHgfpR (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-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.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_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.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-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.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-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits' -> 'wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits
WCS-calibrated image found: wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits
Checking if the catalog wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits.wcscat corresponding to the image wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits.wcscat corresponding to the image wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits
WCS catalog name: wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3591, passed=30191
Got 30191 stars (including 26565 good ones) from the SExtractor catalog wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits.wcscat
util/solve_plate_with_UCAC5 got 30191 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.6'
Seting catalog search parameters based on the expected field of view 943.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013106 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010484 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 341.1617 through 0 to 20.0679, gap 20.0679 to 341.1617
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 27209 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 341.1679 through 0 to 20.0647, gap 20.0647 to 341.1679
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 27226 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.53"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 28091 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.24"
Excluding outliers - 963 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits N_match=963 sigma_overall_arcsec=1.992 sigma_q1_arcsec=1.731 sigma_q2_arcsec=1.562 sigma_q3_arcsec=1.318 sigma_q4_arcsec=1.469 n_q1=158 n_q2=270 n_q3=234 n_q4=301 worst_quadrant_to_overall_ratio=0.869
The image catalog is written to wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits -region wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.jUKYYznrqr (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_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.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_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
WCS-calibrated image found: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
Checking if the catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
WCS catalog name: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2451, passed=25423
Got 25423 stars (including 22962 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat
util/solve_plate_with_UCAC5 got 25423 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
RA wraps around 0/360 boundary: field RA 340.5593 through 0 to 19.2943, gap 19.2943 to 340.5593
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 572 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 486 matched stars entering correct_measured_positions(), 447 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 463 matched stars entering correct_measured_positions(), 14531 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 340.5680 through 0 to 19.3179, gap 19.3179 to 340.5680
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 675 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 629 matched stars entering correct_measured_positions(), 14608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.32"
Accuracy estimation diagnostic: 629 matched stars entering correct_measured_positions(), 17741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.19"
Excluding outliers - 629 stars left (next iteration limit 509)
WCS_QUALITY_DIAG: file=fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits N_match=629 sigma_overall_arcsec=5.071 sigma_q1_arcsec=10.021 sigma_q2_arcsec=2.509 sigma_q3_arcsec=17.361 sigma_q4_arcsec=5.441 n_q1=158 n_q2=295 n_q3=71 n_q4=105 worst_quadrant_to_overall_ratio=3.423
The image catalog is written to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits -region wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Rd9R1LeLWT (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_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.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_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
WCS-calibrated image found: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
Checking if the catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
WCS catalog name: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2435, passed=25376
Got 25376 stars (including 22925 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat
util/solve_plate_with_UCAC5 got 25376 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
RA wraps around 0/360 boundary: field RA 340.5598 through 0 to 19.2942, gap 19.2942 to 340.5598
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 574 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 487 matched stars entering correct_measured_positions(), 446 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 465 matched stars entering correct_measured_positions(), 14429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 340.5707 through 0 to 19.3202, gap 19.3202 to 340.5707
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 682 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 635 matched stars entering correct_measured_positions(), 14504 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.45"
Accuracy estimation diagnostic: 632 matched stars entering correct_measured_positions(), 17760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.20"
Excluding outliers - 632 stars left (next iteration limit 511)
WCS_QUALITY_DIAG: file=fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits N_match=632 sigma_overall_arcsec=5.022 sigma_q1_arcsec=11.451 sigma_q2_arcsec=2.727 sigma_q3_arcsec=19.675 sigma_q4_arcsec=5.760 n_q1=155 n_q2=300 n_q3=67 n_q4=110 worst_quadrant_to_overall_ratio=3.918
The image catalog is written to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits -region wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits sigma_overall=2.004 worst_q_ratio=0.853
ref2=Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits sigma_overall=1.992 worst_q_ratio=0.869
new1=fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits sigma_overall=5.071 worst_q_ratio=3.423
new2=fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits sigma_overall=5.022 worst_q_ratio=3.918
reference average sigma_overall=1.998 worst_q_ratio=0.861
warn-on-ratio threshold: 2.0x reference
###################################
WCS_QUALITY_RETRY: 1st new image (fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits) flagged: sigma=5.071 (ref avg 1.998), ratio=3.423 (ref avg 0.861), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.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_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/lib/make_outxyls_for_astrometric_calibration found 24343 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out2663776.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2663776.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
log-odds ratio 28.2056 (1.77646e+12), 8 match, 0 conflict, 24 distractors, 105 index.
RA,Dec = (0.106549,61.9865), pixel scale 5.90273 arcsec/pix.
Hit/miss: Hit/miss: -------+---+---+--++---+------++(best)-----------+-------+---+-------------------+---+----------+---------
Field 1: solved with index index-4114.fits.
Field 1 solved: writing to file ./out2663776.solved to indicate this.
Field: out2663776.xyls
Field center: (RA,Dec) = (0.108273, 61.987339) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:25.986, +61:59:14.420).
Field size: 15.3953 x 10.3583 degrees
Field rotation angle: up is 10.9449 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits' -> 'fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits'
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jun 20 06:47 fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
-rw-r--r-- 1 apache apache 8.5K Jun 20 06:47 out2663776.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits for reading... done!
Creating new image file (wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits (fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out2663776.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2663776.axy"...
Only searching for solutions within 15.3933 degrees of RA,Dec (0.109996,61.9882)
log-odds ratio 47.0475 (2.70694e+20), 9 match, 0 conflict, 9 distractors, 29 index.
RA,Dec = (0.0247573,61.9975), pixel scale 5.9484 arcsec/pix.
Hit/miss: Hit/miss: +-++-+-+-+-++----+(best)-----------------------+----------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2663776.solved to indicate this.
Field: out2663776.xyls
Field center: (RA,Dec) = (0.026510, 61.998307) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:06.362, +61:59:53.906).
Field size: 15.7087 x 10.5133 degrees
Field rotation angle: up is -2.38016 degrees E of N
Field parity: neg
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jun 20 06:47 fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
-rw-r--r-- 1 apache apache 8.5K Jun 20 06:47 out2663776.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits for reading... done!
Creating new image file (wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 100000 sources.
Solving...
Reading file "./wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.axy"...
Verifying WCS using indices with quads of size [63.3306, 949.364] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS using indices with quads of size [63.3306, 949.364] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
--> log-odds 0
Got 0 solutions.
Field 1 did not solve (index index-5203-47.fits, field objects 1-10).
Field 1 did not solve (index index-5203-46.fits, field objects 1-10).
Field 1 did not solve (index index-5203-45.fits, field objects 1-10).
Field 1 did not solve (index index-5203-44.fits, field objects 1-10).
Field 1 did not solve (index index-5203-43.fits, field objects 1-10).
Field 1 did not solve (index index-5203-42.fits, field objects 1-10).
Field 1 did not solve (index index-5203-41.fits, field objects 1-10).
Field 1 did not solve (index index-5203-40.fits, field objects 1-10).
Field 1 did not solve (index index-5203-39.fits, field objects 1-10).
Field 1 did not solve (index index-5203-38.fits, field objects 1-10).
Field 1 did not solve (index index-5203-37.fits, field objects 1-10).
Field 1 did not solve (index index-5203-36.fits, field objects 1-10).
Field 1 did not solve (index index-5203-35.fits, field objects 1-10).
Field 1 did not solve (index index-5203-34.fits, field objects 1-10).
Field 1 did not solve (index index-5203-33.fits, field objects 1-10).
Field 1 did not solve (index index-5203-32.fits, field objects 1-10).
Field 1 did not solve (index index-5203-31.fits, field objects 1-10).
Field 1 did not solve (index index-5203-30.fits, field objects 1-10).
Field 1 did not solve (index index-5203-29.fits, field objects 1-10).
Field 1 did not solve (index index-5203-28.fits, field objects 1-10).
Field 1 did not solve (index index-5203-27.fits, field objects 1-10).
Field 1 did not solve (index index-5203-26.fits, field objects 1-10).
Field 1 did not solve (index index-5203-25.fits, field objects 1-10).
Field 1 did not solve (index index-5203-24.fits, field objects 1-10).
Field 1 did not solve (index index-5203-23.fits, field objects 1-10).
Field 1 did not solve (index index-5203-22.fits, field objects 1-10).
Field 1 did not solve (index index-5203-21.fits, field objects 1-10).
Field 1 did not solve (index index-5203-20.fits, field objects 1-10).
Field 1 did not solve (index index-5203-19.fits, field objects 1-10).
Field 1 did not solve (index index-5203-18.fits, field objects 1-10).
Field 1 did not solve (index index-5203-17.fits, field objects 1-10).
Field 1 did not solve (index index-5203-16.fits, field objects 1-10).
Field 1 did not solve (index index-5203-15.fits, field objects 1-10).
Field 1 did not solve (index index-5203-14.fits, field objects 1-10).
Field 1 did not solve (index index-5203-13.fits, field objects 1-10).
Field 1 did not solve (index index-5203-12.fits, field objects 1-10).
Field 1 did not solve (index index-5203-11.fits, field objects 1-10).
Field 1 did not solve (index index-5203-10.fits, field objects 1-10).
Field 1 did not solve (index index-5203-09.fits, field objects 1-10).
Field 1 did not solve (index index-5203-08.fits, field objects 1-10).
Field 1 did not solve (index index-5203-07.fits, field objects 1-10).
Field 1 did not solve (index index-5203-06.fits, field objects 1-10).
Field 1 did not solve (index index-5203-05.fits, field objects 1-10).
Field 1 did not solve (index index-5203-04.fits, field objects 1-10).
Field 1 did not solve (index index-5203-03.fits, field objects 1-10).
Field 1 did not solve (index index-5203-02.fits, field objects 1-10).
Field 1 did not solve (index index-5203-01.fits, field objects 1-10).
Field 1 did not solve (index index-5203-00.fits, field objects 1-10).
Field 1 did not solve (index index-5005-11.fits, field objects 1-10).
Field 1 did not solve (index index-5005-10.fits, field objects 1-10).
Field 1 did not solve (index index-5005-09.fits, field objects 1-10).
Field 1 did not solve (index index-5005-08.fits, field objects 1-10).
Field 1 did not solve (index index-5005-07.fits, field objects 1-10).
Field 1 did not solve (index index-5005-06.fits, field objects 1-10).
Field 1 did not solve (index index-5005-05.fits, field objects 1-10).
Field 1 did not solve (index index-5005-04.fits, field objects 1-10).
Field 1 did not solve (index index-5005-03.fits, field objects 1-10).
Field 1 did not solve (index index-5005-02.fits, field objects 1-10).
Field 1 did not solve (index index-5005-01.fits, field objects 1-10).
Field 1 did not solve (index index-5005-00.fits, field objects 1-10).
Field 1 did not solve (index index-4206-11.fits, field objects 1-10).
Field 1 did not solve (index index-4206-10.fits, field objects 1-10).
Field 1 did not solve (index index-4206-09.fits, field objects 1-10).
Field 1 did not solve (index index-4206-08.fits, field objects 1-10).
Field 1 did not solve (index index-4206-07.fits, field objects 1-10).
Field 1 did not solve (index index-4206-06.fits, field objects 1-10).
Field 1 did not solve (index index-4206-05.fits, field objects 1-10).
Field 1 did not solve (index index-4206-04.fits, field objects 1-10).
Field 1 did not solve (index index-4206-03.fits, field objects 1-10).
Field 1 did not solve (index index-4206-02.fits, field objects 1-10).
Field 1 did not solve (index index-4206-01.fits, field objects 1-10).
Field 1 did not solve (index index-4206-00.fits, field objects 1-10).
Field 1 did not solve (index index-4205-11.fits, field objects 1-10).
Field 1 did not solve (index index-4205-10.fits, field objects 1-10).
Field 1 did not solve (index index-4205-09.fits, field objects 1-10).
Field 1 did not solve (index index-4205-08.fits, field objects 1-10).
Field 1 did not solve (index index-4205-07.fits, field objects 1-10).
Field 1 did not solve (index index-4205-06.fits, field objects 1-10).
Field 1 did not solve (index index-4205-05.fits, field objects 1-10).
Field 1 did not solve (index index-4205-04.fits, field objects 1-10).
Field 1 did not solve (index index-4205-03.fits, field objects 1-10).
Field 1 did not solve (index index-4205-02.fits, field objects 1-10).
Field 1 did not solve (index index-4205-01.fits, field objects 1-10).
Field 1 did not solve (index index-4205-00.fits, field objects 1-10).
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
Field 1 did not solve (index index-4113.fits, field objects 1-10).
Field 1 did not solve (index index-4112.fits, field objects 1-10).
Field 1 did not solve (index index-4111.fits, field objects 1-10).
Field 1 did not solve (index index-4110.fits, field objects 1-10).
Field 1 did not solve (index index-4109.fits, field objects 1-10).
Field 1 did not solve (index index-4108.fits, field objects 1-10).
Field 1 did not solve (index index-4107.fits, field objects 1-10).
Field 1 did not solve (index index-204-11.fits, field objects 1-10).
Field 1 did not solve (index index-204-10.fits, field objects 1-10).
Field 1 did not solve (index index-204-09.fits, field objects 1-10).
Field 1 did not solve (index index-204-08.fits, field objects 1-10).
Field 1 did not solve (index index-204-07.fits, field objects 1-10).
Field 1 did not solve (index index-204-06.fits, field objects 1-10).
Field 1 did not solve (index index-204-05.fits, field objects 1-10).
Field 1 did not solve (index index-204-04.fits, field objects 1-10).
Field 1 did not solve (index index-204-03.fits, field objects 1-10).
Field 1 did not solve (index index-204-02.fits, field objects 1-10).
Field 1 did not solve (index index-204-01.fits, field objects 1-10).
Field 1 did not solve (index index-204-00.fits, field objects 1-10).
Field 1 did not solve (index index-5203-47.fits, field objects 11-20).
Field 1 did not solve (index index-5203-46.fits, field objects 11-20).
Field 1 did not solve (index index-5203-45.fits, field objects 11-20).
Field 1 did not solve (index index-5203-44.fits, field objects 11-20).
Field 1 did not solve (index index-5203-43.fits, field objects 11-20).
Field 1 did not solve (index index-5203-42.fits, field objects 11-20).
Field 1 did not solve (index index-5203-41.fits, field objects 11-20).
Field 1 did not solve (index index-5203-40.fits, field objects 11-20).
Field 1 did not solve (index index-5203-39.fits, field objects 11-20).
Field 1 did not solve (index index-5203-38.fits, field objects 11-20).
Field 1 did not solve (index index-5203-37.fits, field objects 11-20).
Field 1 did not solve (index index-5203-36.fits, field objects 11-20).
Field 1 did not solve (index index-5203-35.fits, field objects 11-20).
Field 1 did not solve (index index-5203-34.fits, field objects 11-20).
Field 1 did not solve (index index-5203-33.fits, field objects 11-20).
