This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM
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 20.4200 2461211.9200 8.81 01:56:38.04 +59:15:34.2
131.18803 -2.56317 galactic Cas Second-epoch detections are separated by 0.4" and 3.5 pix
The object was found in VSX 1" X Cas
Type: M
# Max. Min./Amp. JD0 Period
9.450 V 13.200 V 2457020.00000 415.000000000000 C5,4e(N1e)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.04 +59:15:34.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.04 +59:15:34.2: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 56 38.04 +59 15 34.2 8.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
X Cas,2461211.9200,8.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
X Cas 20260620.4200 8.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 12.09 01:50:16.38 +58:52:59.7
130.48298 -3.12324 galactic Cas Second-epoch detections are separated by 3.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:50:16.38 +58:52:59.7 (user input) | T | P | (position from user input) J-Ks=0.292+/-0.045 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:16.38 +58:52:59.7: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:16.38 +58:52:59.7: 14.85 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.85 +/- 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 20.4200* 01 50 16.38 +58 52 59.7 12.1 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,2461211.9200,12.09,0.05,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 20260620.4200 12.09CV 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 20.4200 2461211.9200 12.13 01:43:24.12 +61:12:07.8
129.14970 -1.04069 galactic Cas Second-epoch detections are separated by 2.1" and 3.7 pix
The object was found in VSX 0" Gaia DR3 511249649679966976
Type: ROT
# Max. Min./Amp. JD0 Period
14.700 G 14.730 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:24.12 +61:12:07.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:24.12 +61:12:07.8: 14.85 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.85 +/- 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 20.4200* 01 43 24.12 +61 12 07.8 12.1 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 511249649679966976,2461211.9200,12.13,0.05,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
Gaia DR3 511249649679966976 20260620.4200 12.13CV 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 20.4200 2461211.9200 12.09 01:16:40.37 +61:23:05.9
125.94942 -1.33884 galactic Cas Second-epoch detections are separated by 2.2" and 3.7 pix
The object was found in VSX12" Gaia DR3 510578015567649792
Type: E
# Max. Min./Amp. JD0 Period
18.250 G 18.560 G 3.284190000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:40.37 +61:23:05.9: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:40.37 +61:23:05.9: 14.53 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.53 +/- 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 20.4200* 01 16 40.37 +61 23 05.9 12.1 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 510578015567649792,2461211.9200,12.09,0.05,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
Gaia DR3 510578015567649792 20260620.4200 12.09CV 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 20.4200 2461211.9200 12.06 01:15:30.43 +60:45:22.6
125.86916 -1.97813 galactic Cas Second-epoch detections are separated by 2.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:15:30.43 +60:45:22.6 (user input) | T | P | (position from user input) J-Ks=0.401+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:30.43 +60:45:22.6: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:30.43 +60:45:22.6: 14.56 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.56 +/- 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 20.4200* 01 15 30.43 +60 45 22.6 12.1 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,2461211.9200,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.98 01:24:06.20 +60:41:09.9
126.92209 -1.93235 galactic Cas Second-epoch detections are separated by 0.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:24:06.20 +60:41:09.9 (user input) | T | P | (position from user input) J-Ks=0.246+/-0.047 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:06.20 +60:41:09.9: 12.62 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:06.20 +60:41:09.9: 14.98 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.24 +/- 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 20.4200* 01 24 06.20 +60 41 09.9 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,2461211.9200,11.98,0.05,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 20260620.4200 11.98CV 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 20.4200 2461211.9200 11.93 01:33:22.88 +61:41:09.1
127.88432 -0.78192 galactic Cas Second-epoch detections are separated by 2.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:33:22.88 +61:41:09.1 (user input) | T | P | (position from user input) J-Ks=0.299+/-0.041 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:22.88 +61:41:09.1: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:22.88 +61:41:09.1: 14.61 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.61 +/- 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 20.4200* 01 33 22.88 +61 41 09.1 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
target,2461211.9200,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.91 01:30:06.40 +63:44:41.8
127.19296 1.19357 galactic Cas Second-epoch detections are separated by 3.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:30:06.40 +63:44:41.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:06.40 +63:44:41.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:06.40 +63:44:41.8: 14.86 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 30 06.40 +63 44 41.8 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
target,2461211.9200,11.91,0.05,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 20260620.4200 11.91CV 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 20.4200 2461211.9200 11.81 01:07:06.59 +57:40:47.8
125.03391 -5.12783 galactic Cas Second-epoch detections are separated by 2.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J016.7783+57.6795 | 01:07:06.59 +57:40:47.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.319+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:06.59 +57:40:47.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:06.59 +57:40:47.8: 14.29 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.29 +/- 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 20.4200* 01 07 06.59 +57 40 47.8 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J016.7783+57.6795,2461211.9200,11.81,0.05,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
ATO J016.7783+57.6795 20260620.4200 11.81CV 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 20.4200 2461211.9200 11.71 01:16:23.35 +58:49:28.1
126.16378 -3.89062 galactic Cas Second-epoch detections are separated by 3.1" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J019.0953+58.8254 | 01:16:23.35 +58:49:28.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:23.35 +58:49:28.1: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:23.35 +58:49:28.1: 14.63 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.63 +/- 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 20.4200* 01 16 23.35 +58 49 28.1 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J019.0953+58.8254,2461211.9200,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J019.0953+58.8254 20260620.4200 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.88 01:34:46.03 +62:04:51.5
127.98033 -0.36532 galactic Cas Second-epoch detections are separated by 2.7" and 3.7 pix
The object was found in VSX20" Gaia DR3 512286935820114304
Type: ROT
# Max. Min./Amp. JD0 Period
13.230 G 13.260 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:46.03 +62:04:51.5: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:46.03 +62:04:51.5: 14.36 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 34 46.03 +62 04 51.5 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512286935820114304,2461211.9200,11.88,0.05,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 512286935820114304 20260620.4200 11.88CV 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 20.4200 2461211.9200 11.80 01:07:33.61 +61:22:51.8
124.86186 -1.43026 galactic Cas Second-epoch detections are separated by 1.3" and 3.4 pix
The object was found in VSX 2" Gaia DR3 522528916687681024
Type: ROT
# Max. Min./Amp. JD0 Period
14.690 G 14.710 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:33.61 +61:22:51.8: 12.38 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:33.61 +61:22:51.8: 14.91 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 07 33.61 +61 22 51.8 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522528916687681024,2461211.9200,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522528916687681024 20260620.4200 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.76 01:34:30.25 +59:54:23.8
128.31175 -2.51453 galactic Cas Second-epoch detections are separated by 0.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 509394567397570560 | 01:34:30.25 +59:54:23.8 (user input) | 2021A&A...648A..44M | | (position from user input) (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=0.181+/-0.050 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:30.25 +59:54:23.8: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:30.25 +59:54:23.8: 14.58 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.58 +/- 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 20.4200* 01 34 30.25 +59 54 23.8 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 509394567397570560,2461211.9200,11.76,0.05,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
Large-amplitude variable Gaia DR2 509394567397570560 20260620.4200 11.76CV 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 20.4200 2461211.9200 11.77 01:53:04.68 +62:00:26.5
130.09651 -0.00391 galactic Cas Second-epoch detections are separated by 2.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:53:04.68 +62:00:26.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:53:04.68 +62:00:26.5: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:53:04.68 +62:00:26.5: 14.34 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.34 +/- 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 20.4200* 01 53 04.68 +62 00 26.5 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.90 01:26:38.72 +62:48:30.9
126.94155 0.21125 galactic Cas Second-epoch detections are separated by 2.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:26:38.72 +62:48:30.9 (user input) | T | P | (position from user input) J-Ks=0.398+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:38.72 +62:48:30.9: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:38.72 +62:48:30.9: 14.28 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 26 38.72 +62 48 30.9 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
target,2461211.9200,11.90,0.05,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 20260620.4200 11.90CV 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 20.4200 2461211.9200 11.69 01:46:36.58 +64:06:19.3
128.91157 1.87602 galactic Cas Second-epoch detections are separated by 2.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 512224298010737152 | 01:46:36.58 +64:06:19.3 (user input) | 2021A&A...648A..44M | | (position from user input) (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=0.862+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:36.58 +64:06:19.3: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:36.58 +64:06:19.3: 14.29 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.29 +/- 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 20.4200* 01 46 36.58 +64 06 19.3 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 512224298010737152,2461211.9200,11.69,0.05,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
Large-amplitude variable Gaia DR2 512224298010737152 20260620.4200 11.69CV 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 20.4200 2461211.9200 11.71 01:22:13.69 +62:32:56.6
126.47200 -0.11087 galactic Cas Second-epoch detections are separated by 1.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:22:13.69 +62:32:56.6 (user input) | T | P | (position from user input) J-Ks=0.475+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:13.69 +62:32:56.6: 11.76 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:13.69 +62:32:56.6: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.31 +/- 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 20.4200* 01 22 13.69 +62 32 56.6 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.90 01:49:40.08 +59:34:16.8
130.25241 -2.47023 galactic Cas Second-epoch detections are separated by 2.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:49:40.08 +59:34:16.8 (user input) | T | P | (position from user input) J-Ks=0.643+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:40.08 +59:34:16.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:40.08 +59:34:16.8: 14.79 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.79 +/- 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 20.4200* 01 49 40.08 +59 34 16.8 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
target,2461211.9200,11.90,0.05,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 20260620.4200 11.90CV 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 20.4200 2461211.9200 11.54 01:12:01.47 +58:29:48.8
125.62611 -4.26713 galactic Cas Second-epoch detections are separated by 1.4" and 3.3 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 J017.9864+58.4978 | 01:12:01.47 +58:29:48.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.138+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:01.47 +58:29:48.8: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:01.47 +58:29:48.8: 14.29 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.29 +/- 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 20.4200* 01 12 01.47 +58 29 48.8 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.9864+58.4978,2461211.9200,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.9864+58.4978 20260620.4200 11.54CV 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 20.4200 2461211.9200 11.69 01:08:47.54 +57:50:27.2
125.24831 -4.95279 galactic Cas Second-epoch detections are separated by 1.7" and 3.8 pix
The object was found in VSX23" Gaia DR3 413608859605619200
Type: ROT
# Max. Min./Amp. JD0 Period
13.580 G 13.640 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:47.54 +57:50:27.2: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:47.54 +57:50:27.2: 14.52 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 08 47.54 +57 50 27.2 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413608859605619200,2461211.9200,11.69,0.05,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 413608859605619200 20260620.4200 11.69CV 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 20.4200 2461211.9200 11.78 01:33:40.63 +59:42:23.5
128.24210 -2.72902 galactic Cas Second-epoch detections are separated by 2.3" and 3.6 pix
The object was found in VSX 1" ZTF J013340.67+594224.0
Type: SR
# Max. Min./Amp. JD0 Period
16.002 g Y 0.134 g 2458302.89690 31.071577300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:40.63 +59:42:23.5: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:40.63 +59:42:23.5: 14.44 +/- 0.08 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 20.4200* 01 33 40.63 +59 42 23.5 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J013340.67+594224.0,2461211.9200,11.78,0.05,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
ZTF J013340.67+594224.0 20260620.4200 11.78CV 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 20.4200 2461211.9200 11.80 01:55:28.44 +63:18:55.9
130.04822 1.33198 galactic Cas Second-epoch detections are separated by 2.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:55:28.44 +63:18:55.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:28.44 +63:18:55.9: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:28.44 +63:18:55.9: 14.48 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.48 +/- 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 20.4200* 01 55 28.44 +63 18 55.9 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.77 02:14:26.26 +61:46:49.0
132.57634 0.47261 galactic Cas Second-epoch detections are separated by 5.1" and 2.8 pix
The object was found in VSX18" Gaia DR3 513768149778941568
Type: ROT
# Max. Min./Amp. JD0 Period
13.820 G 13.850 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:26.26 +61:46:49.0: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:14:26.26 +61:46:49.0: 14.47 +/- 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!
TCP 2026 06 20.4200* 02 14 26.26 +61 46 49.0 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 513768149778941568,2461211.9200,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 513768149778941568 20260620.4200 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.80 01:25:02.98 +65:27:16.3
126.41646 2.81043 galactic Cas Second-epoch detections are separated by 2.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:25:02.98 +65:27:16.3 (user input) | T | P | (position from user input) J-Ks=1.021+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:02.98 +65:27:16.3: 12.04 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:02.98 +65:27:16.3: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 25 02.98 +65 27 16.3 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.44 01:25:57.02 +58:48:08.8
127.39850 -3.76968 galactic Cas Second-epoch detections are separated by 0.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:25:57.02 +58:48:08.8 (user input) | T | P | (position from user input) J-Ks=0.454+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:57.02 +58:48:08.8: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:57.02 +58:48:08.8: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 25 57.02 +58 48 08.8 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.54 01:32:22.31 +62:14:57.8
127.67704 -0.24464 galactic Cas Second-epoch detections are separated by 3.0" and 3.2 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 512303600292886912 | 01:32:27.38 +62:14:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1960IzKry..24..160B [B60] +61 285
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:22.31 +62:14:57.8: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:22.31 +62:14:57.8: 14.28 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 32 22.31 +62 14 57.8 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512303600292886912,2461211.9200,11.54,0.05,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 512303600292886912 20260620.4200 11.54CV 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 20.4200 2461211.9200 11.61 01:39:10.54 +58:03:36.0
129.22982 -4.22682 galactic Cas Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:39:10.54 +58:03:36.0 (user input) | T | P | (position from user input) J-Ks=0.470+/-0.037 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:10.54 +58:03:36.0: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:10.54 +58:03:36.0: 14.25 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 39 10.54 +58 03 36.0 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.61,0.05,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
target 20260620.4200 11.61CV 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 20.4200 2461211.9200 11.66 01:32:25.36 +61:29:15.7
127.80348 -0.99579 galactic Cas Second-epoch detections are separated by 0.9" and 3.3 pix
The object was found in VSX14" Gaia DR3 510746485668934272
Type: ROT
# Max. Min./Amp. JD0 Period
15.470 G 15.520 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:25.36 +61:29:15.7: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:25.36 +61:29:15.7: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 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 20.4200* 01 32 25.36 +61 29 15.7 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510746485668934272,2461211.9200,11.66,0.05,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 510746485668934272 20260620.4200 11.66CV 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 20.4200 2461211.9200 11.66 01:04:35.20 +62:44:33.3
124.43676 -0.09074 galactic Cas Second-epoch detections are separated by 2.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:04:35.20 +62:44:33.3 (user input) | T | P | (position from user input) J-Ks=1.374+/-0.143 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:04:35.20 +62:44:33.3: 11.75 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:04:35.20 +62:44:33.3: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 04 35.20 +62 44 33.3 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.66CV 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 20.4200 2461211.9200 11.56 01:34:59.27 +60:09:34.6
128.32898 -2.25499 galactic Cas Second-epoch detections are separated by 0.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J023.7486+60.1542 | 01:34:59.27 +60:09:34.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.509+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:59.27 +60:09:34.6: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:59.27 +60:09:34.6: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 20.4200* 01 34 59.27 +60 09 34.6 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J023.7486+60.1542,2461211.9200,11.56,0.05,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
ATO J023.7486+60.1542 20260620.4200 11.56CV 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 20.4200 2461211.9200 11.45 01:06:15.89 +57:53:25.3
124.90851 -4.92447 galactic Cas Second-epoch detections are separated by 1.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J016.5720+57.8855 | 01:06:15.89 +57:53:25.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.781+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:15.89 +57:53:25.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:15.89 +57:53:25.3: 14.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.19 +/- 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 20.4200* 01 06 15.89 +57 53 25.3 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J016.5720+57.8855,2461211.9200,11.45,0.05,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
ATO J016.5720+57.8855 20260620.4200 11.45CV 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 20.4200 2461211.9200 11.62 01:30:59.89 +63:14:37.6
127.36707 0.71320 galactic Cas Second-epoch detections are separated by 0.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:30:59.89 +63:14:37.6 (user input) | T | P | (position from user input) J-Ks=0.876+/-0.036 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:59.89 +63:14:37.6: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:59.89 +63:14:37.6: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 30 59.89 +63 14 37.6 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.49 01:48:13.35 +59:51:32.6
130.01084 -2.22994 galactic Cas Second-epoch detections are separated by 2.9" and 3.4 pix
The object was found in VSX18" Gaia DR3 506602151467215616
Type: ROT
# Max. Min./Amp. JD0 Period
13.340 G 13.380 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:13.35 +59:51:32.6: 12.94 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:13.35 +59:51:32.6: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 20.4200* 01 48 13.35 +59 51 32.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506602151467215616,2461211.9200,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506602151467215616 20260620.4200 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.52 01:12:41.26 +61:18:08.1
125.48091 -1.46429 galactic Cas Second-epoch detections are separated by 0.3" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:41.26 +61:18:08.1 (user input) | T | P | (position from user input) J-Ks=0.156+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:41.26 +61:18:08.1: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:41.26 +61:18:08.1: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 12 41.26 +61 18 08.1 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.37 01:45:19.33 +61:13:08.4
129.37264 -0.97711 galactic Cas Second-epoch detections are separated by 3.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:45:19.33 +61:13:08.4 (user input) | T | P | (position from user input) J-Ks=0.262+/-0.042 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:19.33 +61:13:08.4: 12.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:19.33 +61:13:08.4: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 45 19.33 +61 13 08.4 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.37,0.05,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 20260620.4200 11.37CV 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 20.4200 2461211.9200 11.46 01:37:23.81 +59:20:12.3
128.77054 -3.01300 galactic Cas Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:37:23.81 +59:20:12.3 (user input) | T | P | (position from user input) J-Ks=0.300+/-0.042 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:23.81 +59:20:12.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:23.81 +59:20:12.3: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 37 23.81 +59 20 12.3 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.71 01:52:03.58 +60:31:38.5
130.32479 -1.47131 galactic Cas Second-epoch detections are separated by 3.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:52:03.58 +60:31:38.5 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:03.58 +60:31:38.5: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:03.58 +60:31:38.5: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.17 +/- 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 20.4200* 01 52 03.58 +60 31 38.5 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.56 01:43:20.74 +61:14:37.9
129.13471 -1.00119 galactic Cas Second-epoch detections are separated by 1.1" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:43:20.74 +61:14:37.9 (user input) | T | P | (position from user input) J-Ks=0.323+/-0.037 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:20.74 +61:14:37.9: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:20.74 +61:14:37.9: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 43 20.74 +61 14 37.9 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.56,0.05,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 20260620.4200 11.56CV 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 20.4200 2461211.9200 11.38 01:22:50.56 +58:12:42.7
127.07066 -4.40730 galactic Cas Second-epoch detections are separated by 1.0" and 3.7 pix
The object was found in VSX22" Gaia DR3 413816392424091520
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.040 G 13.070 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:50.56 +58:12:42.7: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:50.56 +58:12:42.7: 14.27 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.27 +/- 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 20.4200* 01 22 50.56 +58 12 42.7 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413816392424091520,2461211.9200,11.38,0.05,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
Gaia DR3 413816392424091520 20260620.4200 11.38CV 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 20.4200 2461211.9200 11.38 01:07:36.88 +58:09:25.4