Field 1 did not solve (index index-5203-32.fits, field objects 11-20).
Field 1 did not solve (index index-5203-31.fits, field objects 11-20).
Field 1 did not solve (index index-5203-30.fits, field objects 11-20).
Field 1 did not solve (index index-5203-29.fits, field objects 11-20).
Field 1 did not solve (index index-5203-28.fits, field objects 11-20).
Field 1 did not solve (index index-5203-27.fits, field objects 11-20).
Field 1 did not solve (index index-5203-26.fits, field objects 11-20).
Field 1 did not solve (index index-5203-25.fits, field objects 11-20).
Field 1 did not solve (index index-5203-24.fits, field objects 11-20).
Field 1 did not solve (index index-5203-23.fits, field objects 11-20).
Field 1 did not solve (index index-5203-22.fits, field objects 11-20).
Field 1 did not solve (index index-5203-21.fits, field objects 11-20).
Field 1 did not solve (index index-5203-20.fits, field objects 11-20).
Field 1 did not solve (index index-5203-19.fits, field objects 11-20).
Field 1 did not solve (index index-5203-18.fits, field objects 11-20).
Field 1 did not solve (index index-5203-17.fits, field objects 11-20).
Field 1 did not solve (index index-5203-16.fits, field objects 11-20).
Field 1 did not solve (index index-5203-15.fits, field objects 11-20).
Field 1 did not solve (index index-5203-14.fits, field objects 11-20).
Field 1 did not solve (index index-5203-13.fits, field objects 11-20).
Field 1 did not solve (index index-5203-12.fits, field objects 11-20).
Field 1 did not solve (index index-5203-11.fits, field objects 11-20).
Field 1 did not solve (index index-5203-10.fits, field objects 11-20).
Field 1 did not solve (index index-5203-09.fits, field objects 11-20).
Field 1 did not solve (index index-5203-08.fits, field objects 11-20).
Field 1 did not solve (index index-5203-07.fits, field objects 11-20).
Field 1 did not solve (index index-5203-06.fits, field objects 11-20).
Field 1 did not solve (index index-5203-05.fits, field objects 11-20).
Field 1 did not solve (index index-5203-04.fits, field objects 11-20).
Field 1 did not solve (index index-5203-03.fits, field objects 11-20).
Field 1 did not solve (index index-5203-02.fits, field objects 11-20).
Field 1 did not solve (index index-5203-01.fits, field objects 11-20).
Field 1 did not solve (index index-5203-00.fits, field objects 11-20).
Field 1 did not solve (index index-5005-11.fits, field objects 11-20).
Field 1 did not solve (index index-5005-10.fits, field objects 11-20).
Field 1 did not solve (index index-5005-09.fits, field objects 11-20).
Field 1 did not solve (index index-5005-08.fits, field objects 11-20).
Field 1 did not solve (index index-5005-07.fits, field objects 11-20).
Field 1 did not solve (index index-5005-06.fits, field objects 11-20).
Field 1 did not solve (index index-5005-05.fits, field objects 11-20).
Field 1 did not solve (index index-5005-04.fits, field objects 11-20).
Field 1 did not solve (index index-5005-03.fits, field objects 11-20).
Field 1 did not solve (index index-5005-02.fits, field objects 11-20).
Field 1 did not solve (index index-5005-01.fits, field objects 11-20).
Field 1 did not solve (index index-5005-00.fits, field objects 11-20).
Field 1 did not solve (index index-4206-11.fits, field objects 11-20).
Field 1 did not solve (index index-4206-10.fits, field objects 11-20).
Field 1 did not solve (index index-4206-09.fits, field objects 11-20).
Field 1 did not solve (index index-4206-08.fits, field objects 11-20).
Field 1 did not solve (index index-4206-07.fits, field objects 11-20).
Field 1 did not solve (index index-4206-06.fits, field objects 11-20).
Field 1 did not solve (index index-4206-05.fits, field objects 11-20).
Field 1 did not solve (index index-4206-04.fits, field objects 11-20).
Field 1 did not solve (index index-4206-03.fits, field objects 11-20).
Field 1 did not solve (index index-4206-02.fits, field objects 11-20).
Field 1 did not solve (index index-4206-01.fits, field objects 11-20).
Field 1 did not solve (index index-4206-00.fits, field objects 11-20).
Field 1 did not solve (index index-4205-11.fits, field objects 11-20).
Field 1 did not solve (index index-4205-10.fits, field objects 11-20).
Field 1 did not solve (index index-4205-09.fits, field objects 11-20).
Field 1 did not solve (index index-4205-08.fits, field objects 11-20).
Field 1 did not solve (index index-4205-07.fits, field objects 11-20).
Field 1 did not solve (index index-4205-06.fits, field objects 11-20).
Field 1 did not solve (index index-4205-05.fits, field objects 11-20).
Field 1 did not solve (index index-4205-04.fits, field objects 11-20).
Field 1 did not solve (index index-4205-03.fits, field objects 11-20).
Field 1 did not solve (index index-4205-02.fits, field objects 11-20).
Field 1 did not solve (index index-4205-01.fits, field objects 11-20).
Field 1 did not solve (index index-4205-00.fits, field objects 11-20).
Field 1 did not solve (index index-4119.fits, field objects 11-20).
Field 1 did not solve (index index-4118.fits, field objects 11-20).
Field 1 did not solve (index index-4117.fits, field objects 11-20).
Field 1 did not solve (index index-4116.fits, field objects 11-20).
Field 1 did not solve (index index-4115.fits, field objects 11-20).
Field 1 did not solve (index index-4114.fits, field objects 11-20).
Field 1 did not solve (index index-4113.fits, field objects 11-20).
Field 1 did not solve (index index-4112.fits, field objects 11-20).
Field 1 did not solve (index index-4111.fits, field objects 11-20).
Field 1 did not solve (index index-4110.fits, field objects 11-20).
Field 1 did not solve (index index-4109.fits, field objects 11-20).
Field 1 did not solve (index index-4108.fits, field objects 11-20).
Field 1 did not solve (index index-4107.fits, field objects 11-20).
Field 1 did not solve (index index-204-11.fits, field objects 11-20).
Field 1 did not solve (index index-204-10.fits, field objects 11-20).
Field 1 did not solve (index index-204-09.fits, field objects 11-20).
Field 1 did not solve (index index-204-08.fits, field objects 11-20).
Field 1 did not solve (index index-204-07.fits, field objects 11-20).
Field 1 did not solve (index index-204-06.fits, field objects 11-20).
Field 1 did not solve (index index-204-05.fits, field objects 11-20).
Field 1 did not solve (index index-204-04.fits, field objects 11-20).
Field 1 did not solve (index index-204-03.fits, field objects 11-20).
Field 1 did not solve (index index-204-02.fits, field objects 11-20).
Field 1 did not solve (index index-204-01.fits, field objects 11-20).
Field 1 did not solve (index index-204-00.fits, field objects 11-20).
Field 1 did not solve (index index-5203-47.fits, field objects 21-30).
Field 1 did not solve (index index-5203-46.fits, field objects 21-30).
Field 1 did not solve (index index-5203-45.fits, field objects 21-30).
Field 1 did not solve (index index-5203-44.fits, field objects 21-30).
Field 1 did not solve (index index-5203-43.fits, field objects 21-30).
Field 1 did not solve (index index-5203-42.fits, field objects 21-30).
Field 1 did not solve (index index-5203-41.fits, field objects 21-30).
Field 1 did not solve (index index-5203-40.fits, field objects 21-30).
Field 1 did not solve (index index-5203-39.fits, field objects 21-30).
Field 1 did not solve (index index-5203-38.fits, field objects 21-30).
Field 1 did not solve (index index-5203-37.fits, field objects 21-30).
Field 1 did not solve (index index-5203-36.fits, field objects 21-30).
Field 1 did not solve (index index-5203-35.fits, field objects 21-30).
Field 1 did not solve (index index-5203-34.fits, field objects 21-30).
Field 1 did not solve (index index-5203-33.fits, field objects 21-30).
Field 1 did not solve (index index-5203-32.fits, field objects 21-30).
Field 1 did not solve (index index-5203-31.fits, field objects 21-30).
Field 1 did not solve (index index-5203-30.fits, field objects 21-30).
Field 1 did not solve (index index-5203-29.fits, field objects 21-30).
Field 1 did not solve (index index-5203-28.fits, field objects 21-30).
Field 1 did not solve (index index-5203-27.fits, field objects 21-30).
Field 1 did not solve (index index-5203-26.fits, field objects 21-30).
Field 1 did not solve (index index-5203-25.fits, field objects 21-30).
Field 1 did not solve (index index-5203-24.fits, field objects 21-30).
Field 1 did not solve (index index-5203-23.fits, field objects 21-30).
Field 1 did not solve (index index-5203-22.fits, field objects 21-30).
Field 1 did not solve (index index-5203-21.fits, field objects 21-30).
Field 1 did not solve (index index-5203-20.fits, field objects 21-30).
Field 1 did not solve (index index-5203-19.fits, field objects 21-30).
Field 1 did not solve (index index-5203-18.fits, field objects 21-30).
Field 1 did not solve (index index-5203-17.fits, field objects 21-30).
Field 1 did not solve (index index-5203-16.fits, field objects 21-30).
Field 1 did not solve (index index-5203-15.fits, field objects 21-30).
Field 1 did not solve (index index-5203-14.fits, field objects 21-30).
Field 1 did not solve (index index-5203-13.fits, field objects 21-30).
Field 1 did not solve (index index-5203-12.fits, field objects 21-30).
Field 1 did not solve (index index-5203-11.fits, field objects 21-30).
Field 1 did not solve (index index-5203-10.fits, field objects 21-30).
Field 1 did not solve (index index-5203-09.fits, field objects 21-30).
Field 1 did not solve (index index-5203-08.fits, field objects 21-30).
Field 1 did not solve (index index-5203-07.fits, field objects 21-30).
Field 1 did not solve (index index-5203-06.fits, field objects 21-30).
Field 1 did not solve (index index-5203-05.fits, field objects 21-30).
Field 1 did not solve (index index-5203-04.fits, field objects 21-30).
Field 1 did not solve (index index-5203-03.fits, field objects 21-30).
Field 1 did not solve (index index-5203-02.fits, field objects 21-30).
Field 1 did not solve (index index-5203-01.fits, field objects 21-30).
Field 1 did not solve (index index-5203-00.fits, field objects 21-30).
Field 1 did not solve (index index-5005-11.fits, field objects 21-30).
Field 1 did not solve (index index-5005-10.fits, field objects 21-30).
Field 1 did not solve (index index-5005-09.fits, field objects 21-30).
Field 1 did not solve (index index-5005-08.fits, field objects 21-30).
Field 1 did not solve (index index-5005-07.fits, field objects 21-30).
Field 1 did not solve (index index-5005-06.fits, field objects 21-30).
Field 1 did not solve (index index-5005-05.fits, field objects 21-30).
Field 1 did not solve (index index-5005-04.fits, field objects 21-30).
Field 1 did not solve (index index-5005-03.fits, field objects 21-30).
Field 1 did not solve (index index-5005-02.fits, field objects 21-30).
Field 1 did not solve (index index-5005-01.fits, field objects 21-30).
Field 1 did not solve (index index-5005-00.fits, field objects 21-30).
Field 1 did not solve (index index-4206-11.fits, field objects 21-30).
Field 1 did not solve (index index-4206-10.fits, field objects 21-30).
Field 1 did not solve (index index-4206-09.fits, field objects 21-30).
Field 1 did not solve (index index-4206-08.fits, field objects 21-30).
Field 1 did not solve (index index-4206-07.fits, field objects 21-30).
Field 1 did not solve (index index-4206-06.fits, field objects 21-30).
Field 1 did not solve (index index-4206-05.fits, field objects 21-30).
Field 1 did not solve (index index-4206-04.fits, field objects 21-30).
Field 1 did not solve (index index-4206-03.fits, field objects 21-30).
Field 1 did not solve (index index-4206-02.fits, field objects 21-30).
Field 1 did not solve (index index-4206-01.fits, field objects 21-30).
Field 1 did not solve (index index-4206-00.fits, field objects 21-30).
Field 1 did not solve (index index-4205-11.fits, field objects 21-30).
Field 1 did not solve (index index-4205-10.fits, field objects 21-30).
Field 1 did not solve (index index-4205-09.fits, field objects 21-30).
Field 1 did not solve (index index-4205-08.fits, field objects 21-30).
Field 1 did not solve (index index-4205-07.fits, field objects 21-30).
Field 1 did not solve (index index-4205-06.fits, field objects 21-30).
Field 1 did not solve (index index-4205-05.fits, field objects 21-30).
Field 1 did not solve (index index-4205-04.fits, field objects 21-30).
Field 1 did not solve (index index-4205-03.fits, field objects 21-30).
Field 1 did not solve (index index-4205-02.fits, field objects 21-30).
Field 1 did not solve (index index-4205-01.fits, field objects 21-30).
Field 1 did not solve (index index-4205-00.fits, field objects 21-30).
Field 1 did not solve (index index-4119.fits, field objects 21-30).
Field 1 did not solve (index index-4118.fits, field objects 21-30).
Field 1 did not solve (index index-4117.fits, field objects 21-30).
Field 1 did not solve (index index-4116.fits, field objects 21-30).
Field 1 did not solve (index index-4115.fits, field objects 21-30).
Field 1 did not solve (index index-4114.fits, field objects 21-30).
Field 1 did not solve (index index-4113.fits, field objects 21-30).
Total CPU time limit reached!
Field 1 did not solve (index index-4112.fits, field objects 21-30).
Field: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
Did not solve (or no WCS file was written).
Checking if the catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
verification OK: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
Generating wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat from image00003.cat
Catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits created.
verification OK: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
verification OK: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
Image size: 941.2'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:06.783 +61:59:56.88 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 25423 stars ###
'wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/correct_sextractor_wcs_catalog_usingxy2sky3676692.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
WCS catalog name: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2451, passed=25423
Got 25423 stars (including 22962 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat
util/solve_plate_with_UCAC5 got 25423 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
RA wraps around 0/360 boundary: field RA 340.5593 through 0 to 19.2943, gap 19.2943 to 340.5593
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 572 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 486 matched stars entering correct_measured_positions(), 447 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 463 matched stars entering correct_measured_positions(), 14531 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 340.5680 through 0 to 19.3179, gap 19.3179 to 340.5680
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 675 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 629 matched stars entering correct_measured_positions(), 14608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.32"
Accuracy estimation diagnostic: 629 matched stars entering correct_measured_positions(), 17741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.19"
Excluding outliers - 629 stars left (next iteration limit 509)
WCS_QUALITY_DIAG: file=fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits N_match=629 sigma_overall_arcsec=5.071 sigma_q1_arcsec=10.021 sigma_q2_arcsec=2.509 sigma_q3_arcsec=17.361 sigma_q4_arcsec=5.441 n_q1=158 n_q2=295 n_q3=71 n_q4=105 worst_quadrant_to_overall_ratio=3.423
The image catalog is written to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits -region wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 1st new image (fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits): sigma 5.071->5.071, ratio 3.423->3.423; reverting to order 3
WCS_QUALITY_RETRY: 2nd new image (fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits) flagged: sigma=5.022 (ref avg 1.998), ratio=3.918 (ref avg 0.861), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.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_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/lib/make_outxyls_for_astrometric_calibration found 24314 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out3677742.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3677742.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
log-odds ratio 28.3964 (2.14974e+12), 8 match, 0 conflict, 24 distractors, 105 index.