125.07136 -4.64748 galactic Cas Second-epoch detections are separated by 0.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:36.88 +58:09:25.4 (user input) | T | P | (position from user input) J-Ks=0.277+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:36.88 +58:09:25.4: 12.63 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:36.88 +58:09:25.4: 14.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 07 36.88 +58 09 25.4 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.38,0.05,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 20260620.4200 11.38CV 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 20.4200 2461211.9200 11.60 01:45:15.39 +61:13:52.8
129.36235 -0.96668 galactic Cas Second-epoch detections are separated by 2.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:45:15.39 +61:13:52.8 (user input) | T | P | (position from user input) J-Ks=0.494+/-0.043 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:15.39 +61:13:52.8: 12.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:15.39 +61:13:52.8: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 45 15.39 +61 13 52.8 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.39 01:05:04.67 +63:39:45.2
124.44422 0.83087 galactic Cas Second-epoch detections are separated by 1.7" and 3.5 pix
The object was found in VSX 2" Gaia DR3 523370734583110400
Type: ROT
# Max. Min./Amp. JD0 Period
14.210 G 14.240 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:05:04.67 +63:39:45.2: 13.17 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:04.67 +63:39:45.2: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 05 04.67 +63 39 45.2 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 523370734583110400,2461211.9200,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 523370734583110400 20260620.4200 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.32 01:19:12.21 +60:58:37.9
126.29479 -1.71313 galactic Cas Second-epoch detections are separated by 2.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:19:12.21 +60:58:37.9 (user input) | T | P | (position from user input) J-Ks=0.904+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:12.21 +60:58:37.9: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:12.21 +60:58:37.9: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 19 12.21 +60 58 37.9 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.63 01:36:09.46 +61:08:51.7
128.30181 -1.25694 galactic Cas Second-epoch detections are separated by 3.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:36:09.46 +61:08:51.7 (user input) | T | P | (position from user input) J-Ks=0.600+/-0.040 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:09.46 +61:08:51.7: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:09.46 +61:08:51.7: 14.34 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.34 +/- 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 20.4200* 01 36 09.46 +61 08 51.7 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.63,0.05,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 20260620.4200 11.63CV 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 20.4200 2461211.9200 11.46 01:56:27.23 +65:22:09.4
129.64232 3.34808 galactic Cas Second-epoch detections are separated by 2.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:56:27.23 +65:22:09.4 (user input) | T | P | (position from user input) J-Ks=0.861+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:27.23 +65:22:09.4: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:27.23 +65:22:09.4: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 56 27.23 +65 22 09.4 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.43 01:06:24.44 +60:07:16.0
124.79731 -2.69641 galactic Cas Second-epoch detections are separated by 1.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:24.44 +60:07:16.0 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.029 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:24.44 +60:07:16.0: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:24.44 +60:07:16.0: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 06 24.44 +60 07 16.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.43,0.05,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 20260620.4200 11.43CV 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 20.4200 2461211.9200 11.43 01:22:33.26 +60:44:41.1
126.72676 -1.89752 galactic Cas Second-epoch detections are separated by 3.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:22:33.26 +60:44:41.1 (user input) | T | P | (position from user input) J-Ks=1.158+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:33.26 +60:44:41.1: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:33.26 +60:44:41.1: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 20.4200* 01 22 33.26 +60 44 41.1 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.43,0.05,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 20260620.4200 11.43CV 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 20.4200 2461211.9200 11.29 01:25:00.87 +62:50:52.5
126.75179 0.22546 galactic Cas Second-epoch detections are separated by 1.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:25:00.87 +62:50:52.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:00.87 +62:50:52.5: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:00.87 +62:50:52.5: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 25 00.87 +62 50 52.5 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.38 01:34:10.01 +60:13:05.8
128.21850 -2.21415 galactic Cas Second-epoch detections are separated by 0.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J023.5423+60.2306 | 01:34:10.01 +60:13:05.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.936+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:10.01 +60:13:05.8: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:10.01 +60:13:05.8: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.19 +/- 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 20.4200* 01 34 10.01 +60 13 05.8 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J023.5423+60.2306,2461211.9200,11.38,0.05,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
ATO J023.5423+60.2306 20260620.4200 11.38CV 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 20.4200 2461211.9200 11.46 01:05:53.88 +59:06:23.6
124.79102 -3.71299 galactic Cas Second-epoch detections are separated by 2.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:05:53.88 +59:06:23.6 (user input) | T | P | (position from user input) J-Ks=0.794+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:05:53.88 +59:06:23.6: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:53.88 +59:06:23.6: 14.42 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.42 +/- 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 20.4200* 01 05 53.88 +59 06 23.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.43 01:38:59.12 +61:08:53.2
128.63749 -1.19581 galactic Cas Second-epoch detections are separated by 2.3" and 3.2 pix
The object was found in VSX16" Gaia DR3 509947072000083840
Type: ROT
# Max. Min./Amp. JD0 Period
14.000 G 14.010 G 0.811910000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:59.12 +61:08:53.2: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:59.12 +61:08:53.2: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 38 59.12 +61 08 53.2 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509947072000083840,2461211.9200,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509947072000083840 20260620.4200 11.43CV 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 20.4200 2461211.9200 11.30 01:21:11.22 +59:33:02.0
126.69862 -3.10345 galactic Cas Second-epoch detections are separated by 1.3" and 3.3 pix
The object was found in VSX 3" ZTF J012111.28+593304.7
Type: RS
# Max. Min./Amp. JD0 Period
13.949 r Y 0.078 r 2458310.92390 14.521106900000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:11.22 +59:33:02.0: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:11.22 +59:33:02.0: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.84 +/- 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 20.4200* 01 21 11.22 +59 33 02.0 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J012111.28+593304.7,2461211.9200,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J012111.28+593304.7 20260620.4200 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.37 01:30:00.95 +60:10:50.0
127.71471 -2.33246 galactic Cas Second-epoch detections are separated by 2.4" and 3.1 pix
The object was found in VSX22" Gaia DR3 509459713474637440
Type: VAR
# Max. Min./Amp. JD0 Period
13.340 G 13.370 G 0.014865300000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:00.95 +60:10:50.0: 12.46 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:00.95 +60:10:50.0: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 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 20.4200* 01 30 00.95 +60 10 50.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509459713474637440,2461211.9200,11.37,0.05,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 509459713474637440 20260620.4200 11.37CV 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 20.4200 2461211.9200 11.52 02:13:37.67 +61:10:28.1
132.67468 -0.13292 galactic Cas Second-epoch detections are separated by 2.3" and 3.3 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 | 02:13:37.67 +61:10:28.1 (user input) | T | P | (position from user input) J-Ks=0.519+/-0.039 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:37.67 +61:10:28.1: 12.88 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:37.67 +61:10:28.1: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 13 37.67 +61 10 28.1 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.48 01:23:56.99 +62:15:27.9
126.70558 -0.37555 galactic Cas Second-epoch detections are separated by 2.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:23:56.99 +62:15:27.9 (user input) | T | P | (position from user input) J-Ks=0.526+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:56.99 +62:15:27.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:56.99 +62:15:27.9: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 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 20.4200* 01 23 56.99 +62 15 27.9 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.48,0.05,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 20260620.4200 11.48CV 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 20.4200 2461211.9200 11.29 01:23:53.55 +58:03:34.7
127.22749 -4.54117 galactic Cas Second-epoch detections are separated by 1.5" and 3.3 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 J020.9765+58.0503 | 01:23:53.55 +58:03:34.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:53.55 +58:03:34.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:53.55 +58:03:34.7: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 23 53.55 +58 03 34.7 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J020.9765+58.0503,2461211.9200,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J020.9765+58.0503 20260620.4200 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.36 01:32:10.98 +59:36:03.5
128.07256 -2.86348 galactic Cas Second-epoch detections are separated by 1.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J023.0277+59.5942 | 01:32:10.98 +59:36:03.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.889+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:10.98 +59:36:03.5: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:10.98 +59:36:03.5: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 32 10.98 +59 36 03.5 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J023.0277+59.5942,2461211.9200,11.36,0.05,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
ATO J023.0277+59.5942 20260620.4200 11.36CV 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 20.4200 2461211.9200 11.22 01:34:57.93 +61:00:13.6
128.18425 -1.42330 galactic Cas Second-epoch detections are separated by 0.3" and 3.4 pix
The object was found in VSX11" Gaia DR3 509967443017642624
Type: RS
# Max. Min./Amp. JD0 Period
17.430 G 17.560 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:57.93 +61:00:13.6: 12.41 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:57.93 +61:00:13.6: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 20.4200* 01 34 57.93 +61 00 13.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509967443017642624,2461211.9200,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509967443017642624 20260620.4200 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.28 01:33:20.05 +62:33:20.9
127.73805 0.07566 galactic Cas Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512315037781955200 | 01:33:17.17 +62:33:11.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.228+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:20.05 +62:33:20.9: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:20.05 +62:33:20.9: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 20.4200* 01 33 20.05 +62 33 20.9 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512315037781955200,2461211.9200,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512315037781955200 20260620.4200 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.29 01:40:18.20 +61:21:06.0
128.75540 -0.96635 galactic Cas Second-epoch detections are separated by 0.1" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:40:18.20 +61:21:06.0 (user input) | T | P | (position from user input) J-Ks=0.970+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:18.20 +61:21:06.0: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:18.20 +61:21:06.0: 13.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 20.4200* 01 40 18.20 +61 21 06.0 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.26 01:08:25.67 +59:48:03.7
125.06989 -3.00017 galactic Cas Second-epoch detections are separated by 1.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:08:25.67 +59:48:03.7 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:25.67 +59:48:03.7: 12.62 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:25.67 +59:48:03.7: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 08 25.67 +59 48 03.7 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.21 01:08:39.25 +60:32:41.3
125.04854 -2.25617 galactic Cas Second-epoch detections are separated by 2.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:08:39.25 +60:32:41.3 (user input) | T | P | (position from user input) J-Ks=0.751+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:39.25 +60:32:41.3: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:39.25 +60:32:41.3: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 08 39.25 +60 32 41.3 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.33 01:21:45.32 +58:34:15.3
126.88569 -4.06790 galactic Cas Second-epoch detections are separated by 2.9" and 4.0 pix
The object was found in VSX20" ZTF J012144.11+583432.6
Type: EA
# Max. Min./Amp. JD0 Period
17.914 r Y 0.259 r 2458650.93340 0.872868200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:45.32 +58:34:15.3: 12.68 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:45.32 +58:34:15.3: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 21 45.32 +58 34 15.3 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J012144.11+583432.6,2461211.9200,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J012144.11+583432.6 20260620.4200 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 20.4200 2461211.9200 11.33 01:07:01.87 +59:46:17.1
124.89616 -3.04085 galactic Cas Second-epoch detections are separated by 0.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:01.87 +59:46:17.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:01.87 +59:46:17.1: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:01.87 +59:46:17.1: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 07 01.87 +59 46 17.1 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4200 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 20.4200 2461211.9200 11.37 01:55:46.61 +57:57:42.5
131.40283 -3.84787 galactic Per Second-epoch detections are separated by 1.1" and 3.3 pix
The object was found in VSX18" ZTF J015546.41+575800.1
Type: RS
# Max. Min./Amp. JD0 Period
13.450 r Y 0.033 r 2458379.91220 0.825740500000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:46.61 +57:57:42.5: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:46.61 +57:57:42.5: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 55 46.61 +57 57 42.5 11.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J015546.41+575800.1,2461211.9200,11.37,0.05,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
ZTF J015546.41+575800.1 20260620.4200 11.37CV 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 20.4200 2461211.9200 11.30 01:57:29.26 +60:09:19.2
131.06680 -1.66906 galactic Cas Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:57:29.26 +60:09:19.2 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:29.26 +60:09:19.2: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:29.26 +60:09:19.2: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 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 20.4200* 01 57 29.26 +60 09 19.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.21 01:07:39.17 +59:59:18.0
124.96068 -2.81953 galactic Cas Second-epoch detections are separated by 0.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:39.17 +59:59:18.0 (user input) | T | P | (position from user input) J-Ks=0.895+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.17 +59:59:18.0: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.17 +59:59:18.0: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 07 39.17 +59 59 18.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.07 01:26:05.62 +59:01:15.0
127.38753 -3.55078 galactic Cas Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.5231+59.0209 | 01:26:05.62 +59:01:15.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.314+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.62 +59:01:15.0: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.62 +59:01:15.0: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 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 20.4200* 01 26 05.62 +59 01 15.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.5231+59.0209,2461211.9200,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.5231+59.0209 20260620.4200 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.19 01:20:42.12 +59:35:05.3
126.63359 -3.07645 galactic Cas Second-epoch detections are separated by 0.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:20:42.12 +59:35:05.3 (user input) | T | P | (position from user input) J-Ks=0.796+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:42.12 +59:35:05.3: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:42.12 +59:35:05.3: 13.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.91 +/- 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 20.4200* 01 20 42.12 +59 35 05.3 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.29 01:27:32.56 +64:34:36.1
126.79610 1.97617 galactic Cas Second-epoch detections are separated by 2.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:27:32.56 +64:34:36.1 (user input) | T | P | (position from user input) J-Ks=0.823+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:32.56 +64:34:36.1: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:32.56 +64:34:36.1: 14.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 27 32.56 +64 34 36.1 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.12 01:12:59.70 +57:34:09.5
125.83089 -5.18105 galactic Cas Second-epoch detections are separated by 2.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:59.70 +57:34:09.5 (user input) | T | P | (position from user input) J-Ks=0.831+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:59.70 +57:34:09.5: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:59.70 +57:34:09.5: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 20.4200* 01 12 59.70 +57 34 09.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.27 02:03:59.13 +59:34:48.0
132.00609 -2.00753 galactic Cas Second-epoch detections are separated by 1.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:03:59.13 +59:34:48.0 (user input) | T | P | (position from user input) J-Ks=0.876+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:59.13 +59:34:48.0: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:59.13 +59:34:48.0: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 03 59.13 +59 34 48.0 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4200 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 20.4200 2461211.9200 11.21 01:25:42.78 +58:50:45.7
127.36217 -3.73058 galactic Cas Second-epoch detections are separated by 2.5" and 3.3 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 413204617279292544 | 01:25:46.52 +58:50:59.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.746+/-0.042 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:42.78 +58:50:45.7: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:42.78 +58:50:45.7: 14.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 25 42.78 +58 50 45.7 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413204617279292544,2461211.9200,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413204617279292544 20260620.4200 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.10 01:24:55.09 +59:41:48.4
127.14945 -2.90053 galactic Cas Second-epoch detections are separated by 2.1" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:24:55.09 +59:41:48.4 (user input) | T | P | (position from user input) J-Ks=0.217+/-0.043 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:55.09 +59:41:48.4: 12.88 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:55.09 +59:41:48.4: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 24 55.09 +59 41 48.4 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.09 01:06:13.18 +59:33:47.5
124.80604 -3.25475 galactic Cas Second-epoch detections are separated by 1.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:13.18 +59:33:47.5 (user input) | T | P | (position from user input) J-Ks=0.462+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:13.18 +59:33:47.5: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:13.18 +59:33:47.5: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 06 13.18 +59 33 47.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.16 01:25:27.54 +59:27:15.5
127.24918 -3.13196 galactic Cas Second-epoch detections are separated by 1.1" and 3.3 pix
The object was found in VSX 5" Gaia DR3 510073344036983552
Type: ROT
# Max. Min./Amp. JD0 Period
14.460 G 14.520 G 1.820050000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:27.54 +59:27:15.5: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:27.54 +59:27:15.5: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 25 27.54 +59 27 15.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510073344036983552,2461211.9200,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510073344036983552 20260620.4200 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.13 01:51:47.29 +58:37:55.3
130.73218 -3.32275 galactic Cas Second-epoch detections are separated by 1.9" and 3.3 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 506225156418009984 | 01:51:45.68 +58:37:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:47.29 +58:37:55.3: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:47.29 +58:37:55.3: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 20.4200* 01 51 47.29 +58 37 55.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506225156418009984,2461211.9200,11.13,0.05,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
Gaia DR3 506225156418009984 20260620.4200 11.13CV 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 20.4200 2461211.9200 11.16 01:12:00.92 +64:42:18.2
125.12881 1.92112 galactic Cas Second-epoch detections are separated by 1.0" and 3.1 pix
The object was found in VSX 3" ZTF J011201.03+644221.2
Type: RS
# Max. Min./Amp. JD0 Period
14.762 g Y 0.263 g 2458343.85900 3.018403700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:00.92 +64:42:18.2: 12.00 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:00.92 +64:42:18.2: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 12 00.92 +64 42 18.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J011201.03+644221.2,2461211.9200,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011201.03+644221.2 20260620.4200 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.10 01:08:15.48 +61:15:06.7
124.95371 -1.55384 galactic Cas Second-epoch detections are separated by 0.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:08:15.48 +61:15:06.7 (user input) | T | P | (position from user input) J-Ks=0.814+/-0.026 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:15.48 +61:15:06.7: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:15.48 +61:15:06.7: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 08 15.48 +61 15 06.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.16 01:26:37.92 +60:38:02.4
127.23618 -1.94329 galactic Cas Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:26:37.92 +60:38:02.4 (user input) | T | P | (position from user input) J-Ks=0.456+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:37.92 +60:38:02.4: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:37.92 +60:38:02.4: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 26 37.92 +60 38 02.4 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.09 01:43:27.31 +58:38:07.0
129.67095 -3.55420 galactic Cas Second-epoch detections are separated by 2.2" and 3.7 pix
The object was found in VSX 2" Gaia DR3 506084487648397824
Type: ROT
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:27.31 +58:38:07.0: 12.70 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:27.31 +58:38:07.0: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 43 27.31 +58 38 07.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506084487648397824,2461211.9200,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506084487648397824 20260620.4200 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.16 01:29:48.25 +63:19:35.8
127.22193 0.77488 galactic Cas Second-epoch detections are separated by 0.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:29:48.25 +63:19:35.8 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:48.25 +63:19:35.8: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:48.25 +63:19:35.8: 13.76 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 20.4200* 01 29 48.25 +63 19 35.8 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.13 02:00:06.64 +59:00:32.8
131.68376 -2.69079 galactic Cas Second-epoch detections are separated by 0.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 507781618204489856 | 02:00:05.90 +59:00:52.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.381+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:06.64 +59:00:32.8: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:06.64 +59:00:32.8: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 00 06.64 +59 00 32.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507781618204489856,2461211.9200,11.13,0.05,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
Gaia DR3 507781618204489856 20260620.4200 11.13CV 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 20.4200 2461211.9200 11.11 01:07:45.52 +57:45:04.8
125.11625 -5.05118 galactic Cas Second-epoch detections are separated by 0.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J016.9392+57.7509 | 01:07:45.52 +57:45:04.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A9V (LAMOST DR5) J-Ks=0.654+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:45.52 +57:45:04.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:45.52 +57:45:04.8: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 07 45.52 +57 45 04.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J016.9392+57.7509,2461211.9200,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J016.9392+57.7509 20260620.4200 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.96 01:21:40.06 +61:36:42.7