RA,Dec = (0.101993,61.9972), pixel scale 5.90262 arcsec/pix.
Hit/miss: Hit/miss: ---+---+---+------++---+------++(best)-----------+-------+---+-----------------------+-------+--+---------
Field 1: solved with index index-4114.fits.
Field 1 solved: writing to file ./out3677742.solved to indicate this.
Field: out3677742.xyls
Field center: (RA,Dec) = (359.996923, 62.008819) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:59.262, +62:00:31.749).
Field size: 15.7279 x 10.5315 degrees
Field rotation angle: up is -0.191653 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits' -> 'fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits'
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jun 20 06:56 fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
-rw-r--r-- 1 apache apache 12K Jun 20 06:56 out3677742.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits for reading... done!
Creating new image file (wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits (fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out3677742.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3677742.axy"...
Only searching for solutions within 15.6583 degrees of RA,Dec (359.999,62.0096)
log-odds ratio 46.9785 (2.52642e+20), 9 match, 0 conflict, 9 distractors, 29 index.
RA,Dec = (0.0200519,62.0083), pixel scale 5.94841 arcsec/pix.
Hit/miss: Hit/miss: +++--+-+-+-+--+--+(best)-----------------------+----------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out3677742.solved to indicate this.
Field: out3677742.xyls
Field center: (RA,Dec) = (0.021806, 62.009102) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:05.233, +62:00:32.768).
Field size: 15.7087 x 10.5132 degrees
Field rotation angle: up is -2.36753 degrees E of N
Field parity: neg
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jun 20 06:56 fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
-rw-r--r-- 1 apache apache 8.5K Jun 20 06:56 out3677742.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits for reading... done!
Creating new image file (wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 100000 sources.
Solving...
Reading file "./wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.axy"...
Verifying WCS using indices with quads of size [63.3307, 949.366] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS using indices with quads of size [63.3307, 949.366] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
--> log-odds 0
Got 0 solutions.
Field 1 did not solve (index index-5203-47.fits, field objects 1-10).
Field 1 did not solve (index index-5203-46.fits, field objects 1-10).
Field 1 did not solve (index index-5203-45.fits, field objects 1-10).
Field 1 did not solve (index index-5203-44.fits, field objects 1-10).
Field 1 did not solve (index index-5203-43.fits, field objects 1-10).
Field 1 did not solve (index index-5203-42.fits, field objects 1-10).
Field 1 did not solve (index index-5203-41.fits, field objects 1-10).
Field 1 did not solve (index index-5203-40.fits, field objects 1-10).
Field 1 did not solve (index index-5203-39.fits, field objects 1-10).
Field 1 did not solve (index index-5203-38.fits, field objects 1-10).
Field 1 did not solve (index index-5203-37.fits, field objects 1-10).
Field 1 did not solve (index index-5203-36.fits, field objects 1-10).
Field 1 did not solve (index index-5203-35.fits, field objects 1-10).
Field 1 did not solve (index index-5203-34.fits, field objects 1-10).
Field 1 did not solve (index index-5203-33.fits, field objects 1-10).
Field 1 did not solve (index index-5203-32.fits, field objects 1-10).
Field 1 did not solve (index index-5203-31.fits, field objects 1-10).
Field 1 did not solve (index index-5203-30.fits, field objects 1-10).
Field 1 did not solve (index index-5203-29.fits, field objects 1-10).
Field 1 did not solve (index index-5203-28.fits, field objects 1-10).
Field 1 did not solve (index index-5203-27.fits, field objects 1-10).
Field 1 did not solve (index index-5203-26.fits, field objects 1-10).
Field 1 did not solve (index index-5203-25.fits, field objects 1-10).
Field 1 did not solve (index index-5203-24.fits, field objects 1-10).
Field 1 did not solve (index index-5203-23.fits, field objects 1-10).
Field 1 did not solve (index index-5203-22.fits, field objects 1-10).
Field 1 did not solve (index index-5203-21.fits, field objects 1-10).
Field 1 did not solve (index index-5203-20.fits, field objects 1-10).
Field 1 did not solve (index index-5203-19.fits, field objects 1-10).
Field 1 did not solve (index index-5203-18.fits, field objects 1-10).
Field 1 did not solve (index index-5203-17.fits, field objects 1-10).
Field 1 did not solve (index index-5203-16.fits, field objects 1-10).
Field 1 did not solve (index index-5203-15.fits, field objects 1-10).
Field 1 did not solve (index index-5203-14.fits, field objects 1-10).
Field 1 did not solve (index index-5203-13.fits, field objects 1-10).
Field 1 did not solve (index index-5203-12.fits, field objects 1-10).
Field 1 did not solve (index index-5203-11.fits, field objects 1-10).
Field 1 did not solve (index index-5203-10.fits, field objects 1-10).
Field 1 did not solve (index index-5203-09.fits, field objects 1-10).
Field 1 did not solve (index index-5203-08.fits, field objects 1-10).
Field 1 did not solve (index index-5203-07.fits, field objects 1-10).
Field 1 did not solve (index index-5203-06.fits, field objects 1-10).
Field 1 did not solve (index index-5203-05.fits, field objects 1-10).
Field 1 did not solve (index index-5203-04.fits, field objects 1-10).
Field 1 did not solve (index index-5203-03.fits, field objects 1-10).
Field 1 did not solve (index index-5203-02.fits, field objects 1-10).
Field 1 did not solve (index index-5203-01.fits, field objects 1-10).
Field 1 did not solve (index index-5203-00.fits, field objects 1-10).
Field 1 did not solve (index index-5005-11.fits, field objects 1-10).
Field 1 did not solve (index index-5005-10.fits, field objects 1-10).
Field 1 did not solve (index index-5005-09.fits, field objects 1-10).
Field 1 did not solve (index index-5005-08.fits, field objects 1-10).
Field 1 did not solve (index index-5005-07.fits, field objects 1-10).
Field 1 did not solve (index index-5005-06.fits, field objects 1-10).
Field 1 did not solve (index index-5005-05.fits, field objects 1-10).
Field 1 did not solve (index index-5005-04.fits, field objects 1-10).
Field 1 did not solve (index index-5005-03.fits, field objects 1-10).
Field 1 did not solve (index index-5005-02.fits, field objects 1-10).
Field 1 did not solve (index index-5005-01.fits, field objects 1-10).
Field 1 did not solve (index index-5005-00.fits, field objects 1-10).
Field 1 did not solve (index index-4206-11.fits, field objects 1-10).
Field 1 did not solve (index index-4206-10.fits, field objects 1-10).
Field 1 did not solve (index index-4206-09.fits, field objects 1-10).
Field 1 did not solve (index index-4206-08.fits, field objects 1-10).
Field 1 did not solve (index index-4206-07.fits, field objects 1-10).
Field 1 did not solve (index index-4206-06.fits, field objects 1-10).
Field 1 did not solve (index index-4206-05.fits, field objects 1-10).
Field 1 did not solve (index index-4206-04.fits, field objects 1-10).
Field 1 did not solve (index index-4206-03.fits, field objects 1-10).
Field 1 did not solve (index index-4206-02.fits, field objects 1-10).
Field 1 did not solve (index index-4206-01.fits, field objects 1-10).
Field 1 did not solve (index index-4206-00.fits, field objects 1-10).
Field 1 did not solve (index index-4205-11.fits, field objects 1-10).
Field 1 did not solve (index index-4205-10.fits, field objects 1-10).
Field 1 did not solve (index index-4205-09.fits, field objects 1-10).
Field 1 did not solve (index index-4205-08.fits, field objects 1-10).
Field 1 did not solve (index index-4205-07.fits, field objects 1-10).
Field 1 did not solve (index index-4205-06.fits, field objects 1-10).
Field 1 did not solve (index index-4205-05.fits, field objects 1-10).
Field 1 did not solve (index index-4205-04.fits, field objects 1-10).
Field 1 did not solve (index index-4205-03.fits, field objects 1-10).
Field 1 did not solve (index index-4205-02.fits, field objects 1-10).
Field 1 did not solve (index index-4205-01.fits, field objects 1-10).
Field 1 did not solve (index index-4205-00.fits, field objects 1-10).
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
Field 1 did not solve (index index-4113.fits, field objects 1-10).
Field 1 did not solve (index index-4112.fits, field objects 1-10).
Field 1 did not solve (index index-4111.fits, field objects 1-10).
Field 1 did not solve (index index-4110.fits, field objects 1-10).
Field 1 did not solve (index index-4109.fits, field objects 1-10).
Field 1 did not solve (index index-4108.fits, field objects 1-10).
Field 1 did not solve (index index-4107.fits, field objects 1-10).
Field 1 did not solve (index index-204-11.fits, field objects 1-10).
Field 1 did not solve (index index-204-10.fits, field objects 1-10).
Field 1 did not solve (index index-204-09.fits, field objects 1-10).
Field 1 did not solve (index index-204-08.fits, field objects 1-10).
Field 1 did not solve (index index-204-07.fits, field objects 1-10).
Field 1 did not solve (index index-204-06.fits, field objects 1-10).
Field 1 did not solve (index index-204-05.fits, field objects 1-10).
Field 1 did not solve (index index-204-04.fits, field objects 1-10).
Field 1 did not solve (index index-204-03.fits, field objects 1-10).
Field 1 did not solve (index index-204-02.fits, field objects 1-10).
Field 1 did not solve (index index-204-01.fits, field objects 1-10).
Field 1 did not solve (index index-204-00.fits, field objects 1-10).
Field 1 did not solve (index index-5203-47.fits, field objects 11-20).
Field 1 did not solve (index index-5203-46.fits, field objects 11-20).
Field 1 did not solve (index index-5203-45.fits, field objects 11-20).
Field 1 did not solve (index index-5203-44.fits, field objects 11-20).
Field 1 did not solve (index index-5203-43.fits, field objects 11-20).
Field 1 did not solve (index index-5203-42.fits, field objects 11-20).
Field 1 did not solve (index index-5203-41.fits, field objects 11-20).
Field 1 did not solve (index index-5203-40.fits, field objects 11-20).
Field 1 did not solve (index index-5203-39.fits, field objects 11-20).
Field 1 did not solve (index index-5203-38.fits, field objects 11-20).
Field 1 did not solve (index index-5203-37.fits, field objects 11-20).
Field 1 did not solve (index index-5203-36.fits, field objects 11-20).
Field 1 did not solve (index index-5203-35.fits, field objects 11-20).
Field 1 did not solve (index index-5203-34.fits, field objects 11-20).
Field 1 did not solve (index index-5203-33.fits, field objects 11-20).
Field 1 did not solve (index index-5203-32.fits, field objects 11-20).
Field 1 did not solve (index index-5203-31.fits, field objects 11-20).
Field 1 did not solve (index index-5203-30.fits, field objects 11-20).
Field 1 did not solve (index index-5203-29.fits, field objects 11-20).
Field 1 did not solve (index index-5203-28.fits, field objects 11-20).
Field 1 did not solve (index index-5203-27.fits, field objects 11-20).
Field 1 did not solve (index index-5203-26.fits, field objects 11-20).
Field 1 did not solve (index index-5203-25.fits, field objects 11-20).
Field 1 did not solve (index index-5203-24.fits, field objects 11-20).
Field 1 did not solve (index index-5203-23.fits, field objects 11-20).
Field 1 did not solve (index index-5203-22.fits, field objects 11-20).
Field 1 did not solve (index index-5203-21.fits, field objects 11-20).
Field 1 did not solve (index index-5203-20.fits, field objects 11-20).
Field 1 did not solve (index index-5203-19.fits, field objects 11-20).
Field 1 did not solve (index index-5203-18.fits, field objects 11-20).
Field 1 did not solve (index index-5203-17.fits, field objects 11-20).
Field 1 did not solve (index index-5203-16.fits, field objects 11-20).
Field 1 did not solve (index index-5203-15.fits, field objects 11-20).
Field 1 did not solve (index index-5203-14.fits, field objects 11-20).
Field 1 did not solve (index index-5203-13.fits, field objects 11-20).
Field 1 did not solve (index index-5203-12.fits, field objects 11-20).
Field 1 did not solve (index index-5203-11.fits, field objects 11-20).
Field 1 did not solve (index index-5203-10.fits, field objects 11-20).
Field 1 did not solve (index index-5203-09.fits, field objects 11-20).
Field 1 did not solve (index index-5203-08.fits, field objects 11-20).
Field 1 did not solve (index index-5203-07.fits, field objects 11-20).
Field 1 did not solve (index index-5203-06.fits, field objects 11-20).
Field 1 did not solve (index index-5203-05.fits, field objects 11-20).
Field 1 did not solve (index index-5203-04.fits, field objects 11-20).
Field 1 did not solve (index index-5203-03.fits, field objects 11-20).
Field 1 did not solve (index index-5203-02.fits, field objects 11-20).
Field 1 did not solve (index index-5203-01.fits, field objects 11-20).
Field 1 did not solve (index index-5203-00.fits, field objects 11-20).
Field 1 did not solve (index index-5005-11.fits, field objects 11-20).
Field 1 did not solve (index index-5005-10.fits, field objects 11-20).
Field 1 did not solve (index index-5005-09.fits, field objects 11-20).
Field 1 did not solve (index index-5005-08.fits, field objects 11-20).
Field 1 did not solve (index index-5005-07.fits, field objects 11-20).
Field 1 did not solve (index index-5005-06.fits, field objects 11-20).
Field 1 did not solve (index index-5005-05.fits, field objects 11-20).
Field 1 did not solve (index index-5005-04.fits, field objects 11-20).
Field 1 did not solve (index index-5005-03.fits, field objects 11-20).
Field 1 did not solve (index index-5005-02.fits, field objects 11-20).
Field 1 did not solve (index index-5005-01.fits, field objects 11-20).
Field 1 did not solve (index index-5005-00.fits, field objects 11-20).
Field 1 did not solve (index index-4206-11.fits, field objects 11-20).
Field 1 did not solve (index index-4206-10.fits, field objects 11-20).
Field 1 did not solve (index index-4206-09.fits, field objects 11-20).
Field 1 did not solve (index index-4206-08.fits, field objects 11-20).
Field 1 did not solve (index index-4206-07.fits, field objects 11-20).
Field 1 did not solve (index index-4206-06.fits, field objects 11-20).
Field 1 did not solve (index index-4206-05.fits, field objects 11-20).
Field 1 did not solve (index index-4206-04.fits, field objects 11-20).
Field 1 did not solve (index index-4206-03.fits, field objects 11-20).
Field 1 did not solve (index index-4206-02.fits, field objects 11-20).
Field 1 did not solve (index index-4206-01.fits, field objects 11-20).
Field 1 did not solve (index index-4206-00.fits, field objects 11-20).
Field 1 did not solve (index index-4205-11.fits, field objects 11-20).
Field 1 did not solve (index index-4205-10.fits, field objects 11-20).
Field 1 did not solve (index index-4205-09.fits, field objects 11-20).
Field 1 did not solve (index index-4205-08.fits, field objects 11-20).
Field 1 did not solve (index index-4205-07.fits, field objects 11-20).
Field 1 did not solve (index index-4205-06.fits, field objects 11-20).
Field 1 did not solve (index index-4205-05.fits, field objects 11-20).
Field 1 did not solve (index index-4205-04.fits, field objects 11-20).
Field 1 did not solve (index index-4205-03.fits, field objects 11-20).
Field 1 did not solve (index index-4205-02.fits, field objects 11-20).
Field 1 did not solve (index index-4205-01.fits, field objects 11-20).
Field 1 did not solve (index index-4205-00.fits, field objects 11-20).
Field 1 did not solve (index index-4119.fits, field objects 11-20).
Field 1 did not solve (index index-4118.fits, field objects 11-20).
Field 1 did not solve (index index-4117.fits, field objects 11-20).
Field 1 did not solve (index index-4116.fits, field objects 11-20).
Field 1 did not solve (index index-4115.fits, field objects 11-20).
Field 1 did not solve (index index-4114.fits, field objects 11-20).
Field 1 did not solve (index index-4113.fits, field objects 11-20).
Field 1 did not solve (index index-4112.fits, field objects 11-20).
Field 1 did not solve (index index-4111.fits, field objects 11-20).
Field 1 did not solve (index index-4110.fits, field objects 11-20).
Field 1 did not solve (index index-4109.fits, field objects 11-20).
Field 1 did not solve (index index-4108.fits, field objects 11-20).
Field 1 did not solve (index index-4107.fits, field objects 11-20).
Field 1 did not solve (index index-204-11.fits, field objects 11-20).
Field 1 did not solve (index index-204-10.fits, field objects 11-20).
Field 1 did not solve (index index-204-09.fits, field objects 11-20).
Field 1 did not solve (index index-204-08.fits, field objects 11-20).
Field 1 did not solve (index index-204-07.fits, field objects 11-20).
Field 1 did not solve (index index-204-06.fits, field objects 11-20).
Field 1 did not solve (index index-204-05.fits, field objects 11-20).
Field 1 did not solve (index index-204-04.fits, field objects 11-20).
Field 1 did not solve (index index-204-03.fits, field objects 11-20).
Field 1 did not solve (index index-204-02.fits, field objects 11-20).
Field 1 did not solve (index index-204-01.fits, field objects 11-20).
Field 1 did not solve (index index-204-00.fits, field objects 11-20).
Field 1 did not solve (index index-5203-47.fits, field objects 21-30).
Field 1 did not solve (index index-5203-46.fits, field objects 21-30).
Field 1 did not solve (index index-5203-45.fits, field objects 21-30).
Field 1 did not solve (index index-5203-44.fits, field objects 21-30).
Field 1 did not solve (index index-5203-43.fits, field objects 21-30).
Field 1 did not solve (index index-5203-42.fits, field objects 21-30).
Field 1 did not solve (index index-5203-41.fits, field objects 21-30).
Field 1 did not solve (index index-5203-40.fits, field objects 21-30).
Field 1 did not solve (index index-5203-39.fits, field objects 21-30).
Field 1 did not solve (index index-5203-38.fits, field objects 21-30).
Field 1 did not solve (index index-5203-37.fits, field objects 21-30).
Field 1 did not solve (index index-5203-36.fits, field objects 21-30).
Field 1 did not solve (index index-5203-35.fits, field objects 21-30).
Field 1 did not solve (index index-5203-34.fits, field objects 21-30).
Field 1 did not solve (index index-5203-33.fits, field objects 21-30).
Field 1 did not solve (index index-5203-32.fits, field objects 21-30).
Field 1 did not solve (index index-5203-31.fits, field objects 21-30).
Field 1 did not solve (index index-5203-30.fits, field objects 21-30).
Field 1 did not solve (index index-5203-29.fits, field objects 21-30).
Field 1 did not solve (index index-5203-28.fits, field objects 21-30).
Field 1 did not solve (index index-5203-27.fits, field objects 21-30).
Field 1 did not solve (index index-5203-26.fits, field objects 21-30).
Field 1 did not solve (index index-5203-25.fits, field objects 21-30).
Field 1 did not solve (index index-5203-24.fits, field objects 21-30).
Field 1 did not solve (index index-5203-23.fits, field objects 21-30).
Field 1 did not solve (index index-5203-22.fits, field objects 21-30).
Field 1 did not solve (index index-5203-21.fits, field objects 21-30).
Field 1 did not solve (index index-5203-20.fits, field objects 21-30).
Field 1 did not solve (index index-5203-19.fits, field objects 21-30).
Field 1 did not solve (index index-5203-18.fits, field objects 21-30).
Field 1 did not solve (index index-5203-17.fits, field objects 21-30).
Field 1 did not solve (index index-5203-16.fits, field objects 21-30).
Field 1 did not solve (index index-5203-15.fits, field objects 21-30).
Field 1 did not solve (index index-5203-14.fits, field objects 21-30).
Field 1 did not solve (index index-5203-13.fits, field objects 21-30).
Field 1 did not solve (index index-5203-12.fits, field objects 21-30).
Field 1 did not solve (index index-5203-11.fits, field objects 21-30).
Field 1 did not solve (index index-5203-10.fits, field objects 21-30).
Field 1 did not solve (index index-5203-09.fits, field objects 21-30).
Field 1 did not solve (index index-5203-08.fits, field objects 21-30).
Field 1 did not solve (index index-5203-07.fits, field objects 21-30).
Field 1 did not solve (index index-5203-06.fits, field objects 21-30).
Field 1 did not solve (index index-5203-05.fits, field objects 21-30).
Field 1 did not solve (index index-5203-04.fits, field objects 21-30).
Field 1 did not solve (index index-5203-03.fits, field objects 21-30).
Field 1 did not solve (index index-5203-02.fits, field objects 21-30).
Field 1 did not solve (index index-5203-01.fits, field objects 21-30).
Field 1 did not solve (index index-5203-00.fits, field objects 21-30).
Field 1 did not solve (index index-5005-11.fits, field objects 21-30).
Field 1 did not solve (index index-5005-10.fits, field objects 21-30).
Field 1 did not solve (index index-5005-09.fits, field objects 21-30).
Field 1 did not solve (index index-5005-08.fits, field objects 21-30).
Field 1 did not solve (index index-5005-07.fits, field objects 21-30).
Field 1 did not solve (index index-5005-06.fits, field objects 21-30).
Field 1 did not solve (index index-5005-05.fits, field objects 21-30).
Field 1 did not solve (index index-5005-04.fits, field objects 21-30).
Field 1 did not solve (index index-5005-03.fits, field objects 21-30).
Field 1 did not solve (index index-5005-02.fits, field objects 21-30).
Field 1 did not solve (index index-5005-01.fits, field objects 21-30).
Field 1 did not solve (index index-5005-00.fits, field objects 21-30).
Field 1 did not solve (index index-4206-11.fits, field objects 21-30).
Field 1 did not solve (index index-4206-10.fits, field objects 21-30).
Field 1 did not solve (index index-4206-09.fits, field objects 21-30).
Field 1 did not solve (index index-4206-08.fits, field objects 21-30).
Field 1 did not solve (index index-4206-07.fits, field objects 21-30).
Field 1 did not solve (index index-4206-06.fits, field objects 21-30).
Field 1 did not solve (index index-4206-05.fits, field objects 21-30).
Field 1 did not solve (index index-4206-04.fits, field objects 21-30).
Field 1 did not solve (index index-4206-03.fits, field objects 21-30).
Field 1 did not solve (index index-4206-02.fits, field objects 21-30).
Field 1 did not solve (index index-4206-01.fits, field objects 21-30).
Field 1 did not solve (index index-4206-00.fits, field objects 21-30).
Field 1 did not solve (index index-4205-11.fits, field objects 21-30).
Field 1 did not solve (index index-4205-10.fits, field objects 21-30).
Field 1 did not solve (index index-4205-09.fits, field objects 21-30).
Field 1 did not solve (index index-4205-08.fits, field objects 21-30).
Field 1 did not solve (index index-4205-07.fits, field objects 21-30).
Field 1 did not solve (index index-4205-06.fits, field objects 21-30).
Field 1 did not solve (index index-4205-05.fits, field objects 21-30).
Field 1 did not solve (index index-4205-04.fits, field objects 21-30).
Field 1 did not solve (index index-4205-03.fits, field objects 21-30).
Field 1 did not solve (index index-4205-02.fits, field objects 21-30).
Field 1 did not solve (index index-4205-01.fits, field objects 21-30).
Field 1 did not solve (index index-4205-00.fits, field objects 21-30).
Field 1 did not solve (index index-4119.fits, field objects 21-30).
Field 1 did not solve (index index-4118.fits, field objects 21-30).
Field 1 did not solve (index index-4117.fits, field objects 21-30).
Field 1 did not solve (index index-4116.fits, field objects 21-30).
Field 1 did not solve (index index-4115.fits, field objects 21-30).
Field 1 did not solve (index index-4114.fits, field objects 21-30).
Field 1 did not solve (index index-4113.fits, field objects 21-30).
Field 1 did not solve (index index-4112.fits, field objects 21-30).
Total CPU time limit reached!
Field 1 did not solve (index index-4111.fits, field objects 21-30).
Field: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
Did not solve (or no WCS file was written).
Checking if the catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
verification OK: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
Generating wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat from image00004.cat
Catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits created.
verification OK: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
verification OK: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
Image size: 941.2'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:05.654 +62:00:35.74 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 25376 stars ###
'wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/correct_sextractor_wcs_catalog_usingxy2sky3933380.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
WCS catalog name: wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2435, passed=25376
Got 25376 stars (including 22925 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat
util/solve_plate_with_UCAC5 got 25376 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
RA wraps around 0/360 boundary: field RA 340.5598 through 0 to 19.2942, gap 19.2942 to 340.5598
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 574 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 487 matched stars entering correct_measured_positions(), 446 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 465 matched stars entering correct_measured_positions(), 14429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 340.5707 through 0 to 19.3202, gap 19.3202 to 340.5707
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 682 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 635 matched stars entering correct_measured_positions(), 14504 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.45"
Accuracy estimation diagnostic: 632 matched stars entering correct_measured_positions(), 17760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.20"
Excluding outliers - 632 stars left (next iteration limit 511)
WCS_QUALITY_DIAG: file=fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits N_match=632 sigma_overall_arcsec=5.022 sigma_q1_arcsec=11.451 sigma_q2_arcsec=2.727 sigma_q3_arcsec=19.675 sigma_q4_arcsec=5.760 n_q1=155 n_q2=300 n_q3=67 n_q4=110 worst_quadrant_to_overall_ratio=3.918
The image catalog is written to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits -region wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 2nd new image (fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits): sigma 5.022->5.022, ratio 3.918->3.918; reverting to order 3
WARNING: 1st new image has sigma_overall_arcsec=5.071 -- 2.54x the reference average (1.998); plate solution may be of low accuracy
WARNING: 2nd new image has sigma_overall_arcsec=5.022 -- 2.51x the reference average (1.998); plate solution may be of low accuracy
WARNING: 1st new image has worst_quadrant_to_overall_ratio=3.423 -- 3.98x the reference average (0.861); plate solution may be of low accuracy
WARNING: 2nd new image has worst_quadrant_to_overall_ratio=3.918 -- 4.55x the reference average (0.861); plate solution may be of low accuracy
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011_astrometric_residuals.png (968 matched stars from wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 1.06 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014_astrometric_residuals.png (963 matched stars from wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 1.03 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460_astrometric_residuals.png (629 matched stars from wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 2.14 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461_astrometric_residuals.png (632 matched stars from wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 2.20 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-02-33_20.00sec_5.00C_LIGHT_0460.fits'
Saving fully-calibrated image wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-02-Q2b1x1_062903_TTUQ2b1x1_688656_vHrpO5yd/wcs_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461.fits'
Preparing the HTML report for the field Cas-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:07:38.29 +61:54:05.3: 11.80 +/- 0.01 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:49:35.42 +65:15:40.0: 10.99 +/- 0.00 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:22:10.68 +61:21:21.8: 11.73 +/- 0.01 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:31:48.51 +60:14:06.5: 12.70 +/- 0.02 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:32:16.90 +62:16:18.7: 12.66 +/- 0.02 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:17:09.10 +61:53:44.9: 12.30 +/- 0.01 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:10:18.81 +64:39:19.4: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:17:09.10 +61:53:44.9: 12.25 +/- 0.01 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:22:10.68 +61:21:21.8: 11.38 +/- 0.01 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:07:38.29 +61:54:05.3: 11.81 +/- 0.01 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:31:48.51 +60:14:06.5: 12.53 +/- 0.02 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:12:15.73 +60:33:34.5: 12.36 +/- 0.01 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:16:15.51 +61:50:59.6: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry filter REJECTED candidate at 00:31:48.51 +60:14:06.5: ref_mag=12.60 +/- 0.02 new_mean_mag=12.0372 delta=0.56 (need > 0.90)
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Forced photometry reference-image weighted average: 11.50 +/- 0.01
Forced photometry filter REJECTED candidate at 00:17:09.10 +61:53:44.9: ref_mag=12.28 +/- 0.01 new_mean_mag=11.9582 delta=0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:07:38.29 +61:54:05.3: ref_mag=11.81 +/- 0.01 new_mean_mag=11.7656 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:22:10.68 +61:21:21.8: ref_mag=11.50 +/- 0.01 new_mean_mag=11.8128 delta=-0.31 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:32:16.90 +62:16:18.7: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Forced photometry filter REJECTED candidate at 00:32:16.90 +62:16:18.7: ref_mag=12.71 +/- 0.02 new_mean_mag=12.0766 delta=0.63 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:10:18.81 +64:39:19.4: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:49:35.42 +65:15:40.0: 11.17 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.06 +/- 0.00
Forced photometry filter REJECTED candidate at 23:49:35.42 +65:15:40.0: ref_mag=11.06 +/- 0.00 new_mean_mag=11.0175 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:18:09.25 +60:52:58.0: 13.01 +/- 0.04 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:12:15.73 +60:33:34.5: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter REJECTED candidate at 00:12:15.73 +60:33:34.5: ref_mag=12.38 +/- 0.01 new_mean_mag=12.1407 delta=0.24 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:16:15.51 +61:50:59.6: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry filter REJECTED candidate at 00:16:15.51 +61:50:59.6: ref_mag=12.53 +/- 0.01 new_mean_mag=12.1028 delta=0.42 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:18:09.25 +60:52:58.0: 12.86 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter REJECTED candidate at 00:18:09.25 +60:52:58.0: ref_mag=12.93 +/- 0.02 new_mean_mag=12.1572 delta=0.77 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:10:10.97 +61:40:52.4: 12.59 +/- 0.02 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:39:08.45 +63:36:30.9: 13.07 +/- 0.03 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:17:23.57 +60:16:18.9: 12.55 +/- 0.02 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 23:58:22.18 +60:44:48.6: 12.19 +/- 0.01 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:11:32.33 +61:13:55.7: 13.08 +/- 0.03 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:30:43.57 +62:07:11.0: 14.36 +/- 0.10 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:10:10.97 +61:40:52.4: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter REJECTED candidate at 00:10:10.97 +61:40:52.4: ref_mag=12.51 +/- 0.01 new_mean_mag=12.1816 delta=0.33 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:39:08.45 +63:36:30.9: 12.59 +/- 0.02 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:17:23.57 +60:16:18.9: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Forced photometry filter REJECTED candidate at 00:39:08.45 +63:36:30.9: ref_mag=12.71 +/- 0.02 new_mean_mag=12.2255 delta=0.49 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:17:23.57 +60:16:18.9: ref_mag=12.60 +/- 0.01 new_mean_mag=12.1903 delta=0.41 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:11:14.79 +64:53:31.2: 14.74 +/- 0.13 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:29:59.70 +59:04:50.6: 12.63 +/- 0.02 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 23:58:22.18 +60:44:48.6: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter REJECTED candidate at 23:58:22.18 +60:44:48.6: ref_mag=12.20 +/- 0.01 new_mean_mag=12.1748 delta=0.03 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:00:06.28 +60:22:52.9: 12.25 +/- 0.02 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:11:32.33 +61:13:55.7: 13.14 +/- 0.03 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:30:43.57 +62:07:11.0: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter REJECTED candidate at 00:11:32.33 +61:13:55.7: ref_mag=13.11 +/- 0.02 new_mean_mag=12.2320 delta=0.88 (need > 0.90)
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter KEPT candidate at 00:30:43.57 +62:07:11.0: ref_mag=13.74 +/- 0.04 new_mean_mag=12.2687 delta=1.47 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:11:14.79 +64:53:31.2: 15.26 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.11
Forced photometry filter KEPT candidate at 00:11:14.79 +64:53:31.2: ref_mag=14.89 +/- 0.11 new_mean_mag=12.2440 delta=2.64 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:29:59.70 +59:04:50.6: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter REJECTED candidate at 00:29:59.70 +59:04:50.6: ref_mag=12.60 +/- 0.01 new_mean_mag=12.1825 delta=0.42 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:00:06.28 +60:22:52.9: 12.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry filter REJECTED candidate at 00:00:06.28 +60:22:52.9: ref_mag=12.28 +/- 0.01 new_mean_mag=12.2063 delta=0.07 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:13:01.22 +63:09:09.1: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:09:44.32 +62:45:12.4: 12.83 +/- 0.02 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:08:56.27 +62:33:27.5: 12.29 +/- 0.01 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:07:15.48 +63:39:51.5: 12.87 +/- 0.03 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:09:44.32 +62:45:12.4: 12.50 +/- 0.02 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:13:01.22 +63:09:09.1: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter REJECTED candidate at 00:13:01.22 +63:09:09.1: ref_mag=12.68 +/- 0.01 new_mean_mag=12.2709 delta=0.40 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:09:44.32 +62:45:12.4: ref_mag=12.62 +/- 0.01 new_mean_mag=12.2526 delta=0.36 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-08_19-44-36_20.00sec_-14.90C_LIGHT_0011.fits at 00:10:55.38 +61:13:39.3: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:08:56.27 +62:33:27.5: 12.28 +/- 0.01 detection
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:07:15.48 +63:39:51.5: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter REJECTED candidate at 00:08:56.27 +62:33:27.5: ref_mag=12.29 +/- 0.01 new_mean_mag=12.2453 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Forced photometry filter REJECTED candidate at 00:07:15.48 +63:39:51.5: ref_mag=12.69 +/- 0.02 new_mean_mag=12.2424 delta=0.45 (need > 0.90)
Forced photometry on wcs_Cas-02-Q2b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits at 00:10:55.38 +61:13:39.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Forced photometry filter REJECTED candidate at 00:10:55.38 +61:13:39.3: ref_mag=12.89 +/- 0.02 new_mean_mag=12.3072 delta=0.58 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out36204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out35618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36233.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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: 2s