126.51757 -1.04925 galactic Cas Second-epoch detections are separated by 0.7" and 3.3 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 510903887628222848 | 01:21:38.59 +61:37:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.609+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:40.06 +61:36:42.7: 11.95 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:40.06 +61:36:42.7: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 21 40.06 +61 36 42.7 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510903887628222848,2461211.9200,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510903887628222848 20260620.4200 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.94 01:30:34.37 +59:44:32.2
127.84964 -2.75528 galactic Cas Second-epoch detections are separated by 1.9" and 3.3 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 J022.6525+59.7408 | 01:30:34.37 +59:44:32.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.454+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:34.37 +59:44:32.2: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:34.37 +59:44:32.2: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 30 34.37 +59 44 32.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J022.6525+59.7408,2461211.9200,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.6525+59.7408 20260620.4200 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.91 01:35:27.62 +60:33:47.4
128.31830 -1.84737 galactic Cas Second-epoch detections are separated by 0.9" and 3.3 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 509811625915787136 | 01:35:29.25 +60:33:31.0 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.155+/-0.047 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:27.62 +60:33:47.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:27.62 +60:33:47.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 35 27.62 +60 33 47.4 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509811625915787136,2461211.9200,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509811625915787136 20260620.4200 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.95 01:37:17.59 +57:50:54.6
129.02191 -4.48002 galactic Cas Second-epoch detections are separated by 0.3" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J013714.59+575035.9 | 01:37:15.10 +57:50:48.3 (Gaia DR3) | VAR (local) | 46.310000000000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.331+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:17.59 +57:50:54.6: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:17.59 +57:50:54.6: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 37 17.59 +57 50 54.6 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013714.59+575035.9,2461211.9200,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J013714.59+575035.9 20260620.4200 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.87 01:34:16.42 +60:57:34.9
128.10885 -1.48076 galactic Cas Second-epoch detections are separated by 0.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:34:16.42 +60:57:34.9 (user input) | T | P | (position from user input) J-Ks=0.888+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:16.42 +60:57:34.9: 12.55 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:16.42 +60:57:34.9: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 34 16.42 +60 57 34.9 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.71 01:17:15.14 +58:35:37.1
126.29840 -4.10927 galactic Cas Second-epoch detections are separated by 2.5" and 3.3 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 J019.3185+58.5958 | 01:17:17.58 +58:36:18.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1960IzKry..24..160B [B60] +58 130 J-Ks=0.437+/-0.037 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:15.14 +58:35:37.1: 12.46 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:15.14 +58:35:37.1: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 17 15.14 +58 35 37.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J019.3185+58.5958,2461211.9200,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J019.3185+58.5958 20260620.4200 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.79 01:25:45.80 +59:01:22.7
127.34504 -3.55434 galactic Cas Second-epoch detections are separated by 3.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:25:45.80 +59:01:22.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:45.80 +59:01:22.7: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:45.80 +59:01:22.7: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 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 20.4200* 01 25 45.80 +59 01 22.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,10.79,0.05,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 20260620.4200 10.79CV 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 20.4200 2461211.9200 10.77 01:49:15.82 +59:14:38.3
130.27535 -2.80082 galactic Cas Second-epoch detections are separated by 0.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506536352570768768 | 01:49:14.31 +59:14:50.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.811+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:15.82 +59:14:38.3: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:15.82 +59:14:38.3: 13.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 20.4200* 01 49 15.82 +59 14 38.3 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506536352570768768,2461211.9200,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506536352570768768 20260620.4200 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.88 02:05:14.98 +63:02:37.2
131.18380 1.36055 galactic Cas Second-epoch detections are separated by 0.3" and 3.3 pix
The object was found in VSX11" ZTF J020514.76+630248.4
Type: EW
# Max. Min./Amp. JD0 Period
16.621 r Y 0.211 r 2458457.67520 0.337767600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:05:14.98 +63:02:37.2: 13.03 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:05:14.98 +63:02:37.2: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 05 14.98 +63 02 37.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J020514.76+630248.4,2461211.9200,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J020514.76+630248.4 20260620.4200 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.72 01:26:39.09 +59:41:38.1
127.36682 -2.87427 galactic Cas Second-epoch detections are separated by 0.9" and 3.5 pix
The object was found in VSX 2" Gaia DR3 510083239641442688
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.660 G 13.680 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:39.09 +59:41:38.1: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:39.09 +59:41:38.1: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 26 39.09 +59 41 38.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510083239641442688,2461211.9200,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510083239641442688 20260620.4200 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.70 01:18:47.92 +59:08:14.7
126.44139 -3.54777 galactic Cas Second-epoch detections are separated by 0.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:47.92 +59:08:14.7 (user input) | T | P | (position from user input) J-Ks=0.596+/-0.037 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:47.92 +59:08:14.7: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:47.92 +59:08:14.7: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 18 47.92 +59 08 14.7 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,10.70,0.05,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 20260620.4200 10.70CV 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 20.4200 2461211.9200 10.74 01:07:31.84 +61:28:27.2
124.85251 -1.33750 galactic Cas Second-epoch detections are separated by 3.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:31.84 +61:28:27.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:31.84 +61:28:27.2: 12.82 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:31.84 +61:28:27.2: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 07 31.84 +61 28 27.2 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.74 01:56:43.24 +58:07:17.9
131.48419 -3.66199 galactic Cas Second-epoch detections are separated by 1.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:56:43.24 +58:07:17.9 (user input) | T | P | (position from user input) J-Ks=0.952+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:43.24 +58:07:17.9: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:43.24 +58:07:17.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 56 43.24 +58 07 17.9 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.66 01:31:23.12 +59:33:43.6
127.97878 -2.91763 galactic Cas Second-epoch detections are separated by 0.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J022.8294+59.5638 | 01:31:23.12 +59:33:43.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.833+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:23.12 +59:33:43.6: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:23.12 +59:33:43.6: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 31 23.12 +59 33 43.6 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J022.8294+59.5638,2461211.9200,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.8294+59.5638 20260620.4200 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.75 01:35:24.58 +60:39:29.9
128.29600 -1.75467 galactic Cas Second-epoch detections are separated by 1.9" and 3.5 pix
The object was found in VSX15" Gaia DR3 509819081975016960
Type: S
# Max. Min./Amp. JD0 Period
17.140 G 17.450 G O
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:24.58 +60:39:29.9: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:24.58 +60:39:29.9: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 35 24.58 +60 39 29.9 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509819081975016960,2461211.9200,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509819081975016960 20260620.4200 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.61 01:20:45.05 +57:55:09.5
126.82971 -4.73043 galactic Cas Second-epoch detections are separated by 1.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413797116609704704 | 01:20:41.29 +57:55:17.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.023+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:45.05 +57:55:09.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:45.05 +57:55:09.5: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 20 45.05 +57 55 09.5 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413797116609704704,2461211.9200,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413797116609704704 20260620.4200 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.57 01:08:23.32 +61:35:09.9
124.94740 -1.21931 galactic Cas Second-epoch detections are separated by 2.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 522537957607670016 | 01:08:22.26 +61:34:35.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.299+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:23.32 +61:35:09.9: 12.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:23.32 +61:35:09.9: 13.18 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 20.4200* 01 08 23.32 +61 35 09.9 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522537957607670016,2461211.9200,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522537957607670016 20260620.4200 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.59 01:19:08.73 +60:33:58.6
126.33195 -2.12243 galactic Cas Second-epoch detections are separated by 1.2" and 3.3 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 510378080556092032 | 01:19:06.00 +60:34:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.265+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:08.73 +60:33:58.6: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:08.73 +60:33:58.6: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 19 08.73 +60 33 58.6 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510378080556092032,2461211.9200,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510378080556092032 20260620.4200 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 20.4200 2461211.9200 10.46 01:27:35.79 +57:57:00.7
127.72992 -4.58431 galactic Cas Second-epoch detections are separated by 2.1" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413090817828281216 | 01:27:33.40 +57:56:56.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.205+/-0.038 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:35.79 +57:57:00.7: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:35.79 +57:57:00.7: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 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 20.4200* 01 27 35.79 +57 57 00.7 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413090817828281216,2461211.9200,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413090817828281216 20260620.4200 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.32 02:00:26.68 +63:04:13.4
130.65275 1.23772 galactic Cas Second-epoch detections are separated by 0.6" and 3.3 pix
The object was found in VSX 2" Gaia DR3 508892228030391552
Type: E
# Max. Min./Amp. JD0 Period
13.120 G 13.390 G 3.454060000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:26.68 +63:04:13.4: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:26.68 +63:04:13.4: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 20.4200* 02 00 26.68 +63 04 13.4 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508892228030391552,2461211.9200,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508892228030391552 20260620.4200 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.16 01:07:57.25 +63:37:29.5
124.76515 0.81192 galactic Cas Second-epoch detections are separated by 0.9" and 3.6 pix
The object was found in VSX22" V1064 Cas
Type: EW
# Max. Min./Amp. JD0 Period
11.300 R1 11.800 R1 2451349.91900 0.457606000000 B2
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:57.25 +63:37:29.5: 10.60 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:57.25 +63:37:29.5: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 07 57.25 +63 37 29.5 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1064 Cas,2461211.9200,10.16,0.05,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
V1064 Cas 20260620.4200 10.16CV 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 20.4200 2461211.9200 10.12 01:35:25.03 +60:39:14.8
128.29762 -1.75865 galactic Cas Second-epoch detections are separated by 1.2" and 3.4 pix
The object was found in VSX 6" Gaia DR3 509819081975016960
Type: S
# Max. Min./Amp. JD0 Period
17.140 G 17.450 G O
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:25.03 +60:39:14.8: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:25.03 +60:39:14.8: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 35 25.03 +60 39 14.8 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509819081975016960,2461211.9200,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509819081975016960 20260620.4200 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.13 01:49:03.90 +61:04:19.4
129.84527 -1.02381 galactic Cas Second-epoch detections are separated by 1.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:49:03.90 +61:04:19.4 (user input) | T | P | (position from user input) J-Ks=0.226+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:03.90 +61:04:19.4: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:03.90 +61:04:19.4: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 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 20.4200* 01 49 03.90 +61 04 19.4 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 9.88 01:23:31.47 +58:41:48.0
127.09950 -3.91520 galactic Cas Second-epoch detections are separated by 1.2" and 3.7 pix
The object was found in VSX22" Gaia DR3 413949673852809088
Type: ROT
# Max. Min./Amp. JD0 Period
16.410 G 16.550 G 1.041480000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:31.47 +58:41:48.0: 12.11 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:31.47 +58:41:48.0: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 23 31.47 +58 41 48.0 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413949673852809088,2461211.9200,9.88,0.05,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 413949673852809088 20260620.4200 9.88CV 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 20.4200 2461211.9200 9.33 01:27:22.04 +58:51:39.5
127.57250 -3.68667 galactic Cas Second-epoch detections are separated by 0.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.8600+58.8695 | 01:27:20.86 +58:51:57.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.829+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:22.04 +58:51:39.5: 11.69 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:22.04 +58:51:39.5: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 27 22.04 +58 51 39.5 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.8600+58.8695,2461211.9200,9.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.8600+58.8695 20260620.4200 9.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 20.4200 2461211.9200 10.29 01:10:34.59 +60:31:07.6
125.28639 -2.26545 galactic Cas Second-epoch detections are separated by 0.7" and 3.4 pix
The object was found in VSX 1" ZTF J011034.65+603107.8
Type: RS
# Max. Min./Amp. JD0 Period
13.515 r Y 0.105 r 2458370.91340 3.097346100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:34.59 +60:31:07.6: 12.57 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:34.59 +60:31:07.6: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 10 34.59 +60 31 07.6 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J011034.65+603107.8,2461211.9200,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011034.65+603107.8 20260620.4200 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.62 01:46:38.50 +60:07:33.1
129.76019 -2.01198 galactic Cas Second-epoch detections are separated by 0.4" and 3.3 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 J026.6591+60.1406 | 01:46:39.63 +60:07:57.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.50 +60:07:33.1: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:38.50 +60:07:33.1: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 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 20.4200* 01 46 38.50 +60 07 33.1 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.6591+60.1406,2461211.9200,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.6591+60.1406 20260620.4200 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.39 01:18:28.11 +58:11:23.6
126.49892 -4.49453 galactic Cas Second-epoch detections are separated by 2.2" and 3.3 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 J019.6245+58.1745 | 01:18:29.87 +58:10:59.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G8III 1951UppAn...2j...1B NGC 457 236 J-Ks=0.371+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:28.11 +58:11:23.6: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:28.11 +58:11:23.6: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 18 28.11 +58 11 23.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J019.6245+58.1745,2461211.9200,10.39,0.05,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
ATO J019.6245+58.1745 20260620.4200 10.39CV 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 20.4200 2461211.9200 10.72 02:00:21.73 +64:56:38.5
130.14904 3.04251 galactic Cas Second-epoch detections are separated by 1.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 518139017740687360 | 02:00:16.12 +64:56:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9IV/V 1928MeUpp..37....1S BD+64 275 J-Ks=1.311+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:21.73 +64:56:38.5: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:21.73 +64:56:38.5: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 00 21.73 +64 56 38.5 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 518139017740687360,2461211.9200,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518139017740687360 20260620.4200 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.78 01:51:09.35 +64:52:46.8
129.21809 2.73929 galactic Cas Second-epoch detections are separated by 2.6" and 2.8 pix
The object was found in VSX 2" Gaia DR3 518229967963921664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:09.35 +64:52:46.8: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:09.35 +64:52:46.8: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 51 09.35 +64 52 46.8 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 518229967963921664,2461211.9200,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518229967963921664 20260620.4200 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.89 01:08:59.45 +60:47:21.1
125.07320 -2.00956 galactic Cas Second-epoch detections are separated by 1.3" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 522440066710315904 | 01:08:58.80 +60:47:45.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.504+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:59.45 +60:47:21.1: 13.11 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:59.45 +60:47:21.1: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 08 59.45 +60 47 21.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522440066710315904,2461211.9200,10.89,0.05,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 522440066710315904 20260620.4200 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 20.4200 2461211.9200 10.99 01:14:41.44 +58:46:46.5
125.94849 -3.95591 galactic Cas Second-epoch detections are separated by 2.0" and 3.8 pix
The object was found in VSX22" Gaia DR3 414091266028390144
Type: ROT
# Max. Min./Amp. JD0 Period
18.000 G 18.140 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:41.44 +58:46:46.5: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:41.44 +58:46:46.5: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 14 41.44 +58 46 46.5 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414091266028390144,2461211.9200,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 414091266028390144 20260620.4200 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.96 01:22:10.97 +59:09:03.5
126.87182 -3.48538 galactic Cas Second-epoch detections are separated by 1.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413976852405588480 | 01:22:13.31 +59:08:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1960IzKry..24..160B [B60] +58 184 J-Ks=0.462+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:10.97 +59:09:03.5: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:10.97 +59:09:03.5: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 22 10.97 +59 09 03.5 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413976852405588480,2461211.9200,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413976852405588480 20260620.4200 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.07 02:16:07.78 +58:18:14.4
133.88413 -2.75536 galactic Per Second-epoch detections are separated by 1.5" and 3.6 pix
The object was found in VSX 3" Gaia DR3 458762778499159168
Type: VAR
# Max. Min./Amp. JD0 Period
13.750 G 13.790 G 0.014923200000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:07.78 +58:18:14.4: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:07.78 +58:18:14.4: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 16 07.78 +58 18 14.4 11.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458762778499159168,2461211.9200,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458762778499159168 20260620.4200 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.00 01:51:26.73 +57:51:36.7
130.86728 -4.08405 galactic Per Second-epoch detections are separated by 0.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506162862211871616 | 01:51:29.54 +57:50:59.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.266+/-0.053 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:26.73 +57:51:36.7: 12.83 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:26.73 +57:51:36.7: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 51 26.73 +57 51 36.7 11.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506162862211871616,2461211.9200,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506162862211871616 20260620.4200 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.09 02:21:38.04 +65:44:28.6
132.02476 4.47452 galactic Cas Second-epoch detections are separated by 1.3" and 3.3 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 517069845756285184 | 02:21:38.42 +65:45:06.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:38.04 +65:44:28.6: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:38.04 +65:44:28.6: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 21 38.04 +65 44 28.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 517069845756285184,2461211.9200,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 517069845756285184 20260620.4200 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.20 02:15:03.70 +58:28:54.2
133.69449 -2.63173 galactic Per Second-epoch detections are separated by 1.3" and 3.3 pix
The object was found in VSX 3" Gaia DR3 506806798067617152
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.780 G 13.810 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:03.70 +58:28:54.2: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:03.70 +58:28:54.2: 13.71 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 20.4200* 02 15 03.70 +58 28 54.2 11.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506806798067617152,2461211.9200,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506806798067617152 20260620.4200 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.98 01:09:22.61 +57:26:31.1
125.35418 -5.34538 galactic Cas Second-epoch detections are separated by 1.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.3204+57.4562 | 01:09:17.29 +57:26:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.782+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:22.61 +57:26:31.1: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.61 +57:26:31.1: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 09 22.61 +57 26 31.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.3204+57.4562,2461211.9200,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.3204+57.4562 20260620.4200 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.01 01:13:39.03 +58:10:51.2
125.86575 -4.56427 galactic Cas Second-epoch detections are separated by 3.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J018.4234+58.1762 | 01:13:41.63 +58:10:34.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.593+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:39.03 +58:10:51.2: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:39.03 +58:10:51.2: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 20.4200* 01 13 39.03 +58 10 51.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J018.4234+58.1762,2461211.9200,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J018.4234+58.1762 20260620.4200 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 10.97 01:22:23.90 +61:13:51.6
126.64949 -1.41707 galactic Cas Second-epoch detections are separated by 0.6" and 3.5 pix
The object was found in VSX 1" NSVS J0122238+611352
Type: M
# Max. Min./Amp. JD0 Period
14.871 r Y 3.740 r 2458328.87710 325.120339600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:23.90 +61:13:51.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:23.90 +61:13:51.6: 15.73 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.73 +/- 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 20.4200* 01 22 23.90 +61 13 51.6 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0122238+611352,2461211.9200,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0122238+611352 20260620.4200 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.09 02:00:32.94 +59:40:07.3