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Considering the candidate 32080_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 32080_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 32082_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 32082_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 32400_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 32400_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:36:59.19 +63:07:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33916_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 33916_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 34808_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 34808_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 34841_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 34841_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:07:05.54 +61:48:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35151_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 35151_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 35537_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 35537_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 35618_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 35618_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 35721_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 35721_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 35765_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 35765_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 35912_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 35912_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 35935_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 35935_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 36022_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36022_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 36058_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36058_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 36067_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36067_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:34:55.14 +62:55:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36100_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36100_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 36118_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36118_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:26:11.30 +62:03:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36139_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36139_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 36185_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36185_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 36204_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36204_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:30:43.57 +62:07:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.420 430334110785856896 007.68079151321 +62.11954200585 11.9269 11.1351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 36206_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36206_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 36233_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 36233_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 36235_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36235_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 36280_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36280_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 36281_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36281_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 36302_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36302_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 36322_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36322_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 36367_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36367_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:16:56.65 +61:28:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36386_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 36386_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 07985_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 07985_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (33.3") between the two second-epoch detections
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Considering the candidate 246353_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246353_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246356_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246356_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246360_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246360_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246366_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246366_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246367_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246367_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246372_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246372_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246373_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246373_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246379_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246379_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 246390_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246390_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246394_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246394_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 246398_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246398_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 246413_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246413_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 246416_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246416_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246417_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246417_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246422_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246422_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 246425_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246425_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 246430_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246430_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246435_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246435_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246444_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246444_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 246456_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246456_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 246463_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246463_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246465_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246465_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246470_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246470_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246486_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246486_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246497_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246497_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246503_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246503_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 246517_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246517_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 246522_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246522_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 246530_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246530_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 246532_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246532_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 246534_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246534_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246544_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246544_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246557_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246557_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246558_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246558_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246559_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246559_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 246567_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246567_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246569_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246569_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246571_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246571_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246572_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246572_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246573_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246573_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 246586_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246586_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246587_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246587_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246590_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246590_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246592_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246592_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246605_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246605_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246612_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246612_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 246620_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246620_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246627_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246627_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246632_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246632_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246633_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246633_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246634_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246634_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246638_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246638_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246641_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246641_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246644_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246644_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246646_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246646_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246652_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246652_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246661_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246661_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 246670_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246670_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246671_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246671_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246672_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246672_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246679_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246679_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 246680_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246680_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246682_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246682_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246684_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246684_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:23:11.89 +62:26:30.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)
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Considering the candidate 246685_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246685_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246690_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246690_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246692_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246692_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:09:47.55 +62:48:09.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)
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Considering the candidate 246693_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246693_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246694_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246694_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246695_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246695_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 246701_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246701_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246702_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246702_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 246705_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246705_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246707_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246707_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246708_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246708_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 246709_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246709_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246711_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246711_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 23:41:34.62 +59:35:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246715_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246715_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246717_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246717_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246718_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246718_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246725_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246725_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246726_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246726_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246731_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246731_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246733_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246733_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246735_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246735_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246739_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246739_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246742_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246742_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246743_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246743_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246746_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246746_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 246751_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246751_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 246754_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246754_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246757_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246757_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246759_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246759_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246762_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246762_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246763_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246763_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246766_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246766_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 246769_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246769_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246771_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246771_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246772_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246772_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246774_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246774_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 246783_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246783_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246784_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246784_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246790_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246790_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246793_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246793_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246796_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246796_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246799_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246799_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246800_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246800_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246802_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246802_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246804_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246804_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:17:16.59 +62:50:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.396 431272269083225472 004.31670009758 +62.84887232171 13.6447 13.3513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 246805_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246805_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246806_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246806_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:16:34.37 +63:46:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246809_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246809_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 246811_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246811_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246819_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246819_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246824_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246824_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246827_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246827_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246828_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246828_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 246830_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246830_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246835_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246835_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246837_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246837_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:10:43.22 +63:25:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246841_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246841_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246843_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246843_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246847_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246847_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246848_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 246848_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246850_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246850_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246851_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246851_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246852_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246852_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 23:58:29.56 +61:13:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246853_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246853_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 246861_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246861_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246866_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246866_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 246867_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246867_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246869_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246869_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 246870_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 246870_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250031_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 250031_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250074_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 250074_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 23:48:41.44 +62:14:43.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251973_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 251973_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:21:26.26 +59:13:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252161_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 252161_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252515_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 252515_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:04:53.32 +61:20:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253199_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 253199_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 253456_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 253456_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254753_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 254753_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254974_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 254974_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255066_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 255066_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255290_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 255290_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256118_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 256118_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256405_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 256405_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256902_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 256902_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257045_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 257045_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257085_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 257085_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257120_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 257120_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257165_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 257165_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257230_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 257230_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257273_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 257273_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257553_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 257553_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:05:14.94 +61:17:30.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 257847_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 257847_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258051_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 258051_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:35:28.95 +61:53:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.824 430277902557713152 008.86871905799 +61.88558876524 12.9623 11.9181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258212_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 258212_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 258580_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 258580_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:01:49.46 +61:12:24.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 258614_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 258614_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 258822_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 258822_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 258881_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 258881_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:01:41.70 +61:11:25.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259022_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 259022_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 259098_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 259098_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 259152_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 259152_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 259205_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 259205_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 259361_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 259361_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 259374_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 259374_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 23:49:00.70 +59:57:21.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259418_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 259418_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 23:30:20.08 +57:57:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259548_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 259548_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 259639_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 259639_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259670_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 259670_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259680_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 259680_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 259818_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 259818_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:12:35.48 +62:53:08.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
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Considering the candidate 260090_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 260090_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 260261_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 260261_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260299_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 260299_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260766_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 260766_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:17:13.92 +62:51:13.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)
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Considering the candidate 260767_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 260767_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260845_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 260845_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261020_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 261020_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261132_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 261132_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 23:29:48.60 +58:31:43.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 261380_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 261380_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261537_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 261537_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 261677_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 261677_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261825_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 261825_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 262108_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 262108_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 262183_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 262183_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 262316_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 262316_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262701_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 262701_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 262721_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 262721_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 262826_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 262826_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 262854_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 262854_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 262865_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 262865_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 262924_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 262924_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262992_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 262992_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263068_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 263068_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263498_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 263498_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 263646_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 263646_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263891_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 263891_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263924_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 263924_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263946_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 263946_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264174_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 264174_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264189_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 264189_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264210_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 264210_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264285_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 264285_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 264430_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 264430_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264431_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 264431_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264469_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 264469_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264637_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 264637_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264727_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 264727_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264753_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 264753_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264815_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 264815_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264828_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 264828_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:17:09.44 +61:30:55.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 264928_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 264928_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264996_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 264996_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265122_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 265122_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265179_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 265179_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:27:09.64 +61:10:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265212_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 265212_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265510_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 265510_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265604_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 265604_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:30:04.65 +60:13:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 5.616 428621007255201664 007.51652436727 +60.22362261208 14.0218 13.5201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 266087_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 266087_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 266165_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 266165_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266169_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 266169_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266353_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 266353_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266522_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 266522_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 266555_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 266555_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266649_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 266649_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 266668_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 266668_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266726_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 266726_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 266801_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 266801_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266803_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 266803_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 266820_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 266820_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266850_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 266850_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 266861_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 266861_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266973_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 266973_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267008_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 267008_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 267041_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 267041_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267070_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 267070_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267121_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 267121_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 267241_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 267241_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267250_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 267250_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267337_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 267337_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267444_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 267444_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267523_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 267523_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 267632_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 267632_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267669_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 267669_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267945_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 267945_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267950_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 267950_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267953_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 267953_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268052_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 268052_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268150_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 268150_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268350_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 268350_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268356_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 268356_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268408_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 268408_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268424_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 268424_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 268486_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 268486_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268495_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 268495_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268550_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 268550_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268601_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 268601_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268743_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 268743_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 268750_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 268750_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268824_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 268824_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 269023_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 269023_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 269163_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 269163_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269224_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 269224_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269295_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 269295_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269309_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 269309_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269310_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 269310_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269433_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 269433_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269485_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 269485_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269594_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 269594_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269659_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 269659_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269713_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 269713_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 269826_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 269826_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270093_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 270093_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270152_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 270152_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270191_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 270191_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270370_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 270370_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270472_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 270472_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:33:33.36 +62:31:12.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
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Considering the candidate 270521_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 270521_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 270538_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 270538_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270554_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 270554_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270637_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 270637_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270671_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 270671_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 271020_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 271020_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 271076_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 271076_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271140_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 271140_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271206_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 271206_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 271447_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 271447_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271699_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 271699_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 271803_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 271803_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 271815_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 271815_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 271854_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 271854_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 271898_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 271898_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 272007_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 272007_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 272483_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 272483_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 272491_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 272491_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 272496_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 272496_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 272828_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 272828_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 273091_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 273091_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 273333_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 273333_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 273372_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 273372_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 273421_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 273421_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 273494_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 273494_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 273527_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 273527_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 273541_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 273541_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 273770_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 273770_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 274188_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 274188_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 274292_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 274292_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 274388_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 274388_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 274439_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 274439_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 274489_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 274489_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 274520_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 274520_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 274621_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 274621_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 274717_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 274717_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 274738_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 274738_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 274771_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 274771_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 274813_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 274813_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 274907_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 274907_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 275047_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 275047_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 275075_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 275075_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 275432_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 275432_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 275439_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 275439_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 275520_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 275520_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 275526_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 275526_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 275538_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 275538_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 275618_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 275618_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 275751_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 275751_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 275755_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 275755_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 275759_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 275759_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 275857_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 275857_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 275918_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 275918_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 275977_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 275977_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 276005_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 276005_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 276041_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 276041_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 276062_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 276062_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 276147_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 276147_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 276222_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 276222_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 276325_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 276325_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 276447_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 276447_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 276517_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 276517_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 276623_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 276623_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 276636_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 276636_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 276637_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 276637_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 276710_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 276710_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 276723_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 276723_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (24.5") between the two second-epoch detections