131.56360 -2.03982 galactic Cas Second-epoch detections are separated by 2.5" and 3.1 pix
The object was found in VSX 2" ZTF J020033.07+594008.7
Type: SR
# Max. Min./Amp. JD0 Period
13.621 r Y 0.477 r 2458342.93970 344.838134100000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:32.94 +59:40:07.3: 11.53 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.94 +59:40:07.3: 14.20 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 00 32.94 +59 40 07.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J020033.07+594008.7,2461211.9200,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J020033.07+594008.7 20260620.4200 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.05 01:38:05.83 +61:04:14.1
128.54606 -1.29154 galactic Cas Second-epoch detections are separated by 0.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:38:05.83 +61:04:14.1 (user input) | T | P | (position from user input) J-Ks=0.901+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:05.83 +61:04:14.1: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:05.83 +61:04:14.1: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 38 05.83 +61 04 14.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.02 01:24:49.19 +59:47:15.9
127.12536 -2.81193 galactic Cas Second-epoch detections are separated by 0.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510095677857790080 | 01:24:49.88 +59:46:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1960IzKry..24..160B [B60] +59 160 J-Ks=0.149+/-0.051 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:49.19 +59:47:15.9: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:49.19 +59:47:15.9: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 24 49.19 +59 47 15.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510095677857790080,2461211.9200,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510095677857790080 20260620.4200 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.16 02:16:27.39 +64:52:49.7
131.80085 3.48290 galactic Cas Second-epoch detections are separated by 2.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:16:27.39 +64:52:49.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:27.39 +64:52:49.7: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:27.39 +64:52:49.7: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 16 27.39 +64 52 49.7 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.12 01:50:39.84 +62:00:56.4
129.81909 -0.06153 galactic Cas Second-epoch detections are separated by 1.0" and 3.3 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 511356332360621440 | 01:50:34.89 +62:00:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1955ApJS....2..123F LF 5 +61 158 J-Ks=1.202+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:39.84 +62:00:56.4: 13.33 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:39.84 +62:00:56.4: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 50 39.84 +62 00 56.4 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511356332360621440,2461211.9200,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511356332360621440 20260620.4200 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.26 01:41:34.52 +59:13:59.0
129.31483 -3.01593 galactic Cas Second-epoch detections are separated by 0.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:41:34.52 +59:13:59.0 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:34.52 +59:13:59.0: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:34.52 +59:13:59.0: 14.08 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.08 +/- 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 20.4200* 01 41 34.52 +59 13 59.0 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.07 01:25:25.28 +58:19:59.4
127.39246 -4.24396 galactic Cas Second-epoch detections are separated by 1.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.3568+58.3360 | 01:25:26.64 +58:19:32.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8 1960IzKry..24..160B [B60] +58 215 J-Ks=0.486+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:25.28 +58:19:59.4: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:25.28 +58:19:59.4: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 25 25.28 +58 19 59.4 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.3568+58.3360,2461211.9200,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.3568+58.3360 20260620.4200 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.07 01:06:55.34 +59:18:58.6
124.90991 -3.49599 galactic Cas Second-epoch detections are separated by 0.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:55.34 +59:18:58.6 (user input) | T | P | (position from user input) J-Ks=0.785+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.34 +59:18:58.6: 13.12 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.34 +59:18:58.6: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 06 55.34 +59 18 58.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.22 01:52:55.35 +59:33:31.4
130.65677 -2.38771 galactic Cas Second-epoch detections are separated by 1.7" and 3.3 pix
The object was found in VSX18" Gaia DR3 506553498077188608
Type: ROT
# Max. Min./Amp. JD0 Period
15.360 G 15.380 G 2.474540000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:55.35 +59:33:31.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:55.35 +59:33:31.4: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 20.4200* 01 52 55.35 +59 33 31.4 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506553498077188608,2461211.9200,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506553498077188608 20260620.4200 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.19 02:02:25.08 +64:38:23.8
130.44176 2.80815 galactic Cas Second-epoch detections are separated by 1.3" and 3.3 pix
The object was found in VSX 6" ASASSN-V J020225.96+643822.9
Type: SR
# Max. Min./Amp. JD0 Period
14.090 V 14.200 V 2457555.11300 70.630000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:25.08 +64:38:23.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:25.08 +64:38:23.8: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 02 25.08 +64 38 23.8 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J020225.96+643822.9,2461211.9200,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J020225.96+643822.9 20260620.4200 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.16 01:56:57.38 +63:00:32.5
130.28643 1.07661 galactic Cas Second-epoch detections are separated by 2.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:56:57.38 +63:00:32.5 (user input) | T | P | (position from user input) J-Ks=0.837+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:57.38 +63:00:32.5: 13.25 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:57.38 +63:00:32.5: 13.98 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.95 +/- 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 20.4200* 01 56 57.38 +63 00 32.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.21 01:59:34.04 +63:37:09.5
130.41368 1.74158 galactic Cas Second-epoch detections are separated by 2.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:59:34.04 +63:37:09.5 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:34.04 +63:37:09.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:34.04 +63:37:09.5: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 59 34.04 +63 37 09.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.20 01:42:17.62 +63:24:23.7
128.58701 1.09459 galactic Cas Second-epoch detections are separated by 2.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512081945620708864 | 01:42:22.23 +63:24:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.949+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:17.62 +63:24:23.7: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:17.62 +63:24:23.7: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 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 20.4200* 01 42 17.62 +63 24 23.7 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512081945620708864,2461211.9200,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512081945620708864 20260620.4200 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.11 01:38:34.72 +57:58:01.1
129.16899 -4.33277 galactic Cas Second-epoch detections are separated by 2.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J024.6398+57.9682 | 01:38:34.52 +57:58:32.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.366+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:34.72 +57:58:01.1: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:34.72 +57:58:01.1: 13.90 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 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 20.4200* 01 38 34.72 +57 58 01.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.6398+57.9682,2461211.9200,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J024.6398+57.9682 20260620.4200 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.34 01:56:48.73 +61:52:37.5
130.55411 -0.02336 galactic Cas Second-epoch detections are separated by 3.2" and 2.9 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 508708918825570048 | 01:56:44.14 +61:52:29.7 (Gaia DR3) | DSCT/GDOR (local) | B (local) | Gaia3var=VARIABLE SpType: B5 1953IzKry..10..120K [K53] 656
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:48.73 +61:52:37.5: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:48.73 +61:52:37.5: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.21 +/- 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 20.4200* 01 56 48.73 +61 52 37.5 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508708918825570048,2461211.9200,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508708918825570048 20260620.4200 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.13 01:52:55.29 +60:27:25.5
130.44447 -1.51476 galactic Cas Second-epoch detections are separated by 4.3" and 2.7 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 508121436018447744 | 01:52:50.90 +60:27:58.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1928AnHar.100...49C HD 236896 J-Ks=0.210+/-0.044 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:55.29 +60:27:25.5: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:55.29 +60:27:25.5: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 52 55.29 +60 27 25.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508121436018447744,2461211.9200,11.13,0.05,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
Gaia DR3 508121436018447744 20260620.4200 11.13CV 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 20.4200 2461211.9200 11.23 01:17:45.49 +57:34:01.3
126.46951 -5.12382 galactic Cas Second-epoch detections are separated by 2.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:17:45.49 +57:34:01.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:45.49 +57:34:01.3: 12.95 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:45.49 +57:34:01.3: 14.03 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 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 20.4200* 01 17 45.49 +57 34 01.3 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.32 02:08:50.63 +59:21:19.7
132.66198 -2.04608 galactic Cas Second-epoch detections are separated by 1.2" and 3.3 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 | 02:08:50.63 +59:21:19.7 (user input) | T | P | (position from user input) J-Ks=0.939+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:08:50.63 +59:21:19.7: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:08:50.63 +59:21:19.7: 14.05 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 08 50.63 +59 21 19.7 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.30 01:51:53.64 +63:26:20.9
129.62913 1.35623 galactic Cas Second-epoch detections are separated by 1.6" and 3.2 pix
The object was found in VSX11" ZTF J015152.31+632614.6
Type: EB:
# Max. Min./Amp. JD0 Period
15.451 r Y 0.389 r 2458367.82620 5.408679200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:53.64 +63:26:20.9: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:53.64 +63:26:20.9: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 51 53.64 +63 26 20.9 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J015152.31+632614.6,2461211.9200,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J015152.31+632614.6 20260620.4200 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.24 01:23:46.56 +60:53:19.3
126.85693 -1.73637 galactic Cas Second-epoch detections are separated by 1.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:23:46.56 +60:53:19.3 (user input) | T | P | (position from user input) J-Ks=0.260+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:46.56 +60:53:19.3: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:46.56 +60:53:19.3: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 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 20.4200* 01 23 46.56 +60 53 19.3 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.36 02:07:53.85 +58:37:40.7
132.75902 -2.77732 galactic Per Second-epoch detections are separated by 1.2" and 3.2 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 506785185794584448 | 02:07:53.98 +58:37:02.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:53.85 +58:37:40.7: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:53.85 +58:37:40.7: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 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 20.4200* 02 07 53.85 +58 37 40.7 11.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506785185794584448,2461211.9200,11.36,0.05,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 506785185794584448 20260620.4200 11.36CV 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 20.4200 2461211.9200 11.33 01:33:30.69 +58:02:23.6
128.49331 -4.37683 galactic Cas Second-epoch detections are separated by 2.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J023.3712+58.0394 | 01:33:30.69 +58:02:23.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.820+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:30.69 +58:02:23.6: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:30.69 +58:02:23.6: 14.24 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.24 +/- 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 20.4200* 01 33 30.69 +58 02 23.6 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J023.3712+58.0394,2461211.9200,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J023.3712+58.0394 20260620.4200 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 20.4200 2461211.9200 11.36 01:40:29.69 +60:46:50.2
128.88596 -1.52277 galactic Cas Second-epoch detections are separated by 1.2" and 3.4 pix
The object was found in VSX23" Gaia DR3 509739156919523456
Type: ROT
# Max. Min./Amp. JD0 Period
18.190 G 18.370 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:29.69 +60:46:50.2: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:29.69 +60:46:50.2: 14.41 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 40 29.69 +60 46 50.2 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509739156919523456,2461211.9200,11.36,0.05,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 509739156919523456 20260620.4200 11.36CV 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 20.4200 2461211.9200 11.33 01:40:21.93 +60:45:15.1
128.87544 -1.55169 galactic Cas Second-epoch detections are separated by 4.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:40:21.93 +60:45:15.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:21.93 +60:45:15.1: 11.70 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:21.93 +60:45:15.1: 14.25 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 20.4200* 01 40 21.93 +60 45 15.1 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4200 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 20.4200 2461211.9200 11.29 01:26:28.50 +59:41:36.9
127.34478 -2.87763 galactic Cas Second-epoch detections are separated by 1.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.6536+59.6928 | 01:26:31.85 +59:41:21.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:28.50 +59:41:36.9: 12.93 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:28.50 +59:41:36.9: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 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 20.4200* 01 26 28.50 +59 41 36.9 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.6536+59.6928,2461211.9200,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.6536+59.6928 20260620.4200 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.40 01:29:20.11 +59:29:36.8
127.73182 -3.02455 galactic Cas Second-epoch detections are separated by 4.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J022.3174+59.4934 | 01:29:20.11 +59:29:36.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.710+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:20.11 +59:29:36.8: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:20.11 +59:29:36.8: 14.33 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.33 +/- 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 20.4200* 01 29 20.11 +59 29 36.8 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J022.3174+59.4934,2461211.9200,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.3174+59.4934 20260620.4200 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.36 01:24:11.89 +59:17:51.8
127.11001 -3.30801 galactic Cas Second-epoch detections are separated by 0.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:24:11.89 +59:17:51.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:11.89 +59:17:51.8: 12.76 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:11.89 +59:17:51.8: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.04 +/- 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 20.4200* 01 24 11.89 +59 17 51.8 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.36,0.05,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 20260620.4200 11.36CV 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 20.4200 2461211.9200 11.28 01:19:29.32 +59:25:22.1
126.49841 -3.25456 galactic Cas Second-epoch detections are separated by 0.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 414042479505165696 | 01:19:30.78 +59:24:54.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G3 1935BSD...C01....0S BSD 8- 264 J-Ks=0.435+/-0.045 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:29.32 +59:25:22.1: 13.08 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:29.32 +59:25:22.1: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 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 20.4200* 01 19 29.32 +59 25 22.1 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 414042479505165696,2461211.9200,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 414042479505165696 20260620.4200 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.43 02:04:06.48 +60:14:18.0
131.83815 -1.37077 galactic Cas Second-epoch detections are separated by 1.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:04:06.48 +60:14:18.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:04:06.48 +60:14:18.0: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:04:06.48 +60:14:18.0: 14.25 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.25 +/- 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 20.4200* 02 04 06.48 +60 14 18.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.43,0.05,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 20260620.4200 11.43CV 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 20.4200 2461211.9200 11.44 01:25:25.32 +58:37:26.1
127.35412 -3.95573 galactic Cas Second-epoch detections are separated by 2.0" and 3.3 pix
The object was found in VSX 0" Gaia DR3 413195511953349504
Type: ROT
# Max. Min./Amp. JD0 Period
14.240 G 14.260 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:25.32 +58:37:26.1: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:25.32 +58:37:26.1: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 25 25.32 +58 37 26.1 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413195511953349504,2461211.9200,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413195511953349504 20260620.4200 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.34 01:51:52.56 +60:27:42.9
130.31800 -1.54022 galactic Cas Second-epoch detections are separated by 1.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:51:52.56 +60:27:42.9 (user input) | T | P | (position from user input) J-Ks=0.494+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:52.56 +60:27:42.9: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:52.56 +60:27:42.9: 14.27 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.27 +/- 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 20.4200* 01 51 52.56 +60 27 42.9 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.36 02:09:40.63 +60:06:56.2
132.53677 -1.28900 galactic Cas Second-epoch detections are separated by 2.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 507523954523438464 | 02:09:45.94 +60:07:09.6 (Gaia DR3) | E (local) | F (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:40.63 +60:06:56.2: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:40.63 +60:06:56.2: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 09 40.63 +60 06 56.2 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507523954523438464,2461211.9200,11.36,0.05,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 507523954523438464 20260620.4200 11.36CV 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 20.4200 2461211.9200 11.31 01:31:56.01 +59:26:39.7
128.06591 -3.02312 galactic Cas Second-epoch detections are separated by 1.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J023.0100+59.4551 | 01:31:59.23 +59:26:47.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1955ApJS....2..123F LF 5 +59 42 J-Ks=0.314+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:56.01 +59:26:39.7: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:56.01 +59:26:39.7: 14.12 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 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 20.4200* 01 31 56.01 +59 26 39.7 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J023.0100+59.4551,2461211.9200,11.31,0.05,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
ATO J023.0100+59.4551 20260620.4200 11.31CV 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 20.4200 2461211.9200 11.33 01:44:29.89 +65:09:23.0
128.47098 2.85684 galactic Cas Second-epoch detections are separated by 1.8" and 3.3 pix
The object was found in VSX 5" Gaia DR3 519045973088246784
Type: ROT
# Max. Min./Amp. JD0 Period
15.090 G 15.140 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:29.89 +65:09:23.0: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:29.89 +65:09:23.0: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 44 29.89 +65 09 23.0 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 519045973088246784,2461211.9200,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 519045973088246784 20260620.4200 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 20.4200 2461211.9200 11.47 01:52:07.30 +59:13:07.9
130.63740 -2.74200 galactic Cas Second-epoch detections are separated by 0.1" and 3.4 pix
The object was found in VSX 1" Gaia DR3 506523983061019904
Type: ROT
# Max. Min./Amp. JD0 Period
14.190 G 14.230 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:07.30 +59:13:07.9: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:07.30 +59:13:07.9: 14.27 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.27 +/- 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 20.4200* 01 52 07.30 +59 13 07.9 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506523983061019904,2461211.9200,11.47,0.05,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
Gaia DR3 506523983061019904 20260620.4200 11.47CV 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 20.4200 2461211.9200 11.38 01:29:33.79 +60:47:14.9
127.56945 -1.74053 galactic Cas Second-epoch detections are separated by 1.0" and 3.3 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 510609321594344192 | 01:29:30.46 +60:47:41.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0IV/V 1928MeUpp..37....1S BD+60 245
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:33.79 +60:47:14.9: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:33.79 +60:47:14.9: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.19 +/- 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 20.4200* 01 29 33.79 +60 47 14.9 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510609321594344192,2461211.9200,11.38,0.05,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
Gaia DR3 510609321594344192 20260620.4200 11.38CV 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 20.4200 2461211.9200 11.54 01:57:26.38 +63:23:42.4
130.24187 1.46397 galactic Cas Second-epoch detections are separated by 1.0" and 3.3 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 511905955039761920 | 01:57:32.54 +63:23:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8III 1928MeUpp..37....1S [S28] 397 J-Ks=0.602+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:26.38 +63:23:42.4: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:26.38 +63:23:42.4: 14.27 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.27 +/- 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 20.4200* 01 57 26.38 +63 23 42.4 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511905955039761920,2461211.9200,11.54,0.05,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 511905955039761920 20260620.4200 11.54CV 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 20.4200 2461211.9200 11.40 01:19:11.94 +59:07:32.3
126.49380 -3.55398 galactic Cas Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414009562874273024 | 01:19:13.47 +59:07:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1935BSD...C01....0S BSD 8- 261 J-Ks=0.463+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:11.94 +59:07:32.3: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:11.94 +59:07:32.3: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 19 11.94 +59 07 32.3 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414009562874273024,2461211.9200,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 414009562874273024 20260620.4200 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.54 02:08:22.88 +64:18:53.9
131.15055 2.67796 galactic Cas Second-epoch detections are separated by 3.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 515065745303799552 | 02:08:17.17 +64:18:30.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.243+/-0.044 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:08:22.88 +64:18:53.9: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:08:22.88 +64:18:53.9: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 08 22.88 +64 18 53.9 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 515065745303799552,2461211.9200,11.54,0.05,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 515065745303799552 20260620.4200 11.54CV 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 20.4200 2461211.9200 11.55 01:41:39.56 +58:27:14.6
129.47662 -3.77808 galactic Cas Second-epoch detections are separated by 1.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:41:39.56 +58:27:14.6 (user input) | T | P | (position from user input) J-Ks=0.952+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:39.56 +58:27:14.6: 12.03 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:39.56 +58:27:14.6: 14.48 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.47 +/- 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!