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Considering the candidate 276785_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 276785_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 276873_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 276873_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 276914_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 276914_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 276936_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 276936_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 277006_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277006_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 277019_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277019_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 277027_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277027_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 277034_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 277034_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 277040_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277040_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:21:44.48 +59:33:02.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)
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Considering the candidate 277082_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 277082_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 277107_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277107_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 277265_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 277265_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 277330_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277330_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 277350_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277350_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 277422_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277422_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 277438_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277438_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277449_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277449_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277451_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277451_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 277537_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277537_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277542_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277542_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 277574_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 277574_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 277589_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277589_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277605_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277605_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277614_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277614_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277633_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277633_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277651_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 277651_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277711_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277711_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277754_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 277754_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277821_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277821_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277854_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 277854_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277905_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277905_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277956_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277956_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277988_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 277988_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277995_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 277995_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278006_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278006_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (31.7") between the two second-epoch detections
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Considering the candidate 278014_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278014_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278088_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 278088_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278100_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278100_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278151_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278151_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278210_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278210_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278221_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278221_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278226_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278226_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278228_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278228_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278283_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 278283_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278303_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278303_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278304_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278304_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278327_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 278327_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278384_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278384_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278395_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278395_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278411_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278411_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278421_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278421_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278451_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278451_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278458_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278458_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 278495_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278495_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 278533_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278533_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 278569_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 278569_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 278662_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278662_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 278673_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278673_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (25.0") between the two second-epoch detections
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Considering the candidate 278730_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278730_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 278748_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278748_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 278760_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278760_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 278788_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278788_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278817_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 278817_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 49463_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 49463_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
**** FOUND 00:36:59.11 +63:08:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236991_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 236991_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 63831_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 63831_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 30302_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 30302_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 189730_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 189730_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46413_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 46413_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 92653_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 92653_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 29265_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 29265_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
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Considering the candidate 97063_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
Preparing report for the candidate 97063_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24334_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461
The candidate 24334_fd_Cas-02-Q2b1x1_2026-06-20_05-03-34_20.00sec_5.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 9s
make_report_in_HTML.sh TOTAL: 302s
Prepared the HTML report for the field Cas-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:10:18.81 +64:39:19.4
00:11:14.79 +64:53:31.2
23:58:36.89 +58:25:46.5
00:29:27.82 +60:49:56.1
00:16:47.03 +64:42:55.0
00:04:33.49 +58:31:26.0
23:55:08.88 +62:13:12.1
00:06:31.54 +62:21:03.3
00:14:55.02 +58:40:52.3
00:29:41.19 +62:45:12.3
00:18:06.59 +63:05:08.4
00:24:08.36 +62:24:35.2
00:15:46.09 +64:49:40.7
00:27:25.45 +62:36:32.8
23:25:18.12 +57:37:12.1
00:24:21.98 +59:46:31.8
23:34:14.94 +65:40:48.1
00:24:52.06 +58:40:49.6
23:54:02.91 +64:01:04.1
23:24:39.94 +64:41:36.4
23:44:16.65 +61:58:50.3
23:30:23.33 +64:09:25.2
00:18:49.80 +59:41:44.4
00:22:06.77 +63:58:51.2
00:06:39.88 +63:07:45.2
00:03:34.67 +63:34:49.5
23:44:26.64 +61:51:10.5
23:23:11.05 +63:45:18.2
00:00:30.07 +65:48:26.1
23:50:13.48 +61:49:47.5
00:21:17.66 +58:09:09.5
00:11:38.65 +62:49:32.6
00:32:04.74 +63:10:05.9
00:17:26.19 +61:52:46.3
00:22:02.50 +62:11:52.6
00:35:15.80 +63:00:42.3
00:21:56.58 +61:46:06.5
23:52:13.16 +65:38:35.1
00:10:44.24 +59:41:51.2
00:10:45.53 +63:25:28.5
00:10:26.03 +60:01:06.4
00:30:23.15 +60:12:42.8
00:22:14.89 +61:43:13.6
00:23:54.03 +60:22:48.1
00:36:08.60 +62:39:27.6
23:59:12.50 +63:48:15.4
00:15:02.46 +61:26:05.2
00:21:47.25 +61:02:51.3
23:27:44.47 +57:32:13.4
00:11:16.41 +59:58:35.0
00:40:45.62 +64:16:36.7
00:23:45.07 +59:32:01.1
00:23:31.32 +65:19:48.0
00:02:05.43 +63:18:21.2
00:36:20.85 +62:40:04.6
00:01:54.79 +63:10:51.2
00:34:36.24 +62:38:19.3
23:44:59.54 +61:59:31.2
00:27:06.32 +61:13:07.6
00:28:27.63 +63:43:01.9
00:20:42.27 +58:20:31.5
00:09:15.91 +59:38:43.9
00:23:26.38 +62:17:45.0
00:24:10.80 +62:20:28.7
23:46:28.29 +63:40:33.6
00:21:54.61 +64:21:30.0
23:48:52.99 +61:40:27.3
00:17:56.90 +59:09:20.5
00:12:01.75 +57:56:55.7
00:07:55.37 +63:41:10.3
00:05:33.91 +62:32:06.1
00:28:42.73 +63:24:32.8
00:32:03.42 +58:44:20.9
00:20:28.24 +63:28:45.2
00:13:40.51 +62:31:06.5
23:24:49.11 +57:25:54.6
00:19:13.59 +63:35:39.0
00:05:21.04 +63:24:15.2
00:19:24.93 +59:23:46.2
00:12:19.82 +60:34:41.4
00:30:54.68 +63:26:03.2
00:22:10.68 +64:32:05.5
00:28:07.31 +63:12:32.5
00:16:22.75 +61:54:20.3
00:41:22.76 +64:38:36.1
00:05:24.33 +57:58:25.5
00:22:22.12 +59:28:19.3
00:09:20.47 +58:03:30.0
00:11:48.28 +61:45:47.8
00:05:11.91 +60:11:01.0
23:26:59.12 +64:37:21.5
00:31:04.23 +58:32:51.9
23:58:29.51 +63:50:02.4
00:20:42.97 +62:52:57.8
23:42:11.08 +58:56:31.9
23:53:09.74 +62:18:07.4
23:49:37.36 +61:05:24.8
00:36:09.90 +62:54:05.0
00:15:05.59 +63:31:33.7
00:12:27.40 +60:10:24.0
23:28:12.92 +63:48:23.1
23:48:54.64 +64:22:28.6
00:21:41.13 +62:06:54.0
00:08:40.94 +63:50:28.9
00:32:46.68 +59:50:59.1
23:24:47.03 +63:17:45.8
23:30:17.78 +64:29:51.3
00:27:40.15 +64:55:42.0
00:10:35.06 +59:42:25.3
00:11:06.41 +63:53:48.0
00:07:31.54 +62:23:56.3
00:41:03.00 +65:48:58.1
00:05:59.75 +64:46:53.0
23:44:00.19 +63:59:36.5
00:01:08.45 +62:53:36.4
00:26:09.80 +66:06:26.9
00:07:23.74 +64:28:32.7
23:21:47.31 +63:52:52.7
00:22:51.43 +66:01:51.6
00:11:43.97 +61:21:08.7
23:28:06.19 +64:26:26.5
23:29:38.03 +64:59:16.0
00:07:40.74 +64:42:27.6
23:29:21.47 +63:22:22.0
23:51:07.26 +62:08:50.7
00:07:05.62 +61:48:59.6
########### Completed Cas-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
00:10:18.81 +64:39:19.4
00:11:14.79 +64:53:31.2
00:16:47.03 +64:42:55.0
00:04:33.49 +58:31:26.0
23:55:08.88 +62:13:12.1
00:06:31.54 +62:21:03.3
00:14:55.02 +58:40:52.3
00:29:41.19 +62:45:12.3
00:18:06.59 +63:05:08.4
00:24:08.36 +62:24:35.2
00:15:46.09 +64:49:40.7
00:27:25.45 +62:36:32.8
23:25:18.12 +57:37:12.1
00:24:21.98 +59:46:31.8
23:34:14.94 +65:40:48.1
00:24:52.06 +58:40:49.6
23:54:02.91 +64:01:04.1
23:24:39.94 +64:41:36.4
23:44:16.65 +61:58:50.3
23:30:23.33 +64:09:25.2
00:18:49.80 +59:41:44.4
00:22:06.77 +63:58:51.2
00:06:39.88 +63:07:45.2
00:03:34.67 +63:34:49.5
23:44:26.64 +61:51:10.5
23:23:11.05 +63:45:18.2
00:00:30.07 +65:48:26.1
23:50:13.48 +61:49:47.5
00:21:17.66 +58:09:09.5
00:11:38.65 +62:49:32.6
00:32:04.74 +63:10:05.9
00:17:26.19 +61:52:46.3
00:22:02.50 +62:11:52.6
00:35:15.80 +63:00:42.3
00:21:56.58 +61:46:06.5
23:52:13.16 +65:38:35.1
00:10:44.24 +59:41:51.2
00:10:45.53 +63:25:28.5
00:10:26.03 +60:01:06.4
00:30:23.15 +60:12:42.8
00:22:14.89 +61:43:13.6
00:23:54.03 +60:22:48.1
00:36:08.60 +62:39:27.6
23:59:12.50 +63:48:15.4
00:15:02.46 +61:26:05.2
00:21:47.25 +61:02:51.3
23:27:44.47 +57:32:13.4
00:11:16.41 +59:58:35.0
00:40:45.62 +64:16:36.7
00:23:45.07 +59:32:01.1
00:23:31.32 +65:19:48.0
00:02:05.43 +63:18:21.2
00:36:20.85 +62:40:04.6
00:01:54.79 +63:10:51.2
00:34:36.24 +62:38:19.3
23:44:59.54 +61:59:31.2
00:27:06.32 +61:13:07.6
00:28:27.63 +63:43:01.9
00:20:42.27 +58:20:31.5
00:09:15.91 +59:38:43.9
00:23:26.38 +62:17:45.0
00:24:10.80 +62:20:28.7
23:46:28.29 +63:40:33.6
00:21:54.61 +64:21:30.0
23:48:52.99 +61:40:27.3
00:17:56.90 +59:09:20.5
00:12:01.75 +57:56:55.7
00:07:55.37 +63:41:10.3
00:05:33.91 +62:32:06.1
00:28:42.73 +63:24:32.8
00:32:03.42 +58:44:20.9
00:20:28.24 +63:28:45.2
00:13:40.51 +62:31:06.5
23:24:49.11 +57:25:54.6
00:19:13.59 +63:35:39.0
00:05:21.04 +63:24:15.2
00:19:24.93 +59:23:46.2
00:12:19.82 +60:34:41.4
00:30:54.68 +63:26:03.2
00:22:10.68 +64:32:05.5
00:28:07.31 +63:12:32.5
00:16:22.75 +61:54:20.3
00:41:22.76 +64:38:36.1
00:05:24.33 +57:58:25.5
00:22:22.12 +59:28:19.3
00:09:20.47 +58:03:30.0
00:11:48.28 +61:45:47.8
00:05:11.91 +60:11:01.0
23:26:59.12 +64:37:21.5
00:31:04.23 +58:32:51.9
23:58:29.51 +63:50:02.4
00:20:42.97 +62:52:57.8
23:42:11.08 +58:56:31.9
23:53:09.74 +62:18:07.4
23:49:37.36 +61:05:24.8
00:36:09.90 +62:54:05.0
00:15:05.59 +63:31:33.7
00:12:27.40 +60:10:24.0
23:28:12.92 +63:48:23.1
23:48:54.64 +64:22:28.6
00:21:41.13 +62:06:54.0
00:08:40.94 +63:50:28.9
00:32:46.68 +59:50:59.1
23:24:47.03 +63:17:45.8
23:30:17.78 +64:29:51.3
00:27:40.15 +64:55:42.0
00:10:35.06 +59:42:25.3
00:11:06.41 +63:53:48.0
00:07:31.54 +62:23:56.3
00:41:03.00 +65:48:58.1
00:05:59.75 +64:46:53.0
23:44:00.19 +63:59:36.5
00:01:08.45 +62:53:36.4
00:26:09.80 +66:06:26.9
00:07:23.74 +64:28:32.7
23:21:47.31 +63:52:52.7
00:22:51.43 +66:01:51.6
00:11:43.97 +61:21:08.7
23:28:06.19 +64:26:26.5
00:29:27.82 +60:49:56.1
23:29:21.47 +63:22:22.0
00:07:40.74 +64:42:27.6
23:58:36.89 +58:25:46.5
23:51:07.26 +62:08:50.7
23:29:38.03 +64:59:16.0
00:07:05.62 +61:48:59.6
###################################################################################
00:10:18.81 +64:39:19.4 -- not an asteroid (will add it to exclusion list)
00:11:14.79 +64:53:31.2 -- not an asteroid (will add it to exclusion list)
00:16:47.03 +64:42:55.0 -- not an asteroid (will add it to exclusion list)
00:04:33.49 +58:31:26.0 -- not an asteroid (will add it to exclusion list)
23:55:08.88 +62:13:12.1 -- not an asteroid (will add it to exclusion list)
00:06:31.54 +62:21:03.3 -- not an asteroid (will add it to exclusion list)
00:14:55.02 +58:40:52.3 -- not an asteroid (will add it to exclusion list)
00:29:41.19 +62:45:12.3 -- not an asteroid (will add it to exclusion list)
00:18:06.59 +63:05:08.4 -- not an asteroid (will add it to exclusion list)
00:24:08.36 +62:24:35.2 -- not an asteroid (will add it to exclusion list)
00:15:46.09 +64:49:40.7 -- not an asteroid (will add it to exclusion list)
00:27:25.45 +62:36:32.8 -- not an asteroid (will add it to exclusion list)
23:25:18.12 +57:37:12.1 -- not an asteroid (will add it to exclusion list)
00:24:21.98 +59:46:31.8 -- not an asteroid (will add it to exclusion list)
23:34:14.94 +65:40:48.1 -- not an asteroid (will add it to exclusion list)
00:24:52.06 +58:40:49.6 -- not an asteroid (will add it to exclusion list)
23:54:02.91 +64:01:04.1 -- not an asteroid (will add it to exclusion list)
23:24:39.94 +64:41:36.4 -- not an asteroid (will add it to exclusion list)
23:44:16.65 +61:58:50.3 -- not an asteroid (will add it to exclusion list)
23:30:23.33 +64:09:25.2 -- not an asteroid (will add it to exclusion list)
00:18:49.80 +59:41:44.4 -- not an asteroid (will add it to exclusion list)
00:22:06.77 +63:58:51.2 -- not an asteroid (will add it to exclusion list)
00:06:39.88 +63:07:45.2 -- not an asteroid (will add it to exclusion list)
00:03:34.67 +63:34:49.5 -- not an asteroid (will add it to exclusion list)
23:44:26.64 +61:51:10.5 -- not an asteroid (will add it to exclusion list)
23:23:11.05 +63:45:18.2 -- not an asteroid (will add it to exclusion list)
00:00:30.07 +65:48:26.1 -- not an asteroid (will add it to exclusion list)
23:50:13.48 +61:49:47.5 -- not an asteroid (will add it to exclusion list)
00:21:17.66 +58:09:09.5 -- not an asteroid (will add it to exclusion list)
00:11:38.65 +62:49:32.6 -- not an asteroid (will add it to exclusion list)
00:32:04.74 +63:10:05.9 -- not an asteroid (will add it to exclusion list)
00:17:26.19 +61:52:46.3 -- not an asteroid (will add it to exclusion list)
00:22:02.50 +62:11:52.6 -- not an asteroid (will add it to exclusion list)
00:35:15.80 +63:00:42.3 -- not an asteroid (will add it to exclusion list)
00:21:56.58 +61:46:06.5 -- not an asteroid (will add it to exclusion list)
23:52:13.16 +65:38:35.1 -- not an asteroid (will add it to exclusion list)
00:10:44.24 +59:41:51.2 -- not an asteroid (will add it to exclusion list)
00:10:45.53 +63:25:28.5 -- not an asteroid (will add it to exclusion list)
00:10:26.03 +60:01:06.4 -- not an asteroid (will add it to exclusion list)
00:30:23.15 +60:12:42.8 -- not an asteroid (will add it to exclusion list)
00:22:14.89 +61:43:13.6 -- not an asteroid (will add it to exclusion list)
00:23:54.03 +60:22:48.1 -- not an asteroid (will add it to exclusion list)
00:36:08.60 +62:39:27.6 -- not an asteroid (will add it to exclusion list)
23:59:12.50 +63:48:15.4 -- not an asteroid (will add it to exclusion list)
00:15:02.46 +61:26:05.2 -- not an asteroid (will add it to exclusion list)
00:21:47.25 +61:02:51.3 -- not an asteroid (will add it to exclusion list)
23:27:44.47 +57:32:13.4 -- not an asteroid (will add it to exclusion list)
00:11:16.41 +59:58:35.0 -- not an asteroid (will add it to exclusion list)
00:40:45.62 +64:16:36.7 -- not an asteroid (will add it to exclusion list)
00:23:45.07 +59:32:01.1 -- not an asteroid (will add it to exclusion list)
00:23:31.32 +65:19:48.0 -- not an asteroid (will add it to exclusion list)
00:02:05.43 +63:18:21.2 -- not an asteroid (will add it to exclusion list)
00:36:20.85 +62:40:04.6 -- not an asteroid (will add it to exclusion list)
00:01:54.79 +63:10:51.2 -- not an asteroid (will add it to exclusion list)
00:34:36.24 +62:38:19.3 -- not an asteroid (will add it to exclusion list)
23:44:59.54 +61:59:31.2 -- not an asteroid (will add it to exclusion list)
00:27:06.32 +61:13:07.6 -- not an asteroid (will add it to exclusion list)
00:28:27.63 +63:43:01.9 -- not an asteroid (will add it to exclusion list)
00:20:42.27 +58:20:31.5 -- not an asteroid (will add it to exclusion list)
00:09:15.91 +59:38:43.9 -- not an asteroid (will add it to exclusion list)
00:23:26.38 +62:17:45.0 -- not an asteroid (will add it to exclusion list)
00:24:10.80 +62:20:28.7 -- not an asteroid (will add it to exclusion list)
23:46:28.29 +63:40:33.6 -- not an asteroid (will add it to exclusion list)
00:21:54.61 +64:21:30.0 -- not an asteroid (will add it to exclusion list)
23:48:52.99 +61:40:27.3 -- not an asteroid (will add it to exclusion list)
00:17:56.90 +59:09:20.5 -- not an asteroid (will add it to exclusion list)
00:12:01.75 +57:56:55.7 -- not an asteroid (will add it to exclusion list)
00:07:55.37 +63:41:10.3 -- not an asteroid (will add it to exclusion list)
00:05:33.91 +62:32:06.1 -- not an asteroid (will add it to exclusion list)
00:28:42.73 +63:24:32.8 -- not an asteroid (will add it to exclusion list)
00:32:03.42 +58:44:20.9 -- not an asteroid (will add it to exclusion list)
00:20:28.24 +63:28:45.2 -- not an asteroid (will add it to exclusion list)
00:13:40.51 +62:31:06.5 -- not an asteroid (will add it to exclusion list)
23:24:49.11 +57:25:54.6 -- not an asteroid (will add it to exclusion list)
00:19:13.59 +63:35:39.0 -- not an asteroid (will add it to exclusion list)
00:05:21.04 +63:24:15.2 -- not an asteroid (will add it to exclusion list)
00:19:24.93 +59:23:46.2 -- not an asteroid (will add it to exclusion list)
00:12:19.82 +60:34:41.4 -- not an asteroid (will add it to exclusion list)
00:30:54.68 +63:26:03.2 -- not an asteroid (will add it to exclusion list)
00:22:10.68 +64:32:05.5 -- not an asteroid (will add it to exclusion list)
00:28:07.31 +63:12:32.5 -- not an asteroid (will add it to exclusion list)
00:16:22.75 +61:54:20.3 -- not an asteroid (will add it to exclusion list)
00:41:22.76 +64:38:36.1 -- not an asteroid (will add it to exclusion list)
00:05:24.33 +57:58:25.5 -- not an asteroid (will add it to exclusion list)
00:22:22.12 +59:28:19.3 -- not an asteroid (will add it to exclusion list)
00:09:20.47 +58:03:30.0 -- not an asteroid (will add it to exclusion list)
00:11:48.28 +61:45:47.8 -- not an asteroid (will add it to exclusion list)
00:05:11.91 +60:11:01.0 -- not an asteroid (will add it to exclusion list)
23:26:59.12 +64:37:21.5 -- not an asteroid (will add it to exclusion list)
00:31:04.23 +58:32:51.9 -- not an asteroid (will add it to exclusion list)
23:58:29.51 +63:50:02.4 -- not an asteroid (will add it to exclusion list)
00:20:42.97 +62:52:57.8 -- not an asteroid (will add it to exclusion list)
23:42:11.08 +58:56:31.9 -- not an asteroid (will add it to exclusion list)
23:53:09.74 +62:18:07.4 -- not an asteroid (will add it to exclusion list)
23:49:37.36 +61:05:24.8 -- not an asteroid (will add it to exclusion list)
00:36:09.90 +62:54:05.0 -- not an asteroid (will add it to exclusion list)
00:15:05.59 +63:31:33.7 -- not an asteroid (will add it to exclusion list)
00:12:27.40 +60:10:24.0 -- not an asteroid (will add it to exclusion list)
23:28:12.92 +63:48:23.1 -- not an asteroid (will add it to exclusion list)
23:48:54.64 +64:22:28.6 -- not an asteroid (will add it to exclusion list)