TCP 2026 06 20.4200* 01 41 39.56 +58 27 14.6 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.67 02:12:28.07 +59:37:07.8
133.02128 -1.65622 galactic Cas Second-epoch detections are separated by 2.8" and 3.6 pix
The object was found in VSX17" Gaia DR3 507310408755164160
Type: ROT
# Max. Min./Amp. JD0 Period
15.460 G 15.520 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:12:28.07 +59:37:07.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:12:28.07 +59:37:07.8: 14.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.37 +/- 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 20.4200* 02 12 28.07 +59 37 07.8 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507310408755164160,2461211.9200,11.67,0.05,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
Gaia DR3 507310408755164160 20260620.4200 11.67CV 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 20.4200 2461211.9200 11.56 01:46:38.09 +60:08:58.0
129.75434 -1.98912 galactic Cas Second-epoch detections are separated by 4.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.6591+60.1406 | 01:46:38.19 +60:08:26.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.09 +60:08:58.0: 13.21 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:38.09 +60:08:58.0: 14.37 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.28 +/- 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 20.4200* 01 46 38.09 +60 08 58.0 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.6591+60.1406,2461211.9200,11.56,0.05,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
ATO J026.6591+60.1406 20260620.4200 11.56CV 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 20.4200 2461211.9200 11.53 02:19:30.65 +64:32:24.3
132.22154 3.26866 galactic Cas Second-epoch detections are separated by 1.3" and 3.3 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 | 02:19:30.65 +64:32:24.3 (user input) | T | P | (position from user input) J-Ks=0.525+/-0.040 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:30.65 +64:32:24.3: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:30.65 +64:32:24.3: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 02 19 30.65 +64 32 24.3 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.53,0.05,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
target 20260620.4200 11.53CV 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 20.4200 2461211.9200 11.59 02:13:06.76 +59:49:48.1
133.03322 -1.43024 galactic Cas Second-epoch detections are separated by 0.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:13:06.76 +59:49:48.1 (user input) | T | P | (position from user input) J-Ks=0.455+/-0.040 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:06.76 +59:49:48.1: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:06.76 +59:49:48.1: 14.30 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.30 +/- 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 20.4200* 02 13 06.76 +59 49 48.1 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4200 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 20.4200 2461211.9200 11.47 01:38:35.76 +64:48:51.6
127.92435 2.40068 galactic Cas Second-epoch detections are separated by 2.4" and 3.2 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 513065252614504576 | 01:38:36.54 +64:48:07.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.864+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:35.76 +64:48:51.6: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:35.76 +64:48:51.6: 14.27 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.27 +/- 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 20.4200* 01 38 35.76 +64 48 51.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 513065252614504576,2461211.9200,11.47,0.05,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
Gaia DR3 513065252614504576 20260620.4200 11.47CV 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 20.4200 2461211.9200 11.56 01:48:17.78 +60:40:24.8
129.84171 -1.43313 galactic Cas Second-epoch detections are separated by 1.0" and 3.5 pix
The object was found in VSX10" Gaia DR3 511167701701981184
Type: ROT
# Max. Min./Amp. JD0 Period
17.690 G 17.800 G 10.278600000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:17.78 +60:40:24.8: 12.88 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:17.78 +60:40:24.8: 14.24 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 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 20.4200* 01 48 17.78 +60 40 24.8 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511167701701981184,2461211.9200,11.56,0.05,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
Gaia DR3 511167701701981184 20260620.4200 11.56CV 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 20.4200 2461211.9200 11.60 01:17:06.09 +60:05:14.0
126.12973 -2.62509 galactic Cas Second-epoch detections are separated by 2.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510335680638017792 | 01:17:05.01 +60:05:37.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:06.09 +60:05:14.0: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:06.09 +60:05:14.0: 14.44 +/- 0.08 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 20.4200* 01 17 06.09 +60 05 14.0 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510335680638017792,2461211.9200,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510335680638017792 20260620.4200 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.51 01:54:07.61 +61:05:02.2
130.43805 -0.87089 galactic Cas Second-epoch detections are separated by 0.3" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:54:07.61 +61:05:02.2 (user input) | T | P | (position from user input) J-Ks=0.446+/-0.043 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:07.61 +61:05:02.2: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:07.61 +61:05:02.2: 14.23 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 54 07.61 +61 05 02.2 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.54 01:38:40.34 +64:31:56.1
127.98379 2.12480 galactic Cas Second-epoch detections are separated by 0.3" and 3.2 pix
The object was found in VSX20" Gaia DR3 512964166264921856
Type: YSO
# Max. Min./Amp. JD0 Period
17.250 G 17.380 G M
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:40.34 +64:31:56.1: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:40.34 +64:31:56.1: 14.14 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 38 40.34 +64 31 56.1 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512964166264921856,2461211.9200,11.54,0.05,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 512964166264921856 20260620.4200 11.54CV 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 20.4200 2461211.9200 11.59 01:26:22.39 +61:16:26.2
127.11817 -1.31353 galactic Cas Second-epoch detections are separated by 1.8" and 3.6 pix
The object was found in VSX 1" Gaia DR3 510682198601256192
Type: RS
# Max. Min./Amp. JD0 Period
14.670 G 14.770 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:22.39 +61:16:26.2: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:22.39 +61:16:26.2: 14.44 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.44 +/- 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 20.4200* 01 26 22.39 +61 16 26.2 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510682198601256192,2461211.9200,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 510682198601256192 20260620.4200 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 20.4200 2461211.9200 11.71 01:34:06.30 +59:58:54.9
128.24993 -2.44854 galactic Cas Second-epoch detections are separated by 0.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:34:06.30 +59:58:54.9 (user input) | T | P | (position from user input) J-Ks=0.739+/-0.037 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:06.30 +59:58:54.9: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:06.30 +59:58:54.9: 14.57 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.57 +/- 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 20.4200* 01 34 06.30 +59 58 54.9 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.59 01:50:44.27 +59:04:33.9
130.49751 -2.92184 galactic Cas Second-epoch detections are separated by 0.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506518863460113152 | 01:50:42.44 +59:04:03.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:44.27 +59:04:33.9: 12.52 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:44.27 +59:04:33.9: 14.41 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.11 +/- 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 20.4200* 01 50 44.27 +59 04 33.9 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506518863460113152,2461211.9200,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 506518863460113152 20260620.4200 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 20.4200 2461211.9200 11.91 01:56:50.95 +59:00:21.1
131.27837 -2.80181 galactic Cas Second-epoch detections are separated by 5.5" and 2.6 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 | ZTF J015651.97+590057.5 | 01:56:53.98 +59:00:40.4 (Gaia DR3) | EB: (local) | 2458538.60540 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.272+/-0.049 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:50.95 +59:00:21.1: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:50.95 +59:00:21.1: 14.66 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 56 50.95 +59 00 21.1 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
ZTF J015651.97+590057.5,2461211.9200,11.91,0.05,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
ZTF J015651.97+590057.5 20260620.4200 11.91CV 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 20.4200 2461211.9200 11.87 01:40:27.31 +58:35:19.4
129.29616 -3.67603 galactic Cas Second-epoch detections are separated by 1.8" and 3.1 pix
The object was found in VSX17" Gaia DR3 509063202085906688
Type: RS
# Max. Min./Amp. JD0 Period
15.310 G 15.390 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:27.31 +58:35:19.4: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:27.31 +58:35:19.4: 14.83 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.83 +/- 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 20.4200* 01 40 27.31 +58 35 19.4 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509063202085906688,2461211.9200,11.87,0.05,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
Gaia DR3 509063202085906688 20260620.4200 11.87CV 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 20.4200 2461211.9200 11.86 01:58:56.43 +65:19:00.3
129.90696 3.36320 galactic Cas Second-epoch detections are separated by 2.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:58:56.43 +65:19:00.3 (user input) | T | P | (position from user input) J-Ks=0.286+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:56.43 +65:19:00.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:56.43 +65:19:00.3: 15.04 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.04 +/- 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 20.4200* 01 58 56.43 +65 19 00.3 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
target,2461211.9200,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.64 01:58:46.64 +60:45:03.9
131.06835 -1.05246 galactic Cas Second-epoch detections are separated by 1.8" and 3.5 pix
The object was found in VSX24" Gaia DR3 508026740578798208
Type: ROT
# Max. Min./Amp. JD0 Period
15.330 G 15.370 G M
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:46.64 +60:45:03.9: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:46.64 +60:45:03.9: 14.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.19 +/- 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 20.4200* 01 58 46.64 +60 45 03.9 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508026740578798208,2461211.9200,11.64,0.05,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
Gaia DR3 508026740578798208 20260620.4200 11.64CV 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 20.4200 2461211.9200 11.78 01:27:06.87 +61:26:15.3
127.18384 -1.13929 galactic Cas Second-epoch detections are separated by 2.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:27:06.87 +61:26:15.3 (user input) | T | P | (position from user input) J-Ks=0.535+/-0.040 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:06.87 +61:26:15.3: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:06.87 +61:26:15.3: 14.77 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.77 +/- 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 20.4200* 01 27 06.87 +61 26 15.3 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.78CV 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 20.4200 2461211.9200 11.80 01:20:49.30 +59:05:42.6
126.70457 -3.56118 galactic Cas Second-epoch detections are separated by 0.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:20:49.30 +59:05:42.6 (user input) | T | P | (position from user input) J-Ks=0.296+/-0.075 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:49.30 +59:05:42.6: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:49.30 +59:05:42.6: 14.81 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.81 +/- 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 20.4200* 01 20 49.30 +59 05 42.6 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.9200,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.90 01:16:20.04 +60:08:56.4
126.02844 -2.57298 galactic Cas Second-epoch detections are separated by 1.8" and 3.3 pix
The object was found in VSX 1" Gaia DR3 510339593344873472
Type: ROT
# Max. Min./Amp. JD0 Period
14.590 G 14.640 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:20.04 +60:08:56.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:20.04 +60:08:56.4: 14.99 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.99 +/- 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 20.4200* 01 16 20.04 +60 08 56.4 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510339593344873472,2461211.9200,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510339593344873472 20260620.4200 11.90CV 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 20.4200 2461211.9200 11.82 01:41:40.36 +62:34:09.1
128.68090 0.25950 galactic Cas Second-epoch detections are separated by 3.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511660484767387136 | 01:41:35.49 +62:34:37.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.349+/-0.041 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:40.36 +62:34:09.1: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:40.36 +62:34:09.1: 14.61 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 41 40.36 +62 34 09.1 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511660484767387136,2461211.9200,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511660484767387136 20260620.4200 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 11.81 01:28:14.72 +60:19:21.0
127.47654 -2.22406 galactic Cas Second-epoch detections are separated by 1.0" and 3.5 pix
The object was found in VSX16" Gaia DR3 510216005670888320
Type: ROT
# Max. Min./Amp. JD0 Period
17.120 G 17.200 G 3.707550000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:14.72 +60:19:21.0: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:14.72 +60:19:21.0: 14.69 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.69 +/- 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 20.4200* 01 28 14.72 +60 19 21.0 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510216005670888320,2461211.9200,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510216005670888320 20260620.4200 11.81CV 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 20.4200 2461211.9200 11.91 01:48:47.41 +58:57:20.8
130.27993 -3.09532 galactic Cas Second-epoch detections are separated by 1.7" and 3.2 pix
The object was found in VSX13" ZTF J014846.35+585710.4
Type: SR
# Max. Min./Amp. JD0 Period
17.221 g Y 0.891 g 2458486.60390 282.148464900000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:47.41 +58:57:20.8: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:47.41 +58:57:20.8: 14.76 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.76 +/- 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 20.4200* 01 48 47.41 +58 57 20.8 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
ZTF J014846.35+585710.4,2461211.9200,11.91,0.05,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
ZTF J014846.35+585710.4 20260620.4200 11.91CV 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 20.4200 2461211.9200 11.99 02:00:31.55 +62:35:42.1
130.78726 0.78169 galactic Cas Second-epoch detections are separated by 1.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:00:31.55 +62:35:42.1 (user input) | T | P | (position from user input) J-Ks=0.925+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:31.55 +62:35:42.1: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:31.55 +62:35:42.1: 14.90 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.90 +/- 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 20.4200* 02 00 31.55 +62 35 42.1 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,2461211.9200,11.99,0.05,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 20260620.4200 11.99CV 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 20.4200 2461211.9200 11.88 01:45:00.28 +59:26:56.2
129.70051 -2.71701 galactic Cas Second-epoch detections are separated by 1.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:45:00.28 +59:26:56.2 (user input) | T | P | (position from user input) J-Ks=0.729+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:00.28 +59:26:56.2: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:00.28 +59:26:56.2: 15.09 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.09 +/- 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 20.4200* 01 45 00.28 +59 26 56.2 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
target,2461211.9200,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 11.88CV 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 20.4200 2461211.9200 12.00 01:23:52.18 +60:52:55.6
126.86907 -1.74147 galactic Cas Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:23:52.18 +60:52:55.6 (user input) | T | P | (position from user input) J-Ks=0.858+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:52.18 +60:52:55.6: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:52.18 +60:52:55.6: 14.83 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.83 +/- 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 20.4200* 01 23 52.18 +60 52 55.6 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,2461211.9200,12.00,0.05,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
target 20260620.4200 12.00CV 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 20.4200 2461211.9200 12.05 01:45:41.64 +60:27:33.5
129.57508 -1.71075 galactic Cas Second-epoch detections are separated by 1.8" and 3.2 pix
The object was found in VSX23" ZTF J014540.43+602755.0
Type: BY
# Max. Min./Amp. JD0 Period
17.856 r Y 0.096 r 2458343.97890 6.103808900000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:41.64 +60:27:33.5: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:41.64 +60:27:33.5: 15.21 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.21 +/- 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 20.4200* 01 45 41.64 +60 27 33.5 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J014540.43+602755.0,2461211.9200,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J014540.43+602755.0 20260620.4200 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 12.11 01:29:04.21 +61:34:53.8
127.39432 -0.96365 galactic Cas Second-epoch detections are separated by 7.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:29:04.21 +61:34:53.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:04.21 +61:34:53.8: 12.85 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:04.21 +61:34:53.8: 14.93 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.30 +/- 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 20.4200* 01 29 04.21 +61 34 53.8 12.1 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,2461211.9200,12.11,0.05,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 20260620.4200 12.11CV 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 20.4200 2461211.9200 12.16 01:34:30.28 +61:09:14.8
128.10417 -1.28440 galactic Cas Second-epoch detections are separated by 1.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:34:30.28 +61:09:14.8 (user input) | T | P | (position from user input) J-Ks=0.296+/-0.051 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:30.28 +61:09:14.8: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:30.28 +61:09:14.8: 15.14 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.14 +/- 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 20.4200* 01 34 30.28 +61 09 14.8 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,2461211.9200,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 12.16CV 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 20.4200 2461211.9200 12.25 01:37:32.86 +60:29:03.7
128.58501 -1.88030 galactic Cas Second-epoch detections are separated by 1.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:37:32.86 +60:29:03.7 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:32.86 +60:29:03.7: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:32.86 +60:29:03.7: 15.17 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.17 +/- 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 20.4200* 01 37 32.86 +60 29 03.7 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,2461211.9200,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 12.12 01:29:43.49 +58:27:52.9
127.93364 -4.03475 galactic Cas Second-epoch detections are separated by 1.8" and 3.7 pix
The object was found in VSX19" Gaia DR3 509210261773768448
Type: S
# Max. Min./Amp. JD0 Period
17.320 G 18.090 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:43.49 +58:27:52.9: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:43.49 +58:27:52.9: 15.11 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.11 +/- 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 20.4200* 01 29 43.49 +58 27 52.9 12.1 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 509210261773768448,2461211.9200,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509210261773768448 20260620.4200 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4200 2461211.9200 12.07 01:22:41.20 +59:08:56.9
126.93628 -3.47944 galactic Cas Second-epoch detections are separated by 1.3" and 3.3 pix
The object was found in VSX 3" Gaia DR3 413977470877214080
Type: ROT
# Max. Min./Amp. JD0 Period
17.610 G 17.660 G 5.201000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:41.20 +59:08:56.9: 12.91 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:41.20 +59:08:56.9: 14.85 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.50 +/- 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 20.4200* 01 22 41.20 +59 08 56.9 12.1 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 413977470877214080,2461211.9200,12.07,0.05,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 413977470877214080 20260620.4200 12.07CV 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 20.4200 2461211.9200 12.10 01:25:27.61 +59:53:35.3
127.19141 -2.69694 galactic Cas Second-epoch detections are separated by 2.6" and 3.9 pix
The object was found in VSX 1" Gaia DR3 510098151767785984
Type: ROT
# Max. Min./Amp. JD0 Period
14.630 G 14.670 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:27.61 +59:53:35.3: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:27.61 +59:53:35.3: 15.27 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.27 +/- 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 20.4200* 01 25 27.61 +59 53 35.3 12.1 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 510098151767785984,2461211.9200,12.10,0.05,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
Gaia DR3 510098151767785984 20260620.4200 12.10CV 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 20.4200 2461211.9200 12.12 01:26:31.68 +62:18:33.2
126.99605 -0.28531 galactic Cas Second-epoch detections are separated by 1.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:26:31.68 +62:18:33.2 (user input) | T | P | (position from user input) J-Ks=0.590+/-0.040 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:31.68 +62:18:33.2: 11.70 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:31.68 +62:18:33.2: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.4200* 01 26 31.68 +62 18 33.2 12.1 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,2461211.9200,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.4200 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461211.92022163 20.06.2026 10:04:57.149 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 10 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): 26338
Objects passed selection criteria: 26223
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 19887.2
Average stars matched: 18221.2 (91.6228 %)
Memory usage VmPeak: 128424 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 07:22:49 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461211.92022163 20.06.2026 10:04:57.149 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 418
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 175 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): 195545
Objects passed selection criteria: 194983
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: 154417
Average stars matched: 141018 (91.323 %)
Memory usage VmPeak: 2065996 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 07:28:34 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.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: 2461211.91975792
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits'
wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:43:35.746 +62:00:07.25 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:43:35.746 +62:00:07.25
Angular distance between the image centers 0.1323 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:43:38.303 +61:59:58.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:43:38.303 +61:59:58.36
Angular distance between the image centers 0.1369 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:43:35.746 +62:00:07.25
Second-epoch second image center 01:43:38.303 +61:59:58.36
Angular distance between the image centers 0.00558 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.M14eoErru0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.JDgF56glLL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits &> /tmp/tmp.b50h29E9W9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits &> /tmp/tmp.e6cWTY4a4O
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.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-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat' -> 'wcsmag.cat'
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929150
a=0.000000 b=1.000000 c=22.929150
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=5.8)
Read 31681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.0659 to 45.7628 deg, Dec +55.3336 to +67.4023 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.0659 to 45.7628 deg, Dec 55.3336 to 67.4023 deg
Loaded 26179 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 14497 out of 16269 total matches.