00:21:41.13 +62:06:54.0 -- not an asteroid (will add it to exclusion list)
00:08:40.94 +63:50:28.9 -- not an asteroid (will add it to exclusion list)
00:32:46.68 +59:50:59.1 -- not an asteroid (will add it to exclusion list)
23:24:47.03 +63:17:45.8 -- not an asteroid (will add it to exclusion list)
23:30:17.78 +64:29:51.3 -- not an asteroid (will add it to exclusion list)
00:27:40.15 +64:55:42.0 -- not an asteroid (will add it to exclusion list)
00:10:35.06 +59:42:25.3 -- not an asteroid (will add it to exclusion list)
00:11:06.41 +63:53:48.0 -- not an asteroid (will add it to exclusion list)
00:07:31.54 +62:23:56.3 -- not an asteroid (will add it to exclusion list)
00:41:03.00 +65:48:58.1 -- not an asteroid (will add it to exclusion list)
00:05:59.75 +64:46:53.0 -- not an asteroid (will add it to exclusion list)
23:44:00.19 +63:59:36.5 -- not an asteroid (will add it to exclusion list)
00:01:08.45 +62:53:36.4 -- not an asteroid (will add it to exclusion list)
00:26:09.80 +66:06:26.9 -- not an asteroid (will add it to exclusion list)
00:07:23.74 +64:28:32.7 -- not an asteroid (will add it to exclusion list)
23:21:47.31 +63:52:52.7 -- not an asteroid (will add it to exclusion list)
00:22:51.43 +66:01:51.6 -- not an asteroid (will add it to exclusion list)
00:11:43.97 +61:21:08.7 -- not an asteroid (will add it to exclusion list)
23:28:06.19 +64:26:26.5 -- not an asteroid (will add it to exclusion list)
00:29:27.82 +60:49:56.1 -- not an asteroid (will add it to exclusion list)
23:29:21.47 +63:22:22.0 -- not an asteroid (will add it to exclusion list)
00:07:40.74 +64:42:27.6 -- not an asteroid (will add it to exclusion list)
23:58:36.89 +58:25:46.5 -- not an asteroid (will add it to exclusion list)
23:51:07.26 +62:08:50.7 -- not an asteroid (will add it to exclusion list)
23:29:38.03 +64:59:16.0 -- not an asteroid (will add it to exclusion list)
00:07:05.62 +61:48:59.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:30.07 +65:48:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:08.45 +62:53:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:54.79 +63:10:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:05.43 +63:18:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:34.67 +63:34:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:33.49 +58:31:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:11.91 +60:11:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:21.04 +63:24:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:24.33 +57:58:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:33.91 +62:32:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:59.75 +64:46:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:31.54 +62:21:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:39.88 +63:07:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:05.62 +61:48:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:23.74 +64:28:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:31.54 +62:23:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:40.74 +64:42:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:55.37 +63:41:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:40.94 +63:50:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:15.91 +59:38:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:20.47 +58:03:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:18.81 +64:39:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:26.03 +60:01:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:35.06 +59:42:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:44.24 +59:41:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:45.53 +63:25:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:06.41 +63:53:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:14.79 +64:53:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:16.41 +59:58:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:38.65 +62:49:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:43.97 +61:21:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:48.28 +61:45:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:01.75 +57:56:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:19.82 +60:34:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:27.40 +60:10:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:40.51 +62:31:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:55.02 +58:40:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:02.46 +61:26:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:05.59 +63:31:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:46.09 +64:49:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:22.75 +61:54:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:47.03 +64:42:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:26.19 +61:52:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:56.90 +59:09:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:06.59 +63:05:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:49.80 +59:41:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:13.59 +63:35:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:24.93 +59:23:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:28.24 +63:28:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:42.27 +58:20:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:42.97 +62:52:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:17.66 +58:09:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:41.13 +62:06:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:47.25 +61:02:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:54.61 +64:21:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:56.58 +61:46:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:02.50 +62:11:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:06.77 +63:58:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:10.68 +64:32:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:14.89 +61:43:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:22.12 +59:28:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:51.43 +66:01:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:26.38 +62:17:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:31.32 +65:19:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:45.07 +59:32:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:54.03 +60:22:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:08.36 +62:24:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:10.80 +62:20:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:21.98 +59:46:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:52.06 +58:40:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:09.80 +66:06:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:06.32 +61:13:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:25.45 +62:36:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:40.15 +64:55:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:07.31 +63:12:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:27.63 +63:43:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:42.73 +63:24:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:27.82 +60:49:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:41.19 +62:45:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:23.15 +60:12:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:54.68 +63:26:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:04.23 +58:32:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:03.42 +58:44:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:04.74 +63:10:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:46.68 +59:50:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:36.24 +62:38:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:15.80 +63:00:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:08.60 +62:39:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:09.90 +62:54:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:20.85 +62:40:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:45.62 +64:16:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:03.00 +65:48:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:22.76 +64:38:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:47.31 +63:52:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:11.05 +63:45:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:39.94 +64:41:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:47.03 +63:17:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:49.11 +57:25:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:18.12 +57:37:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:59.12 +64:37:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:44.47 +57:32:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:06.19 +64:26:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:12.92 +63:48:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:21.47 +63:22:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:38.03 +64:59:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:17.78 +64:29:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:23.33 +64:09:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:14.94 +65:40:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:11.08 +58:56:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:00.19 +63:59:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:16.65 +61:58:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:26.64 +61:51:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:59.54 +61:59:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:28.29 +63:40:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:52.99 +61:40:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:54.64 +64:22:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:37.36 +61:05:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:13.48 +61:49:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:07.26 +62:08:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:13.16 +65:38:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:09.74 +62:18:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:02.91 +64:01:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:08.88 +62:13:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:29.51 +63:50:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:36.89 +58:25:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:12.50 +63:48:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:00:30.07 +65:48:26.1 -- not a known variable star
00:01:08.45 +62:53:36.4 -- a known variable star
00:01:54.79 +63:10:51.2 -- a known variable star
00:02:05.43 +63:18:21.2 -- not a known variable star
00:03:34.67 +63:34:49.5 -- a known variable star
00:04:33.49 +58:31:26.0 -- not a known variable star
00:05:11.91 +60:11:01.0 -- not a known variable star
00:05:21.04 +63:24:15.2 -- not a known variable star
00:05:24.33 +57:58:25.5 -- not a known variable star
00:05:33.91 +62:32:06.1 -- not a known variable star
00:05:59.75 +64:46:53.0 -- not a known variable star
00:06:31.54 +62:21:03.3 -- not a known variable star
00:06:39.88 +63:07:45.2 -- a known variable star
00:07:05.62 +61:48:59.6 -- a known variable star
00:07:23.74 +64:28:32.7 -- not a known variable star
00:07:31.54 +62:23:56.3 -- not a known variable star
00:07:40.74 +64:42:27.6 -- not a known variable star
00:07:55.37 +63:41:10.3 -- not a known variable star
00:08:40.94 +63:50:28.9 -- not a known variable star
00:09:15.91 +59:38:43.9 -- not a known variable star
00:09:20.47 +58:03:30.0 -- a known variable star
00:10:18.81 +64:39:19.4 -- not a known variable star
00:10:26.03 +60:01:06.4 -- not a known variable star
00:10:35.06 +59:42:25.3 -- not a known variable star
00:10:44.24 +59:41:51.2 -- not a known variable star
00:10:45.53 +63:25:28.5 -- not a known variable star
00:11:06.41 +63:53:48.0 -- not a known variable star
00:11:14.79 +64:53:31.2 -- not a known variable star
00:11:16.41 +59:58:35.0 -- a known variable star
00:11:38.65 +62:49:32.6 -- not a known variable star
00:11:43.97 +61:21:08.7 -- not a known variable star
00:11:48.28 +61:45:47.8 -- not a known variable star
00:12:01.75 +57:56:55.7 -- not a known variable star
00:12:19.82 +60:34:41.4 -- a known variable star
00:12:27.40 +60:10:24.0 -- a known variable star
00:13:40.51 +62:31:06.5 -- not a known variable star
00:14:55.02 +58:40:52.3 -- not a known variable star
00:15:02.46 +61:26:05.2 -- not a known variable star
00:15:05.59 +63:31:33.7 -- not a known variable star
00:15:46.09 +64:49:40.7 -- not a known variable star
00:16:22.75 +61:54:20.3 -- a known variable star
00:16:47.03 +64:42:55.0 -- not a known variable star
00:17:26.19 +61:52:46.3 -- not a known variable star
00:17:56.90 +59:09:20.5 -- a known variable star
00:18:06.59 +63:05:08.4 -- not a known variable star
00:18:49.80 +59:41:44.4 -- not a known variable star
00:19:13.59 +63:35:39.0 -- not a known variable star
00:19:24.93 +59:23:46.2 -- not a known variable star
00:20:28.24 +63:28:45.2 -- a known variable star
00:20:42.27 +58:20:31.5 -- not a known variable star
00:20:42.97 +62:52:57.8 -- not a known variable star
00:21:17.66 +58:09:09.5 -- not a known variable star
00:21:41.13 +62:06:54.0 -- a known variable star
00:21:47.25 +61:02:51.3 -- not a known variable star
00:21:54.61 +64:21:30.0 -- not a known variable star
00:21:56.58 +61:46:06.5 -- a known variable star
00:22:02.50 +62:11:52.6 -- a known variable star
00:22:06.77 +63:58:51.2 -- not a known variable star
00:22:10.68 +64:32:05.5 -- not a known variable star
00:22:14.89 +61:43:13.6 -- not a known variable star
00:22:22.12 +59:28:19.3 -- not a known variable star
00:22:51.43 +66:01:51.6 -- not a known variable star
00:23:26.38 +62:17:45.0 -- a known variable star
00:23:31.32 +65:19:48.0 -- not a known variable star
00:23:45.07 +59:32:01.1 -- a known variable star
00:23:54.03 +60:22:48.1 -- not a known variable star
00:24:08.36 +62:24:35.2 -- not a known variable star
00:24:10.80 +62:20:28.7 -- not a known variable star
00:24:21.98 +59:46:31.8 -- not a known variable star
00:24:52.06 +58:40:49.6 -- not a known variable star
00:26:09.80 +66:06:26.9 -- not a known variable star
00:27:06.32 +61:13:07.6 -- not a known variable star
00:27:25.45 +62:36:32.8 -- not a known variable star
00:27:40.15 +64:55:42.0 -- not a known variable star
00:28:07.31 +63:12:32.5 -- not a known variable star
00:28:27.63 +63:43:01.9 -- not a known variable star
00:28:42.73 +63:24:32.8 -- not a known variable star
00:29:27.82 +60:49:56.1 -- a known variable star
00:29:41.19 +62:45:12.3 -- not a known variable star
00:30:23.15 +60:12:42.8 -- not a known variable star
00:30:54.68 +63:26:03.2 -- not a known variable star
00:31:04.23 +58:32:51.9 -- not a known variable star
00:32:03.42 +58:44:20.9 -- not a known variable star
00:32:04.74 +63:10:05.9 -- a known variable star
00:32:46.68 +59:50:59.1 -- not a known variable star
00:34:36.24 +62:38:19.3 -- not a known variable star
00:35:15.80 +63:00:42.3 -- not a known variable star
00:36:08.60 +62:39:27.6 -- not a known variable star
00:36:09.90 +62:54:05.0 -- not a known variable star
00:36:20.85 +62:40:04.6 -- a known variable star
00:40:45.62 +64:16:36.7 -- not a known variable star
00:41:03.00 +65:48:58.1 -- not a known variable star
00:41:22.76 +64:38:36.1 -- not a known variable star
23:21:47.31 +63:52:52.7 -- not a known variable star
23:23:11.05 +63:45:18.2 -- not a known variable star
23:24:39.94 +64:41:36.4 -- not a known variable star
23:24:47.03 +63:17:45.8 -- not a known variable star
23:24:49.11 +57:25:54.6 -- not a known variable star
23:25:18.12 +57:37:12.1 -- not a known variable star
23:26:59.12 +64:37:21.5 -- not a known variable star
23:27:44.47 +57:32:13.4 -- not a known variable star
23:28:06.19 +64:26:26.5 -- not a known variable star
23:28:12.92 +63:48:23.1 -- not a known variable star
23:29:21.47 +63:22:22.0 -- a known variable star
23:29:38.03 +64:59:16.0 -- not a known variable star
23:30:17.78 +64:29:51.3 -- not a known variable star
23:30:23.33 +64:09:25.2 -- not a known variable star
23:34:14.94 +65:40:48.1 -- not a known variable star
23:42:11.08 +58:56:31.9 -- a known variable star
23:44:00.19 +63:59:36.5 -- not a known variable star
23:44:16.65 +61:58:50.3 -- not a known variable star
23:44:26.64 +61:51:10.5 -- not a known variable star
23:44:59.54 +61:59:31.2 -- not a known variable star
23:46:28.29 +63:40:33.6 -- not a known variable star
23:48:52.99 +61:40:27.3 -- not a known variable star
23:48:54.64 +64:22:28.6 -- not a known variable star
23:49:37.36 +61:05:24.8 -- a known variable star
23:50:13.48 +61:49:47.5 -- not a known variable star
23:51:07.26 +62:08:50.7 -- not a known variable star
23:52:13.16 +65:38:35.1 -- not a known variable star
23:53:09.74 +62:18:07.4 -- not a known variable star
23:54:02.91 +64:01:04.1 -- not a known variable star
23:55:08.88 +62:13:12.1 -- not a known variable star
23:58:29.51 +63:50:02.4 -- not a known variable star
23:58:36.89 +58:25:46.5 -- a known variable star
23:59:12.50 +63:48:15.4 -- not a known variable star
Found 102 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
126 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 126 (excluding asteroids and hot pixels, 102 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)2461211.91855711 -observatory V36
07:37:51.00 +21:39:49.4 Mercury (0.9mag)
08:42:40.11 +20:15:57.8 Venus (-4.0mag)
03:25:19.45 +18:15:41.8 Mars (1.3mag)
07:58:52.59 +21:03:59.4 Jupiter (-1.8mag)
00:52:29.60 +03:05:09.7 Saturn (0.8mag)
04:03:02.90 +20:33:31.9 Uranus (5.8mag)
00:16:43.07 +00:19:50.9 Neptune (7.8mag)
20:32:34.29 -23:09:23.7 Pluto (14.5mag)
10:45:43.71 +06:15:04.8 Moon (-9.9mag)
-rw-r--r-- 1 apache apache 361 Jun 20 06:36 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461211.91855711:
07:58:50.06 +21:04:09.5 Io (6.2mag)
07:58:58.60 +21:03:38.8 Europa (6.3mag)
07:59:00.39 +21:03:30.0 Ganymede (5.6mag)
07:59:15.55 +21:02:50.4 Callisto (6.9mag)
07:58:26.73 +20:41:57.3 Himalia (15.6mag)
07:58:56.55 +21:03:46.1 Thebe (16.6mag)
07:58:06.37 +20:52:23.0 Elara (17.6mag)
08:01:38.83 +21:09:00.1 Pasiphae (17.8mag)
08:04:53.68 +21:06:43.9 Carme (18.9mag)
00:52:23.90 +03:05:38.5 Titan (8.6mag)
00:52:34.16 +03:05:13.5 Rhea (9.9mag)
00:52:43.42 +03:07:32.4 Iapetus (11.3mag)
00:52:32.94 +03:05:38.0 Hyperion (14.6mag)
00:52:56.51 +03:05:19.4 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jun 20 06:36 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461211.91855711:
17:28:22.32 -35:30:05.4 JWST
18:33:54.68 +21:25:44.8 Chandra
04:06:56.69 +56:08:46.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 20 06:36 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461211.91855711 -observatory V36
18:34:15.15 -33:28:18.7 13.6mag P/2010 H2 (Vales)
06:05:38.02 -67:59:41.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:53:35.22 +32:08:08.2 17.6mag C/2017 K2 (PANSTARRS)
17:09:54.05 +15:49:48.0 17.9mag C/2021 G2 (ATLAS)
23:13:40.55 -35:57:29.2 15.9mag P/2021 N1 (ZTF)
23:09:04.82 +31:59:51.6 17.2mag C/2022 E2 (ATLAS)
05:48:55.56 +27:00:44.3 16.6mag C/2022 N2 (PANSTARRS)
09:38:56.96 +30:37:32.4 16.7mag C/2022 QE78 (ATLAS)
08:57:25.18 +04:26:47.5 17.7mag C/2022 R6 (PANSTARRS)
18:20:07.40 +21:42:10.2 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:15:27.24 -11:04:21.5 17.6mag P/2023 B1 (PANSTARRS)
22:08:14.69 +67:11:00.4 17.8mag C/2023 H5 (Lemmon)
17:15:59.46 -07:56:43.0 13.7mag C/2023 R1 (PANSTARRS)
13:17:38.81 +80:07:18.2 18.0mag C/2023 X2 (Lemmon)
07:28:13.76 +64:45:56.8 17.8mag C/2024 A1 (ATLAS)
07:05:21.86 +28:48:33.8 14.0mag C/2024 E1 (Wierzchos)
15:28:12.52 +14:26:42.3 17.4mag C/2024 G6 (ATLAS)
20:03:22.27 +34:38:20.6 13.9mag C/2024 J3 (ATLAS)
04:30:14.66 -14:58:24.9 15.9mag C/2024 T5 (ATLAS)
06:17:10.90 +32:23:58.9 17.9mag C/2025 J1 (Borisov)
11:32:04.40 +52:00:03.5 17.8mag C/2025 L1 (ATLAS)
06:58:03.19 -11:28:35.3 15.2mag C/2025 R3 (PANSTARRS)
09:35:00.96 +23:06:28.4 17.8mag C/2025 V2 (Rankin)
12:40:13.33 +04:33:13.1 17.1mag C/2025 Y1 (ATLAS)
17:48:11.45 +77:23:31.8 17.7mag C/2026 A2 (Bok)
02:20:30.26 +44:12:52.7 16.3mag C/2026 B2 (Sun-Gao)
11:15:03.51 +00:05:05.4 16.7mag A/2026 E1
20:45:30.36 -09:58:11.0 8.1mag 10P/Tempel
11:05:28.03 -01:12:36.1 16.0mag 29P/Schwassmann-Wachmann
03:30:30.65 +27:13:32.0 17.7mag 47P/Ashbrook-Jackson
09:26:01.90 +20:11:13.9 16.9mag 63P/Wild
00:36:37.37 -05:41:18.7 15.6mag 65P/Gunn
07:23:10.82 +34:17:50.0 17.2mag 76P/West-Kohoutek-Ikemura
03:38:52.15 +18:37:22.5 13.8mag 78P/Gehrels
01:46:11.59 +07:20:07.7 15.8mag 88P/Howell
05:33:50.24 +30:54:00.6 15.4mag 93P/Lovas
03:18:36.48 +29:22:59.3 17.3mag 114P/Wiseman-Skiff
07:20:00.11 +32:25:48.5 15.5mag 123P/West-Hartley
10:11:45.10 +09:26:44.5 16.6mag 124P/Mrkos
04:19:12.36 +19:59:10.1 16.3mag 128P/Shoemaker-Holt
04:57:45.39 +19:31:27.1 17.8mag 131P/Mueller
06:47:39.42 +16:55:51.6 16.2mag 141P/Machholz
06:51:14.98 +17:52:18.8 16.1mag 141P-A/Machholz
05:53:15.69 +17:17:31.3 13.0mag 141P-D/Machholz
03:05:55.94 -23:07:41.0 16.4mag 161P/Hartley-IRAS
04:22:39.91 +28:20:59.9 15.0mag 162P/SidingSpring
19:32:29.50 +05:44:46.9 16.2mag 169P/NEAT
00:50:49.82 +04:43:10.1 17.8mag 220P/McNaught
16:43:40.73 -08:06:00.0 16.6mag 235P/LINEAR
08:02:03.84 +34:51:02.7 17.7mag 240P/NEAT
01:04:45.51 +02:53:02.5 16.1mag 260P/McNaught
04:38:19.99 +34:30:40.4 17.5mag 295P/LINEAR
00:55:40.05 +03:21:46.1 17.9mag 320P/McNaught
15:10:28.81 +07:32:00.2 17.5mag 391P/Kowalski
08:17:11.08 +20:23:45.7 17.9mag 450P/LONEOS
07:19:52.38 +40:47:56.9 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 20 06:36 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -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
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.18 +22:02:03.40 AT2026lxf 2026-05-8.07 13.94
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:49:13.39 +25:17:59.20 2026-06-15.39 15.93
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:49:13.39 +25:17:59.20 2026-06-15.39 15.93
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
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
19:32:43.68 -22:39:32.70 ASASSN-26cm 2026-04-4.27 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
-rw-r--r-- 1 apache apache 5.6K Jun 20 06:36 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:43:38.36 +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
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
-rw-r--r-- 1 apache apache 189K Jun 20 06:36 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:46:06.891 +33:41:13.54 AT 2026oyn 2026-06-03.92 19.91
22:04:59.426 +17:15:40.14 AT 2026oym 2026-06-09.20 19.68
15:19:51.792 +48:33:17.32 AT 2026oyl 2026-06-09.90 20.47
21:06:36.637 +12:42:18.62 AT 2026oyk 2026-06-10.12 19.64
13:35:55.780 +35:23:15.20 AT 2026oyj 2026-05-24.78 21.27
18:33:47.510 +37:36:07.65 AT 2026oyi 2026-05-10.79 21.55
18:14:44.150 +51:46:11.54 AT 2026oyh 2026-05-08.79 22.03
15:07:33.090 +20:01:11.55 AT 2026oyg 2026-05-07.82 21.15
13:35:40.460 -01:57:01.30 AT 2026oyf 2026-05-22.68 22.32
10:26:08.380 +04:26:57.22 AT 2026oye 2026-05-22.61 21.23
14:00:27.900 -01:28:05.40 AT 2026oyd 2026-06-02.72 21
13:47:00.850 +01:08:03.86 AT 2026oyc 2026-06-02.72 20.42
14:34:07.980 +03:43:00.64 AT 2026oyb 2026-05-25.68 21.54
13:48:38.410 +04:03:32.72 AT 2026oya 2026-05-09.68 22.13
00:38:19.802 -05:15:31.84 AT 2026oxz 2026-06-08.47 19.6034
14:39:23.496 +35:21:27.84 AT 2026oxy 2026-06-04.97 20.13
23:44:57.556 +04:18:42.85 SN 2026oxx 2026-06-11.15 19.97
15:19:13.587 +27:52:58.57 SN 2026oxw 2026-06-11.02 19.96
09:53:09.311 +42:13:35.56 AT 2026oxv 2026-06-10.17 19.7446
20:30:02.168 +37:49:06.79 AT 2026oxu 2026-06-10.94 19.78
-rw-r--r-- 1 apache apache 30K Jun 20 06:36 tns_transients_list.txt