Matched with Tycho-2 16269 out of 31681 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
14.8 mag. fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits
14.8 mag. fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (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.M14eoErru0 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, passed=31559
Got 31559 stars (including 27744 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
util/solve_plate_with_UCAC5 got 31559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 280 matched stars entering correct_measured_positions(), 228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 266 matched stars entering correct_measured_positions(), 9996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 403 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 337 matched stars entering correct_measured_positions(), 10041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.88"
Excluding outliers - 331 stars left (next iteration limit 292)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=331 sigma_overall_arcsec=7.729 sigma_q1_arcsec=31.346 sigma_q2_arcsec=12.794 sigma_q3_arcsec=22.422 sigma_q4_arcsec=4.202 n_q1=16 n_q2=97 n_q3=37 n_q4=181 worst_quadrant_to_overall_ratio=4.055
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JDgF56glLL (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, passed=31681
Got 31681 stars (including 27947 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat
util/solve_plate_with_UCAC5 got 31681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=973 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.346 n_q1=119 n_q2=244 n_q3=303 n_q4=307 worst_quadrant_to_overall_ratio=1.316
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.b50h29E9W9 (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-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.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-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.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-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1891, passed=21402
Got 21402 stars (including 19483 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits.wcscat
util/solve_plate_with_UCAC5 got 21402 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 20832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 20833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 20833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits N_match=974 sigma_overall_arcsec=0.627 sigma_q1_arcsec=0.540 sigma_q2_arcsec=0.631 sigma_q3_arcsec=0.711 sigma_q4_arcsec=0.542 n_q1=232 n_q2=360 n_q3=202 n_q4=180 worst_quadrant_to_overall_ratio=1.134
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.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.e6cWTY4a4O (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-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.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-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.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-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2024, passed=21171
Got 21171 stars (including 19125 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits.wcscat
util/solve_plate_with_UCAC5 got 21171 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 20635 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 20633 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 20633 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits N_match=971 sigma_overall_arcsec=0.657 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.682 sigma_q3_arcsec=0.743 sigma_q4_arcsec=0.702 n_q1=246 n_q2=364 n_q3=190 n_q4=171 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.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-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=7.729 worst_q_ratio=4.055
ref2=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=0.405 worst_q_ratio=1.316
new1=fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits sigma_overall=0.627 worst_q_ratio=1.134
new2=fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits sigma_overall=0.657 worst_q_ratio=1.130
reference average sigma_overall=4.067 worst_q_ratio=2.6855
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018_astrometric_residuals.png (331 matched stars from wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.16 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019_astrometric_residuals.png (973 matched stars from wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462_astrometric_residuals.png (974 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.57 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463_astrometric_residuals.png (971 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.59 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-17_20.00sec_5.00C_LIGHT_0462.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-03-Q2b1x1_063101_TTUQ2b1x1_1328212_clZM9BzM/wcs_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:13.11 +63:30:31.4: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:24.61 +62:28:18.8: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:06.11 +63:57:55.9: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.04 +59:15:34.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:13.11 +63:30:31.4: 12.03 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:06.11 +63:57:55.9: 12.31 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:24.61 +62:28:18.8: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter REJECTED candidate at 01:52:13.11 +63:30:31.4: ref_mag=12.03 +/- 0.01 new_mean_mag=12.1380 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:55:06.11 +63:57:55.9: ref_mag=12.31 +/- 0.01 new_mean_mag=12.2190 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:11:24.61 +62:28:18.8: ref_mag=12.24 +/- 0.01 new_mean_mag=12.2792 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.04 +59:15:34.2: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter KEPT candidate at 01:56:38.04 +59:15:34.2: ref_mag=9.75 +/- 0.00 new_mean_mag=8.8178 delta=0.94 (need > 0.90)
Adding exclusion_list_local.txt__out20109.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 51605_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 51605_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
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Considering the candidate 54547_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 54547_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:46:08.68 +61:12:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55768_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 55768_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
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Considering the candidate 56121_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 56121_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
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Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 08339_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
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Considering the candidate 247773_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247773_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247774_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247774_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247775_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247775_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247777_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247777_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247780_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247780_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247785_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247785_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247790_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247790_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247791_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247791_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247792_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247792_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247793_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247793_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247795_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247795_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247811_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247811_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247821_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247821_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247824_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247824_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247825_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247825_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247827_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247827_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247831_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247831_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247833_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247833_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247834_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247834_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247837_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247837_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247839_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247839_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247840_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247840_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247842_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247842_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247844_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247844_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247846_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247846_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247848_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247848_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247849_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247849_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247852_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247852_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247855_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247855_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:30:06.76 +61:51:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247856_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247856_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247862_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247862_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247869_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247869_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247870_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247870_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:45:21.45 +65:13:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247874_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247874_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247877_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247877_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247878_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247878_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247879_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247879_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 247881_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247881_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247882_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247882_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247885_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247885_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247886_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247886_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247888_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247888_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247894_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247894_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247895_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247895_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247896_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247896_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247899_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247899_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247901_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247901_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:10:03.18 +57:48:13.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247904_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247904_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247905_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247905_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247907_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247907_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247908_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247908_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:33:01.59 +59:16:33.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247910_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247910_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:14:01.31 +57:40:46.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247911_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247911_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247913_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247913_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:17:40.65 +58:13:26.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247918_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247918_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:09:24.52 +58:01:32.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247926_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247926_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247928_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247928_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247932_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247932_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247933_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247933_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247936_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247936_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247938_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247938_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247942_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247942_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247943_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247943_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247946_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247946_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:07:41.81 +60:54:06.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247948_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247948_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247954_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247954_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:58:54.91 +58:10:50.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247955_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247955_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247958_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247958_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247959_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247959_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247960_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247960_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247961_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247961_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247964_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247964_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:00:46.20 +57:54:03.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247967_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247967_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247968_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247968_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247972_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247972_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247973_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247973_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:12:31.09 +61:17:18.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247979_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247979_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:07:35.00 +57:33:10.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247980_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 247980_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:33:35.21 +59:56:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247981_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247981_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247987_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247987_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247988_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247988_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247991_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247991_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247992_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247992_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247993_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247993_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247994_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247994_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247996_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 247996_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248001_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 248001_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248002_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248002_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:07:34.12 +60:52:43.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248005_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248005_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:18:38.95 +64:37:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248006_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 248006_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248012_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248012_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:19:24.14 +58:26:40.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248015_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248015_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:05:57.09 +63:03:31.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248016_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248016_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:09:47.68 +58:11:57.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248017_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 248017_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248018_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248018_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248023_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 248023_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248025_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248025_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:10:37.58 +57:22:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248028_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248028_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:03:21.74 +57:48:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248029_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248029_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:39:04.37 +61:53:24.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248031_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 248031_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248032_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248032_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:14:45.26 +60:30:04.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248033_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 248033_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248036_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248036_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:07:08.03 +57:44:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248037_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248037_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:12:41.01 +61:20:37.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248038_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248038_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:25:26.60 +60:57:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248039_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 248039_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 248041_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 248041_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 248043_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 248043_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 248044_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248044_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:15:56.00 +58:23:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248045_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248045_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:43:59.18 +61:55:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248046_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248046_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:55:14.60 +59:32:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248047_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248047_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:15:16.90 +57:28:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248048_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248048_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:20:24.43 +59:10:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248050_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248050_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:15:30.59 +63:53:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248051_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248051_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:19:48.72 +61:38:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248054_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248054_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:23:56.48 +62:06:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248055_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 248055_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 248056_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248056_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:51:35.74 +57:52:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248057_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248057_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:22:08.40 +60:22:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248060_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248060_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:16:01.12 +62:41:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248061_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 248061_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:47:13.11 +57:44:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249082_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 249082_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 250762_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 250762_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 251561_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 251561_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:44:02.07 +61:53:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251865_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 251865_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:38:00.47 +57:56:45.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252200_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 252200_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:19:11.14 +58:20:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252881_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 252881_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:40:01.39 +60:52:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252952_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 252952_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 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 253424_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 253424_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:26:41.14 +60:46:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254559_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 254559_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:28:15.49 +58:44:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256012_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 256012_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:44:17.77 +61:53:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256340_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 256340_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:43:53.17 +61:53:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256832_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 256832_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:16:08.72 +58:49:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257063_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 257063_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:25:50.37 +61:06:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257125_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 257125_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:33:59.40 +58:28:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257151_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 257151_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:23:23.64 +63:36:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257265_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 257265_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:15:58.88 +63:12:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257851_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 257851_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:44:32.37 +58:45:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257972_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 257972_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:00:36.79 +58:30:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258021_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 258021_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:11:23.02 +61:21:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258193_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 258193_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 258356_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 258356_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:26:15.45 +60:37:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258414_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 258414_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:13:30.07 +58:34:24.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 258657_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 258657_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:02:54.77 +64:25:00.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 258815_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 258815_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 259535_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 259535_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:13:36.00 +57:52:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259665_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 259665_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:58:04.25 +57:58:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259685_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 259685_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:19:03.91 +63:57:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259835_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 259835_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:16:05.18 +58:49:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259865_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 259865_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 259963_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 259963_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 260011_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 260011_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:42:33.05 +63:52:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260377_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 260377_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:26:35.89 +57:57:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260404_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 260404_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:43:07.00 +58:57:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260439_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 260439_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:10:23.82 +60:01:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260558_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 260558_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:35:50.58 +61:27:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260774_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 260774_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:08:30.38 +58:24:18.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 260934_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 260934_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:49:34.31 +61:03:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261161_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 261161_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:15:49.02 +59:33:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261302_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 261302_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 261463_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 261463_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:01:15.21 +59:23:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261546_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 261546_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:14:29.92 +63:16:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261607_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 261607_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:02:54.00 +60:15:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261893_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 261893_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:29:32.87 +63:19:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261920_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 261920_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:09:09.32 +61:37:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262161_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 262161_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 262163_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 262163_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:06:23.57 +62:44:03.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262228_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 262228_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:02:50.36 +60:14:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262266_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 262266_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:19:41.58 +62:51:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262728_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 262728_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:11:35.94 +57:37:15.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262820_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 262820_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:44:56.62 +59:46:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262933_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 262933_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:34:34.47 +65:48:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262963_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 262963_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:54:34.90 +59:52:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263046_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263046_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:55:53.04 +64:15:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263048_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263048_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:38:12.02 +61:01:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263065_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263065_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:43:12.90 +64:00:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263094_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263094_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:48:39.89 +59:09:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263141_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263141_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:37:41.50 +58:37:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263144_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263144_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:18:04.25 +65:36:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263159_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263159_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:38:34.03 +58:07:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263233_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263233_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
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Considering the candidate 263284_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263284_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:37:13.50 +58:38:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263311_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263311_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 263324_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263324_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:16:36.75 +64:56:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263444_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263444_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:46:18.33 +60:59:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263785_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263785_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:38:07.64 +61:01:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263824_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 263824_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 263835_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263835_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:23:07.64 +61:11:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263849_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 263849_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:03:25.27 +57:50:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263922_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 263922_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 264215_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 264215_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:31:32.47 +61:02:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264222_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 264222_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:42:54.79 +64:01:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264255_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 264255_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:55:22.01 +64:02:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264311_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 264311_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:20:40.58 +60:23:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264446_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 264446_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:14:00.39 +61:42:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264458_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 264458_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:42:28.48 +58:17:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264559_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 264559_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:10:10.06 +59:08:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264617_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 264617_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:55:21.58 +59:26:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264823_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 264823_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 265065_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 265065_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:59:06.00 +59:55:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265216_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 265216_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:37:13.14 +58:38:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265256_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 265256_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 265301_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 265301_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:33:46.81 +62:31:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265307_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 265307_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:16:02.42 +60:36:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265451_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 265451_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 265466_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 265466_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:54:30.54 +59:06:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265527_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 265527_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 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 265533_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 265533_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:43:03.29 +58:57:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265558_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 265558_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:58:14.06 +60:03:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265604_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 265604_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 265605_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 265605_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:11:50.21 +59:02:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265719_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 265719_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 265731_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 265731_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:44:32.24 +61:36:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265770_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 265770_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 265834_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 265834_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 266019_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 266019_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 266165_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 266165_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 266167_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 266167_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:15:05.62 +64:08:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266184_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 266184_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:34:42.64 +58:42:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266248_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 266248_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 266324_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 266324_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 266415_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 266415_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:56:15.96 +60:00:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266450_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 266450_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:23:42.26 +63:43:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266476_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 266476_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266487_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 266487_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:00:35.62 +58:32:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266553_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 266553_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:36:07.56 +59:27:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266671_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 266671_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:27:04.13 +64:43:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266780_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 266780_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:56:25.40 +62:05:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266811_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 266811_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:54:26.83 +63:42:26.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 266833_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 266833_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 266994_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 266994_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 267026_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 267026_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267295_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 267295_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267342_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 267342_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267440_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 267440_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267479_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 267479_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:17:01.76 +63:21:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267723_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 267723_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:15:16.89 +59:21:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267824_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 267824_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267848_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 267848_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267912_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 267912_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267932_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 267932_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267952_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 267952_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:55:05.21 +59:57:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268023_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 268023_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:49:06.25 +65:23:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268183_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 268183_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268406_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 268406_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:02:40.28 +59:57:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268534_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 268534_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:27:56.36 +62:46:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268551_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 268551_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:13:35.50 +58:31:51.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 268621_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 268621_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
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Considering the candidate 268694_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 268694_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268757_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 268757_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268774_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 268774_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 268805_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 268805_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:54:05.74 +61:05:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268871_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 268871_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:31:48.55 +64:22:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268941_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 268941_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 269009_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 269009_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:42:49.60 +61:24:06.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 269193_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 269193_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 269220_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 269220_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:23:20.35 +62:03:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269575_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 269575_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 269618_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 269618_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 269657_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 269657_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 269986_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 269986_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 270064_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 270064_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:54:57.13 +63:41:22.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 270116_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 270116_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 270137_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 270137_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 270161_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 270161_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 270354_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 270354_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 270550_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 270550_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:38:56.98 +63:28:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270561_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 270561_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 270598_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 270598_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 270783_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 270783_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 270850_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 270850_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 270866_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 270866_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 271378_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 271378_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 271625_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 271625_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:46:23.72 +59:12:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271736_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 271736_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 271906_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 271906_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 271918_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 271918_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:40:47.27 +65:05:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271979_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 271979_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 272099_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 272099_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:41:41.14 +57:56:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272230_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 272230_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:47:18.81 +58:31:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272316_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 272316_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:53:03.05 +60:26:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272437_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 272437_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 272469_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 272469_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 272759_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 272759_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 273195_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 273195_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 273391_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 273391_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 273499_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 273499_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 273605_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 273605_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 273652_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 273652_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 273685_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 273685_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 273806_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 273806_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 274155_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 274155_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 274182_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 274182_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
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Considering the candidate 274501_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 274501_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 274535_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 274535_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 274630_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 274630_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 274928_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 274928_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 275100_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 275100_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 275183_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 275183_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:23:24.77 +58:10:16.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 275302_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 275302_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 276059_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 276059_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 276828_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 276828_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 277371_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 277371_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 277572_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 277572_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 277855_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 277855_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 277968_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 277968_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
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Considering the candidate 278139_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 278139_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 278176_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 278176_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278505_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 278505_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 278896_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 278896_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278993_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 278993_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279200_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 279200_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 279456_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 279456_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 280083_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 280083_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280086_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 280086_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280135_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 280135_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280142_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 280142_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280371_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 280371_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280763_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 280763_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
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Considering the candidate 280793_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 280793_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280997_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 280997_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281026_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 281026_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281035_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 281035_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
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Considering the candidate 281057_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 281057_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281072_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 281072_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281173_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
Preparing report for the candidate 281173_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
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Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 72532_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:45:35.73 +63:07:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 112593_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:21:55.25 +61:20:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 70271_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:20:32.46 +62:32:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156692_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 156692_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:56:38.05 +59:15:34.1 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76113_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 76113_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 02:02:02.24 +62:41:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463
The candidate 39378_fd_Cas-03-Q2b1x1_2026-06-20_05-04-57_20.00sec_4.90C_LIGHT_0463 did not pass the final checks
**** FOUND 01:47:55.66 +64:32:55.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 353s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:56:38.04 +59:15:34.2
01:50:16.38 +58:52:59.7
01:43:24.12 +61:12:07.8
01:16:40.37 +61:23:05.9
01:15:30.43 +60:45:22.6
01:24:06.20 +60:41:09.9
01:33:22.88 +61:41:09.1
01:30:06.40 +63:44:41.8
01:07:06.59 +57:40:47.8
01:16:23.35 +58:49:28.1
01:34:46.03 +62:04:51.5
01:07:33.61 +61:22:51.8
01:34:30.25 +59:54:23.8
01:53:04.68 +62:00:26.5
01:26:38.72 +62:48:30.9
01:46:36.58 +64:06:19.3
01:22:13.69 +62:32:56.6
01:49:40.08 +59:34:16.8
01:12:01.47 +58:29:48.8
01:08:47.54 +57:50:27.2
01:33:40.63 +59:42:23.5
01:55:28.44 +63:18:55.9
02:14:26.26 +61:46:49.0
01:25:02.98 +65:27:16.3
01:25:57.02 +58:48:08.8
01:32:22.31 +62:14:57.8
01:39:10.54 +58:03:36.0
01:32:25.36 +61:29:15.7
01:04:35.20 +62:44:33.3
01:34:59.27 +60:09:34.6
01:06:15.89 +57:53:25.3
01:30:59.89 +63:14:37.6
01:48:13.35 +59:51:32.6
01:12:41.26 +61:18:08.1
01:45:19.33 +61:13:08.4
01:37:23.81 +59:20:12.3
01:52:03.58 +60:31:38.5
01:43:20.74 +61:14:37.9
01:22:50.56 +58:12:42.7
01:07:36.88 +58:09:25.4
01:45:15.39 +61:13:52.8
01:05:04.67 +63:39:45.2
01:19:12.21 +60:58:37.9
01:36:09.46 +61:08:51.7
01:56:27.23 +65:22:09.4
01:06:24.44 +60:07:16.0
01:22:33.26 +60:44:41.1
01:25:00.87 +62:50:52.5
01:34:10.01 +60:13:05.8
01:05:53.88 +59:06:23.6
01:38:59.12 +61:08:53.2
01:21:11.22 +59:33:02.0
01:30:00.95 +60:10:50.0
02:13:37.67 +61:10:28.1
01:23:56.99 +62:15:27.9
01:23:53.55 +58:03:34.7
01:32:10.98 +59:36:03.5
01:34:57.93 +61:00:13.6
01:33:20.05 +62:33:20.9
01:40:18.20 +61:21:06.0
01:08:25.67 +59:48:03.7
01:08:39.25 +60:32:41.3
01:21:45.32 +58:34:15.3
01:07:01.87 +59:46:17.1
01:55:46.61 +57:57:42.5
01:57:29.26 +60:09:19.2
01:07:39.17 +59:59:18.0
01:26:05.62 +59:01:15.0
01:20:42.12 +59:35:05.3
01:27:32.56 +64:34:36.1
01:12:59.70 +57:34:09.5
02:03:59.13 +59:34:48.0
01:25:42.78 +58:50:45.7
01:24:55.09 +59:41:48.4
01:06:13.18 +59:33:47.5
01:25:27.54 +59:27:15.5
01:51:47.29 +58:37:55.3
01:12:00.92 +64:42:18.2
01:08:15.48 +61:15:06.7
01:26:37.92 +60:38:02.4
01:43:27.31 +58:38:07.0
01:29:48.25 +63:19:35.8
02:00:06.64 +59:00:32.8
01:07:45.52 +57:45:04.8
01:21:40.06 +61:36:42.7
01:30:34.37 +59:44:32.2
01:35:27.62 +60:33:47.4
01:37:17.59 +57:50:54.6
01:34:16.42 +60:57:34.9
01:17:15.14 +58:35:37.1
01:25:45.80 +59:01:22.7
01:49:15.82 +59:14:38.3
02:05:14.98 +63:02:37.2
01:26:39.09 +59:41:38.1
01:18:47.92 +59:08:14.7
01:07:31.84 +61:28:27.2
01:56:43.24 +58:07:17.9
01:31:23.12 +59:33:43.6
01:35:24.58 +60:39:29.9
01:20:45.05 +57:55:09.5
01:08:23.32 +61:35:09.9
01:19:08.73 +60:33:58.6
01:27:35.79 +57:57:00.7
02:00:26.68 +63:04:13.4
01:07:57.25 +63:37:29.5
01:35:25.03 +60:39:14.8
01:49:03.90 +61:04:19.4
01:23:31.47 +58:41:48.0
01:27:22.04 +58:51:39.5
01:10:34.59 +60:31:07.6
01:46:38.50 +60:07:33.1
01:18:28.11 +58:11:23.6
02:00:21.73 +64:56:38.5
01:51:09.35 +64:52:46.8
01:08:59.45 +60:47:21.1
01:14:41.44 +58:46:46.5
01:22:10.97 +59:09:03.5
02:16:07.78 +58:18:14.4
01:51:26.73 +57:51:36.7
02:21:38.04 +65:44:28.6
02:15:03.70 +58:28:54.2
01:09:22.61 +57:26:31.1
01:13:39.03 +58:10:51.2
01:22:23.90 +61:13:51.6
02:00:32.94 +59:40:07.3
01:38:05.83 +61:04:14.1
01:24:49.19 +59:47:15.9
02:16:27.39 +64:52:49.7
01:50:39.84 +62:00:56.4
01:41:34.52 +59:13:59.0
01:25:25.28 +58:19:59.4
01:06:55.34 +59:18:58.6
01:52:55.35 +59:33:31.4
02:02:25.08 +64:38:23.8
01:56:57.38 +63:00:32.5
01:59:34.04 +63:37:09.5
01:42:17.62 +63:24:23.7
01:38:34.72 +57:58:01.1
01:56:48.73 +61:52:37.5
01:52:55.29 +60:27:25.5
01:17:45.49 +57:34:01.3
02:08:50.63 +59:21:19.7
01:51:53.64 +63:26:20.9
01:23:46.56 +60:53:19.3
02:07:53.85 +58:37:40.7
01:33:30.69 +58:02:23.6
01:40:29.69 +60:46:50.2
01:40:21.93 +60:45:15.1
01:26:28.50 +59:41:36.9
01:29:20.11 +59:29:36.8
01:24:11.89 +59:17:51.8
01:19:29.32 +59:25:22.1
02:04:06.48 +60:14:18.0
01:25:25.32 +58:37:26.1
01:51:52.56 +60:27:42.9
02:09:40.63 +60:06:56.2
01:31:56.01 +59:26:39.7
01:44:29.89 +65:09:23.0
01:52:07.30 +59:13:07.9
01:29:33.79 +60:47:14.9
01:57:26.38 +63:23:42.4
01:19:11.94 +59:07:32.3
02:08:22.88 +64:18:53.9
01:41:39.56 +58:27:14.6
02:12:28.07 +59:37:07.8
01:46:38.09 +60:08:58.0
02:19:30.65 +64:32:24.3
02:13:06.76 +59:49:48.1
01:38:35.76 +64:48:51.6
01:48:17.78 +60:40:24.8
01:17:06.09 +60:05:14.0
01:54:07.61 +61:05:02.2
01:38:40.34 +64:31:56.1
01:26:22.39 +61:16:26.2
01:34:06.30 +59:58:54.9
01:50:44.27 +59:04:33.9
01:56:50.95 +59:00:21.1
01:40:27.31 +58:35:19.4
01:58:56.43 +65:19:00.3
01:58:46.64 +60:45:03.9
01:27:06.87 +61:26:15.3
01:20:49.30 +59:05:42.6
01:16:20.04 +60:08:56.4
01:41:40.36 +62:34:09.1
01:28:14.72 +60:19:21.0
01:48:47.41 +58:57:20.8
02:00:31.55 +62:35:42.1
01:45:00.28 +59:26:56.2
01:23:52.18 +60:52:55.6
01:45:41.64 +60:27:33.5
01:29:04.21 +61:34:53.8
01:34:30.28 +61:09:14.8
01:37:32.86 +60:29:03.7
01:29:43.49 +58:27:52.9
01:22:41.20 +59:08:56.9
01:25:27.61 +59:53:35.3
01:26:31.68 +62:18:33.2
########### Completed Cas-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:56:38.04 +59:15:34.2
01:50:16.38 +58:52:59.7
01:43:24.12 +61:12:07.8
01:16:40.37 +61:23:05.9
01:15:30.43 +60:45:22.6
01:24:06.20 +60:41:09.9
01:33:22.88 +61:41:09.1
01:30:06.40 +63:44:41.8
01:07:06.59 +57:40:47.8
01:16:23.35 +58:49:28.1
01:34:46.03 +62:04:51.5
01:07:33.61 +61:22:51.8
01:34:30.25 +59:54:23.8
01:53:04.68 +62:00:26.5
01:26:38.72 +62:48:30.9
01:46:36.58 +64:06:19.3
01:22:13.69 +62:32:56.6
01:49:40.08 +59:34:16.8
01:12:01.47 +58:29:48.8
01:08:47.54 +57:50:27.2
01:33:40.63 +59:42:23.5
01:55:28.44 +63:18:55.9
02:14:26.26 +61:46:49.0
01:25:02.98 +65:27:16.3
01:25:57.02 +58:48:08.8
01:32:22.31 +62:14:57.8
01:39:10.54 +58:03:36.0
01:32:25.36 +61:29:15.7
01:04:35.20 +62:44:33.3
01:34:59.27 +60:09:34.6
01:06:15.89 +57:53:25.3
01:30:59.89 +63:14:37.6
01:48:13.35 +59:51:32.6
01:12:41.26 +61:18:08.1
01:45:19.33 +61:13:08.4
01:37:23.81 +59:20:12.3
01:52:03.58 +60:31:38.5
01:43:20.74 +61:14:37.9
01:22:50.56 +58:12:42.7
01:07:36.88 +58:09:25.4
01:45:15.39 +61:13:52.8
01:05:04.67 +63:39:45.2
01:19:12.21 +60:58:37.9
01:36:09.46 +61:08:51.7
01:56:27.23 +65:22:09.4
01:06:24.44 +60:07:16.0
01:22:33.26 +60:44:41.1
01:25:00.87 +62:50:52.5
01:34:10.01 +60:13:05.8
01:05:53.88 +59:06:23.6
01:38:59.12 +61:08:53.2
01:21:11.22 +59:33:02.0
01:30:00.95 +60:10:50.0
02:13:37.67 +61:10:28.1
01:23:56.99 +62:15:27.9
01:23:53.55 +58:03:34.7
01:32:10.98 +59:36:03.5
01:34:57.93 +61:00:13.6
01:33:20.05 +62:33:20.9
01:40:18.20 +61:21:06.0
01:08:25.67 +59:48:03.7
01:08:39.25 +60:32:41.3
01:21:45.32 +58:34:15.3
01:07:01.87 +59:46:17.1
01:55:46.61 +57:57:42.5
01:57:29.26 +60:09:19.2
01:07:39.17 +59:59:18.0
01:26:05.62 +59:01:15.0
01:20:42.12 +59:35:05.3
01:27:32.56 +64:34:36.1
01:12:59.70 +57:34:09.5
02:03:59.13 +59:34:48.0
01:25:42.78 +58:50:45.7
01:24:55.09 +59:41:48.4
01:06:13.18 +59:33:47.5
01:25:27.54 +59:27:15.5
01:51:47.29 +58:37:55.3
01:12:00.92 +64:42:18.2
01:08:15.48 +61:15:06.7
01:26:37.92 +60:38:02.4
01:43:27.31 +58:38:07.0
01:29:48.25 +63:19:35.8
02:00:06.64 +59:00:32.8
01:07:45.52 +57:45:04.8
01:21:40.06 +61:36:42.7
01:30:34.37 +59:44:32.2
01:35:27.62 +60:33:47.4
01:37:17.59 +57:50:54.6
01:34:16.42 +60:57:34.9
01:17:15.14 +58:35:37.1
01:25:45.80 +59:01:22.7
01:49:15.82 +59:14:38.3
02:05:14.98 +63:02:37.2
01:26:39.09 +59:41:38.1
01:18:47.92 +59:08:14.7
01:07:31.84 +61:28:27.2
01:56:43.24 +58:07:17.9
01:31:23.12 +59:33:43.6
01:35:24.58 +60:39:29.9
01:20:45.05 +57:55:09.5
01:08:23.32 +61:35:09.9
01:19:08.73 +60:33:58.6
01:27:35.79 +57:57:00.7
02:00:26.68 +63:04:13.4
01:07:57.25 +63:37:29.5
01:35:25.03 +60:39:14.8
01:49:03.90 +61:04:19.4
01:23:31.47 +58:41:48.0
01:27:22.04 +58:51:39.5
01:10:34.59 +60:31:07.6
01:46:38.50 +60:07:33.1
01:18:28.11 +58:11:23.6
02:00:21.73 +64:56:38.5
01:51:09.35 +64:52:46.8
01:08:59.45 +60:47:21.1
01:14:41.44 +58:46:46.5
01:22:10.97 +59:09:03.5
02:16:07.78 +58:18:14.4
01:51:26.73 +57:51:36.7
02:21:38.04 +65:44:28.6
02:15:03.70 +58:28:54.2
01:09:22.61 +57:26:31.1
01:13:39.03 +58:10:51.2
01:22:23.90 +61:13:51.6
02:00:32.94 +59:40:07.3
01:38:05.83 +61:04:14.1
01:24:49.19 +59:47:15.9
02:16:27.39 +64:52:49.7
01:50:39.84 +62:00:56.4
01:41:34.52 +59:13:59.0
01:25:25.28 +58:19:59.4
01:06:55.34 +59:18:58.6
01:52:55.35 +59:33:31.4
02:02:25.08 +64:38:23.8
01:56:57.38 +63:00:32.5
01:59:34.04 +63:37:09.5
01:42:17.62 +63:24:23.7
01:38:34.72 +57:58:01.1
01:56:48.73 +61:52:37.5
01:52:55.29 +60:27:25.5
01:17:45.49 +57:34:01.3
02:08:50.63 +59:21:19.7
01:51:53.64 +63:26:20.9
01:23:46.56 +60:53:19.3
02:07:53.85 +58:37:40.7
01:33:30.69 +58:02:23.6
01:40:29.69 +60:46:50.2
01:40:21.93 +60:45:15.1
01:26:28.50 +59:41:36.9
01:29:20.11 +59:29:36.8
01:24:11.89 +59:17:51.8
01:19:29.32 +59:25:22.1
02:04:06.48 +60:14:18.0
01:25:25.32 +58:37:26.1
01:51:52.56 +60:27:42.9
02:09:40.63 +60:06:56.2
01:31:56.01 +59:26:39.7
01:44:29.89 +65:09:23.0
01:52:07.30 +59:13:07.9
01:29:33.79 +60:47:14.9
01:57:26.38 +63:23:42.4
01:19:11.94 +59:07:32.3
02:08:22.88 +64:18:53.9
01:41:39.56 +58:27:14.6
02:12:28.07 +59:37:07.8
01:46:38.09 +60:08:58.0
02:19:30.65 +64:32:24.3
02:13:06.76 +59:49:48.1
01:38:35.76 +64:48:51.6
01:48:17.78 +60:40:24.8
01:17:06.09 +60:05:14.0
01:54:07.61 +61:05:02.2
01:38:40.34 +64:31:56.1
01:26:22.39 +61:16:26.2
01:34:06.30 +59:58:54.9
01:50:44.27 +59:04:33.9
01:56:50.95 +59:00:21.1
01:40:27.31 +58:35:19.4
01:58:56.43 +65:19:00.3
01:58:46.64 +60:45:03.9
01:27:06.87 +61:26:15.3
01:20:49.30 +59:05:42.6
01:16:20.04 +60:08:56.4
01:41:40.36 +62:34:09.1
01:28:14.72 +60:19:21.0
01:48:47.41 +58:57:20.8
02:00:31.55 +62:35:42.1
01:45:00.28 +59:26:56.2
01:23:52.18 +60:52:55.6
01:45:41.64 +60:27:33.5
01:29:04.21 +61:34:53.8
01:34:30.28 +61:09:14.8
01:37:32.86 +60:29:03.7
01:29:43.49 +58:27:52.9
01:22:41.20 +59:08:56.9
01:25:27.61 +59:53:35.3
01:26:31.68 +62:18:33.2
###################################################################################
01:56:38.04 +59:15:34.2 -- not an asteroid (will add it to exclusion list)
01:50:16.38 +58:52:59.7 -- not an asteroid (will add it to exclusion list)
01:43:24.12 +61:12:07.8 -- not an asteroid (will add it to exclusion list)
01:16:40.37 +61:23:05.9 -- not an asteroid (will add it to exclusion list)
01:15:30.43 +60:45:22.6 -- not an asteroid (will add it to exclusion list)
01:24:06.20 +60:41:09.9 -- not an asteroid (will add it to exclusion list)
01:33:22.88 +61:41:09.1 -- not an asteroid (will add it to exclusion list)
01:30:06.40 +63:44:41.8 -- not an asteroid (will add it to exclusion list)
01:07:06.59 +57:40:47.8 -- not an asteroid (will add it to exclusion list)
01:16:23.35 +58:49:28.1 -- not an asteroid (will add it to exclusion list)
01:34:46.03 +62:04:51.5 -- not an asteroid (will add it to exclusion list)
01:07:33.61 +61:22:51.8 -- not an asteroid (will add it to exclusion list)
01:34:30.25 +59:54:23.8 -- not an asteroid (will add it to exclusion list)
01:53:04.68 +62:00:26.5 -- not an asteroid (will add it to exclusion list)
01:26:38.72 +62:48:30.9 -- not an asteroid (will add it to exclusion list)
01:46:36.58 +64:06:19.3 -- not an asteroid (will add it to exclusion list)
01:22:13.69 +62:32:56.6 -- not an asteroid (will add it to exclusion list)
01:49:40.08 +59:34:16.8 -- not an asteroid (will add it to exclusion list)
01:12:01.47 +58:29:48.8 -- not an asteroid (will add it to exclusion list)
01:08:47.54 +57:50:27.2 -- not an asteroid (will add it to exclusion list)
01:33:40.63 +59:42:23.5 -- not an asteroid (will add it to exclusion list)
01:55:28.44 +63:18:55.9 -- not an asteroid (will add it to exclusion list)
02:14:26.26 +61:46:49.0 -- not an asteroid (will add it to exclusion list)
01:25:02.98 +65:27:16.3 -- not an asteroid (will add it to exclusion list)
01:25:57.02 +58:48:08.8 -- not an asteroid (will add it to exclusion list)
01:32:22.31 +62:14:57.8 -- not an asteroid (will add it to exclusion list)
01:39:10.54 +58:03:36.0 -- not an asteroid (will add it to exclusion list)
01:32:25.36 +61:29:15.7 -- not an asteroid (will add it to exclusion list)
01:04:35.20 +62:44:33.3 -- not an asteroid (will add it to exclusion list)
01:34:59.27 +60:09:34.6 -- not an asteroid (will add it to exclusion list)
01:06:15.89 +57:53:25.3 -- not an asteroid (will add it to exclusion list)
01:30:59.89 +63:14:37.6 -- not an asteroid (will add it to exclusion list)
01:48:13.35 +59:51:32.6 -- not an asteroid (will add it to exclusion list)
01:12:41.26 +61:18:08.1 -- not an asteroid (will add it to exclusion list)
01:45:19.33 +61:13:08.4 -- not an asteroid (will add it to exclusion list)
01:37:23.81 +59:20:12.3 -- not an asteroid (will add it to exclusion list)
01:52:03.58 +60:31:38.5 -- not an asteroid (will add it to exclusion list)
01:43:20.74 +61:14:37.9 -- not an asteroid (will add it to exclusion list)
01:22:50.56 +58:12:42.7 -- not an asteroid (will add it to exclusion list)
01:07:36.88 +58:09:25.4 -- not an asteroid (will add it to exclusion list)
01:45:15.39 +61:13:52.8 -- not an asteroid (will add it to exclusion list)
01:05:04.67 +63:39:45.2 -- not an asteroid (will add it to exclusion list)
01:19:12.21 +60:58:37.9 -- not an asteroid (will add it to exclusion list)
01:36:09.46 +61:08:51.7 -- not an asteroid (will add it to exclusion list)
01:56:27.23 +65:22:09.4 -- not an asteroid (will add it to exclusion list)
01:06:24.44 +60:07:16.0 -- not an asteroid (will add it to exclusion list)
01:22:33.26 +60:44:41.1 -- not an asteroid (will add it to exclusion list)
01:25:00.87 +62:50:52.5 -- not an asteroid (will add it to exclusion list)
01:34:10.01 +60:13:05.8 -- not an asteroid (will add it to exclusion list)
01:05:53.88 +59:06:23.6 -- not an asteroid (will add it to exclusion list)
01:38:59.12 +61:08:53.2 -- not an asteroid (will add it to exclusion list)
01:21:11.22 +59:33:02.0 -- not an asteroid (will add it to exclusion list)
01:30:00.95 +60:10:50.0 -- not an asteroid (will add it to exclusion list)
02:13:37.67 +61:10:28.1 -- not an asteroid (will add it to exclusion list)
01:23:56.99 +62:15:27.9 -- not an asteroid (will add it to exclusion list)
01:23:53.55 +58:03:34.7 -- not an asteroid (will add it to exclusion list)
01:32:10.98 +59:36:03.5 -- not an asteroid (will add it to exclusion list)
01:34:57.93 +61:00:13.6 -- not an asteroid (will add it to exclusion list)
01:33:20.05 +62:33:20.9 -- not an asteroid (will add it to exclusion list)
01:40:18.20 +61:21:06.0 -- not an asteroid (will add it to exclusion list)
01:08:25.67 +59:48:03.7 -- not an asteroid (will add it to exclusion list)
01:08:39.25 +60:32:41.3 -- not an asteroid (will add it to exclusion list)
01:21:45.32 +58:34:15.3 -- not an asteroid (will add it to exclusion list)
01:07:01.87 +59:46:17.1 -- not an asteroid (will add it to exclusion list)
01:55:46.61 +57:57:42.5 -- not an asteroid (will add it to exclusion list)
01:57:29.26 +60:09:19.2 -- not an asteroid (will add it to exclusion list)
01:07:39.17 +59:59:18.0 -- not an asteroid (will add it to exclusion list)
01:26:05.62 +59:01:15.0 -- not an asteroid (will add it to exclusion list)
01:20:42.12 +59:35:05.3 -- not an asteroid (will add it to exclusion list)
01:27:32.56 +64:34:36.1 -- not an asteroid (will add it to exclusion list)
01:12:59.70 +57:34:09.5 -- not an asteroid (will add it to exclusion list)
02:03:59.13 +59:34:48.0 -- not an asteroid (will add it to exclusion list)
01:25:42.78 +58:50:45.7 -- not an asteroid (will add it to exclusion list)
01:24:55.09 +59:41:48.4 -- not an asteroid (will add it to exclusion list)
01:06:13.18 +59:33:47.5 -- not an asteroid (will add it to exclusion list)
01:25:27.54 +59:27:15.5 -- not an asteroid (will add it to exclusion list)
01:51:47.29 +58:37:55.3 -- not an asteroid (will add it to exclusion list)
01:12:00.92 +64:42:18.2 -- not an asteroid (will add it to exclusion list)
01:08:15.48 +61:15:06.7 -- not an asteroid (will add it to exclusion list)
01:26:37.92 +60:38:02.4 -- not an asteroid (will add it to exclusion list)
01:43:27.31 +58:38:07.0 -- not an asteroid (will add it to exclusion list)
01:29:48.25 +63:19:35.8 -- not an asteroid (will add it to exclusion list)
02:00:06.64 +59:00:32.8 -- not an asteroid (will add it to exclusion list)
01:07:45.52 +57:45:04.8 -- not an asteroid (will add it to exclusion list)
01:21:40.06 +61:36:42.7 -- not an asteroid (will add it to exclusion list)
01:30:34.37 +59:44:32.2 -- not an asteroid (will add it to exclusion list)
01:35:27.62 +60:33:47.4 -- not an asteroid (will add it to exclusion list)
01:37:17.59 +57:50:54.6 -- not an asteroid (will add it to exclusion list)
01:34:16.42 +60:57:34.9 -- not an asteroid (will add it to exclusion list)
01:17:15.14 +58:35:37.1 -- not an asteroid (will add it to exclusion list)
01:25:45.80 +59:01:22.7 -- not an asteroid (will add it to exclusion list)
01:49:15.82 +59:14:38.3 -- not an asteroid (will add it to exclusion list)
02:05:14.98 +63:02:37.2 -- not an asteroid (will add it to exclusion list)
01:26:39.09 +59:41:38.1 -- not an asteroid (will add it to exclusion list)
01:18:47.92 +59:08:14.7 -- not an asteroid (will add it to exclusion list)
01:07:31.84 +61:28:27.2 -- not an asteroid (will add it to exclusion list)
01:56:43.24 +58:07:17.9 -- not an asteroid (will add it to exclusion list)
01:31:23.12 +59:33:43.6 -- not an asteroid (will add it to exclusion list)
01:35:24.58 +60:39:29.9 -- not an asteroid (will add it to exclusion list)
01:20:45.05 +57:55:09.5 -- not an asteroid (will add it to exclusion list)
01:08:23.32 +61:35:09.9 -- not an asteroid (will add it to exclusion list)
01:19:08.73 +60:33:58.6 -- not an asteroid (will add it to exclusion list)
01:27:35.79 +57:57:00.7 -- not an asteroid (will add it to exclusion list)
02:00:26.68 +63:04:13.4 -- not an asteroid (will add it to exclusion list)
01:07:57.25 +63:37:29.5 -- not an asteroid (will add it to exclusion list)
01:35:25.03 +60:39:14.8 -- not an asteroid (will add it to exclusion list)
01:49:03.90 +61:04:19.4 -- not an asteroid (will add it to exclusion list)
01:23:31.47 +58:41:48.0 -- not an asteroid (will add it to exclusion list)
01:27:22.04 +58:51:39.5 -- not an asteroid (will add it to exclusion list)
01:10:34.59 +60:31:07.6 -- not an asteroid (will add it to exclusion list)
01:46:38.50 +60:07:33.1 -- not an asteroid (will add it to exclusion list)
01:18:28.11 +58:11:23.6 -- not an asteroid (will add it to exclusion list)
02:00:21.73 +64:56:38.5 -- not an asteroid (will add it to exclusion list)
01:51:09.35 +64:52:46.8 -- not an asteroid (will add it to exclusion list)
01:08:59.45 +60:47:21.1 -- not an asteroid (will add it to exclusion list)
01:14:41.44 +58:46:46.5 -- not an asteroid (will add it to exclusion list)
01:22:10.97 +59:09:03.5 -- not an asteroid (will add it to exclusion list)
02:16:07.78 +58:18:14.4 -- not an asteroid (will add it to exclusion list)
01:51:26.73 +57:51:36.7 -- not an asteroid (will add it to exclusion list)
02:21:38.04 +65:44:28.6 -- not an asteroid (will add it to exclusion list)
02:15:03.70 +58:28:54.2 -- not an asteroid (will add it to exclusion list)
01:09:22.61 +57:26:31.1 -- not an asteroid (will add it to exclusion list)
01:13:39.03 +58:10:51.2 -- not an asteroid (will add it to exclusion list)
01:22:23.90 +61:13:51.6 -- not an asteroid (will add it to exclusion list)
02:00:32.94 +59:40:07.3 -- not an asteroid (will add it to exclusion list)
01:38:05.83 +61:04:14.1 -- not an asteroid (will add it to exclusion list)
01:24:49.19 +59:47:15.9 -- not an asteroid (will add it to exclusion list)
02:16:27.39 +64:52:49.7 -- not an asteroid (will add it to exclusion list)
01:50:39.84 +62:00:56.4 -- not an asteroid (will add it to exclusion list)
01:41:34.52 +59:13:59.0 -- not an asteroid (will add it to exclusion list)
01:25:25.28 +58:19:59.4 -- not an asteroid (will add it to exclusion list)
01:06:55.34 +59:18:58.6 -- not an asteroid (will add it to exclusion list)
01:52:55.35 +59:33:31.4 -- not an asteroid (will add it to exclusion list)
02:02:25.08 +64:38:23.8 -- not an asteroid (will add it to exclusion list)
01:56:57.38 +63:00:32.5 -- not an asteroid (will add it to exclusion list)
01:59:34.04 +63:37:09.5 -- not an asteroid (will add it to exclusion list)
01:42:17.62 +63:24:23.7 -- not an asteroid (will add it to exclusion list)
01:38:34.72 +57:58:01.1 -- not an asteroid (will add it to exclusion list)
01:56:48.73 +61:52:37.5 -- not an asteroid (will add it to exclusion list)
01:52:55.29 +60:27:25.5 -- not an asteroid (will add it to exclusion list)
01:17:45.49 +57:34:01.3 -- not an asteroid (will add it to exclusion list)
02:08:50.63 +59:21:19.7 -- not an asteroid (will add it to exclusion list)
01:51:53.64 +63:26:20.9 -- not an asteroid (will add it to exclusion list)
01:23:46.56 +60:53:19.3 -- not an asteroid (will add it to exclusion list)
02:07:53.85 +58:37:40.7 -- not an asteroid (will add it to exclusion list)
01:33:30.69 +58:02:23.6 -- not an asteroid (will add it to exclusion list)
01:40:29.69 +60:46:50.2 -- not an asteroid (will add it to exclusion list)
01:40:21.93 +60:45:15.1 -- not an asteroid (will add it to exclusion list)
01:26:28.50 +59:41:36.9 -- not an asteroid (will add it to exclusion list)
01:29:20.11 +59:29:36.8 -- not an asteroid (will add it to exclusion list)
01:24:11.89 +59:17:51.8 -- not an asteroid (will add it to exclusion list)
01:19:29.32 +59:25:22.1 -- not an asteroid (will add it to exclusion list)
02:04:06.48 +60:14:18.0 -- not an asteroid (will add it to exclusion list)
01:25:25.32 +58:37:26.1 -- not an asteroid (will add it to exclusion list)
01:51:52.56 +60:27:42.9 -- not an asteroid (will add it to exclusion list)
02:09:40.63 +60:06:56.2 -- not an asteroid (will add it to exclusion list)
01:31:56.01 +59:26:39.7 -- not an asteroid (will add it to exclusion list)
01:44:29.89 +65:09:23.0 -- not an asteroid (will add it to exclusion list)
01:52:07.30 +59:13:07.9 -- not an asteroid (will add it to exclusion list)
01:29:33.79 +60:47:14.9 -- not an asteroid (will add it to exclusion list)
01:57:26.38 +63:23:42.4 -- not an asteroid (will add it to exclusion list)
01:19:11.94 +59:07:32.3 -- not an asteroid (will add it to exclusion list)
02:08:22.88 +64:18:53.9 -- not an asteroid (will add it to exclusion list)
01:41:39.56 +58:27:14.6 -- not an asteroid (will add it to exclusion list)
02:12:28.07 +59:37:07.8 -- not an asteroid (will add it to exclusion list)
01:46:38.09 +60:08:58.0 -- not an asteroid (will add it to exclusion list)
02:19:30.65 +64:32:24.3 -- not an asteroid (will add it to exclusion list)
02:13:06.76 +59:49:48.1 -- not an asteroid (will add it to exclusion list)
01:38:35.76 +64:48:51.6 -- not an asteroid (will add it to exclusion list)
01:48:17.78 +60:40:24.8 -- not an asteroid (will add it to exclusion list)
01:17:06.09 +60:05:14.0 -- not an asteroid (will add it to exclusion list)
01:54:07.61 +61:05:02.2 -- not an asteroid (will add it to exclusion list)
01:38:40.34 +64:31:56.1 -- not an asteroid (will add it to exclusion list)
01:26:22.39 +61:16:26.2 -- not an asteroid (will add it to exclusion list)
01:34:06.30 +59:58:54.9 -- not an asteroid (will add it to exclusion list)
01:50:44.27 +59:04:33.9 -- not an asteroid (will add it to exclusion list)
01:56:50.95 +59:00:21.1 -- not an asteroid (will add it to exclusion list)
01:40:27.31 +58:35:19.4 -- not an asteroid (will add it to exclusion list)
01:58:56.43 +65:19:00.3 -- not an asteroid (will add it to exclusion list)
01:58:46.64 +60:45:03.9 -- not an asteroid (will add it to exclusion list)
01:27:06.87 +61:26:15.3 -- not an asteroid (will add it to exclusion list)
01:20:49.30 +59:05:42.6 -- not an asteroid (will add it to exclusion list)
01:16:20.04 +60:08:56.4 -- not an asteroid (will add it to exclusion list)
01:41:40.36 +62:34:09.1 -- not an asteroid (will add it to exclusion list)
01:28:14.72 +60:19:21.0 -- not an asteroid (will add it to exclusion list)
01:48:47.41 +58:57:20.8 -- not an asteroid (will add it to exclusion list)
02:00:31.55 +62:35:42.1 -- not an asteroid (will add it to exclusion list)
01:45:00.28 +59:26:56.2 -- not an asteroid (will add it to exclusion list)
01:23:52.18 +60:52:55.6 -- not an asteroid (will add it to exclusion list)
01:45:41.64 +60:27:33.5 -- not an asteroid (will add it to exclusion list)
01:29:04.21 +61:34:53.8 -- not an asteroid (will add it to exclusion list)
01:34:30.28 +61:09:14.8 -- not an asteroid (will add it to exclusion list)
01:37:32.86 +60:29:03.7 -- not an asteroid (will add it to exclusion list)
01:29:43.49 +58:27:52.9 -- not an asteroid (will add it to exclusion list)
01:22:41.20 +59:08:56.9 -- not an asteroid (will add it to exclusion list)
01:25:27.61 +59:53:35.3 -- not an asteroid (will add it to exclusion list)
01:26:31.68 +62:18:33.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:04:35.20 +62:44:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:04.67 +63:39:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:53.88 +59:06:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:13.18 +59:33:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:15.89 +57:53:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:24.44 +60:07:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:55.34 +59:18:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:01.87 +59:46:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:06.59 +57:40:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:31.84 +61:28:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:33.61 +61:22:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:36.88 +58:09:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.17 +59:59:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:45.52 +57:45:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:57.25 +63:37:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:15.48 +61:15:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:23.32 +61:35:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:25.67 +59:48:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:39.25 +60:32:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:47.54 +57:50:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:59.45 +60:47:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:22.61 +57:26:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:34.59 +60:31:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:00.92 +64:42:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:01.47 +58:29:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:41.26 +61:18:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:59.70 +57:34:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:39.03 +58:10:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:41.44 +58:46:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:30.43 +60:45:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:20.04 +60:08:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:23.35 +58:49:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:40.37 +61:23:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:06.09 +60:05:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:15.14 +58:35:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:45.49 +57:34:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:28.11 +58:11:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:47.92 +59:08:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:08.73 +60:33:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:11.94 +59:07:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:12.21 +60:58:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:29.32 +59:25:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:42.12 +59:35:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:45.05 +57:55:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:49.30 +59:05:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:11.22 +59:33:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:40.06 +61:36:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:45.32 +58:34:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:10.97 +59:09:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:13.69 +62:32:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:23.90 +61:13:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:33.26 +60:44:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:41.20 +59:08:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:50.56 +58:12:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:31.47 +58:41:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:46.56 +60:53:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:52.18 +60:52:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:53.55 +58:03:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:56.99 +62:15:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:06.20 +60:41:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:11.89 +59:17:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:49.19 +59:47:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:55.09 +59:41:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:00.87 +62:50:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:02.98 +65:27:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:25.28 +58:19:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:25.32 +58:37:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:27.54 +59:27:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:27.61 +59:53:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:42.78 +58:50:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:45.80 +59:01:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:57.02 +58:48:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:05.62 +59:01:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:22.39 +61:16:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:28.50 +59:41:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:31.68 +62:18:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:37.92 +60:38:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:38.72 +62:48:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:39.09 +59:41:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:06.87 +61:26:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:22.04 +58:51:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:32.56 +64:34:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:35.79 +57:57:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:14.72 +60:19:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:04.21 +61:34:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:20.11 +59:29:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:33.79 +60:47:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:43.49 +58:27:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:48.25 +63:19:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:00.95 +60:10:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:06.40 +63:44:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:34.37 +59:44:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:59.89 +63:14:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:23.12 +59:33:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:56.01 +59:26:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:10.98 +59:36:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:22.31 +62:14:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:25.36 +61:29:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:20.05 +62:33:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:22.88 +61:41:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:30.69 +58:02:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:40.63 +59:42:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:06.30 +59:58:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:10.01 +60:13:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:16.42 +60:57:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:30.25 +59:54:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:30.28 +61:09:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:46.03 +62:04:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:57.93 +61:00:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:59.27 +60:09:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:24.58 +60:39:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:25.03 +60:39:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:27.62 +60:33:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:09.46 +61:08:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:17.59 +57:50:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:23.81 +59:20:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:32.86 +60:29:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:05.83 +61:04:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:34.72 +57:58:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:35.76 +64:48:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:40.34 +64:31:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:59.12 +61:08:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:10.54 +58:03:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:18.20 +61:21:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:21.93 +60:45:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:27.31 +58:35:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:29.69 +60:46:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:34.52 +59:13:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:39.56 +58:27:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:40.36 +62:34:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:17.62 +63:24:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:20.74 +61:14:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:24.12 +61:12:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:27.31 +58:38:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:29.89 +65:09:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:00.28 +59:26:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:15.39 +61:13:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:19.33 +61:13:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:41.64 +60:27:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:36.58 +64:06:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.09 +60:08:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.50 +60:07:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:13.35 +59:51:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:17.78 +60:40:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:47.41 +58:57:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:03.90 +61:04:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:15.82 +59:14:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:40.08 +59:34:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:16.38 +58:52:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:39.84 +62:00:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:44.27 +59:04:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:09.35 +64:52:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:26.73 +57:51:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:47.29 +58:37:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:52.56 +60:27:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:53.64 +63:26:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:03.58 +60:31:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:07.30 +59:13:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:55.29 +60:27:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:55.35 +59:33:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:04.68 +62:00:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:07.61 +61:05:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:28.44 +63:18:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:46.61 +57:57:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:27.23 +65:22:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:38.04 +59:15:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:43.24 +58:07:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:48.73 +61:52:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:50.95 +59:00:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:57.38 +63:00:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:26.38 +63:23:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:29.26 +60:09:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:46.64 +60:45:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:56.43 +65:19:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:34.04 +63:37:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:06.64 +59:00:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:21.73 +64:56:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:26.68 +63:04:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:31.55 +62:35:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:32.94 +59:40:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:25.08 +64:38:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:59.13 +59:34:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:06.48 +60:14:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:14.98 +63:02:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:53.85 +58:37:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:22.88 +64:18:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:50.63 +59:21:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:40.63 +60:06:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:28.07 +59:37:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:06.76 +59:49:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:37.67 +61:10:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:26.26 +61:46:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:03.70 +58:28:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:07.78 +58:18:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:27.39 +64:52:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:30.65 +64:32:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:38.04 +65:44:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:04:35.20 +62:44:33.3 -- not a known variable star
01:05:04.67 +63:39:45.2 -- a known variable star
01:05:53.88 +59:06:23.6 -- not a known variable star
01:06:13.18 +59:33:47.5 -- not a known variable star
01:06:15.89 +57:53:25.3 -- not a known variable star
01:06:24.44 +60:07:16.0 -- not a known variable star
01:06:55.34 +59:18:58.6 -- not a known variable star
01:07:01.87 +59:46:17.1 -- not a known variable star
01:07:06.59 +57:40:47.8 -- not a known variable star
01:07:31.84 +61:28:27.2 -- not a known variable star
01:07:33.61 +61:22:51.8 -- a known variable star
01:07:36.88 +58:09:25.4 -- not a known variable star
01:07:39.17 +59:59:18.0 -- not a known variable star
01:07:45.52 +57:45:04.8 -- not a known variable star
01:07:57.25 +63:37:29.5 -- a known variable star
01:08:15.48 +61:15:06.7 -- not a known variable star
01:08:23.32 +61:35:09.9 -- not a known variable star
01:08:25.67 +59:48:03.7 -- not a known variable star
01:08:39.25 +60:32:41.3 -- not a known variable star
01:08:47.54 +57:50:27.2 -- a known variable star
01:08:59.45 +60:47:21.1 -- not a known variable star
01:09:22.61 +57:26:31.1 -- not a known variable star
01:10:34.59 +60:31:07.6 -- a known variable star
01:12:00.92 +64:42:18.2 -- a known variable star
01:12:01.47 +58:29:48.8 -- not a known variable star
01:12:41.26 +61:18:08.1 -- not a known variable star
01:12:59.70 +57:34:09.5 -- not a known variable star
01:13:39.03 +58:10:51.2 -- not a known variable star
01:14:41.44 +58:46:46.5 -- a known variable star
01:15:30.43 +60:45:22.6 -- not a known variable star
01:16:20.04 +60:08:56.4 -- a known variable star
01:16:23.35 +58:49:28.1 -- not a known variable star
01:16:40.37 +61:23:05.9 -- a known variable star
01:17:06.09 +60:05:14.0 -- not a known variable star
01:17:15.14 +58:35:37.1 -- not a known variable star
01:17:45.49 +57:34:01.3 -- not a known variable star
01:18:28.11 +58:11:23.6 -- not a known variable star
01:18:47.92 +59:08:14.7 -- not a known variable star
01:19:08.73 +60:33:58.6 -- not a known variable star
01:19:11.94 +59:07:32.3 -- not a known variable star
01:19:12.21 +60:58:37.9 -- not a known variable star
01:19:29.32 +59:25:22.1 -- not a known variable star
01:20:42.12 +59:35:05.3 -- not a known variable star
01:20:45.05 +57:55:09.5 -- not a known variable star
01:20:49.30 +59:05:42.6 -- not a known variable star
01:21:11.22 +59:33:02.0 -- a known variable star
01:21:40.06 +61:36:42.7 -- not a known variable star
01:21:45.32 +58:34:15.3 -- a known variable star
01:22:10.97 +59:09:03.5 -- not a known variable star
01:22:13.69 +62:32:56.6 -- not a known variable star
01:22:23.90 +61:13:51.6 -- a known variable star
01:22:33.26 +60:44:41.1 -- not a known variable star
01:22:41.20 +59:08:56.9 -- a known variable star
01:22:50.56 +58:12:42.7 -- a known variable star
01:23:31.47 +58:41:48.0 -- a known variable star
01:23:46.56 +60:53:19.3 -- not a known variable star
01:23:52.18 +60:52:55.6 -- not a known variable star
01:23:53.55 +58:03:34.7 -- not a known variable star
01:23:56.99 +62:15:27.9 -- not a known variable star
01:24:06.20 +60:41:09.9 -- not a known variable star
01:24:11.89 +59:17:51.8 -- not a known variable star
01:24:49.19 +59:47:15.9 -- not a known variable star
01:24:55.09 +59:41:48.4 -- not a known variable star
01:25:00.87 +62:50:52.5 -- not a known variable star
01:25:02.98 +65:27:16.3 -- not a known variable star
01:25:25.28 +58:19:59.4 -- not a known variable star
01:25:25.32 +58:37:26.1 -- a known variable star
01:25:27.54 +59:27:15.5 -- a known variable star
01:25:27.61 +59:53:35.3 -- a known variable star
01:25:42.78 +58:50:45.7 -- not a known variable star
01:25:45.80 +59:01:22.7 -- not a known variable star
01:25:57.02 +58:48:08.8 -- not a known variable star
01:26:05.62 +59:01:15.0 -- not a known variable star
01:26:22.39 +61:16:26.2 -- a known variable star
01:26:28.50 +59:41:36.9 -- not a known variable star
01:26:31.68 +62:18:33.2 -- not a known variable star
01:26:37.92 +60:38:02.4 -- not a known variable star
01:26:38.72 +62:48:30.9 -- not a known variable star
01:26:39.09 +59:41:38.1 -- a known variable star
01:27:06.87 +61:26:15.3 -- not a known variable star
01:27:22.04 +58:51:39.5 -- not a known variable star
01:27:32.56 +64:34:36.1 -- not a known variable star
01:27:35.79 +57:57:00.7 -- not a known variable star
01:28:14.72 +60:19:21.0 -- a known variable star
01:29:04.21 +61:34:53.8 -- not a known variable star
01:29:20.11 +59:29:36.8 -- not a known variable star
01:29:33.79 +60:47:14.9 -- not a known variable star
01:29:43.49 +58:27:52.9 -- a known variable star
01:29:48.25 +63:19:35.8 -- not a known variable star
01:30:00.95 +60:10:50.0 -- a known variable star
01:30:06.40 +63:44:41.8 -- not a known variable star
01:30:34.37 +59:44:32.2 -- not a known variable star
01:30:59.89 +63:14:37.6 -- not a known variable star
01:31:23.12 +59:33:43.6 -- not a known variable star
01:31:56.01 +59:26:39.7 -- not a known variable star
01:32:10.98 +59:36:03.5 -- not a known variable star
01:32:22.31 +62:14:57.8 -- not a known variable star
01:32:25.36 +61:29:15.7 -- a known variable star
01:33:20.05 +62:33:20.9 -- not a known variable star
01:33:22.88 +61:41:09.1 -- not a known variable star
01:33:30.69 +58:02:23.6 -- not a known variable star
01:33:40.63 +59:42:23.5 -- a known variable star
01:34:06.30 +59:58:54.9 -- not a known variable star
01:34:10.01 +60:13:05.8 -- not a known variable star
01:34:16.42 +60:57:34.9 -- not a known variable star
01:34:30.25 +59:54:23.8 -- not a known variable star
01:34:30.28 +61:09:14.8 -- not a known variable star
01:34:46.03 +62:04:51.5 -- a known variable star
01:34:57.93 +61:00:13.6 -- a known variable star
01:34:59.27 +60:09:34.6 -- not a known variable star
01:35:24.58 +60:39:29.9 -- a known variable star
01:35:25.03 +60:39:14.8 -- a known variable star
01:35:27.62 +60:33:47.4 -- not a known variable star
01:36:09.46 +61:08:51.7 -- not a known variable star
01:37:17.59 +57:50:54.6 -- not a known variable star
01:37:23.81 +59:20:12.3 -- not a known variable star
01:37:32.86 +60:29:03.7 -- not a known variable star
01:38:05.83 +61:04:14.1 -- not a known variable star
01:38:34.72 +57:58:01.1 -- not a known variable star
01:38:35.76 +64:48:51.6 -- not a known variable star
01:38:40.34 +64:31:56.1 -- a known variable star
01:38:59.12 +61:08:53.2 -- a known variable star
01:39:10.54 +58:03:36.0 -- not a known variable star
01:40:18.20 +61:21:06.0 -- not a known variable star
01:40:21.93 +60:45:15.1 -- not a known variable star
01:40:27.31 +58:35:19.4 -- a known variable star
01:40:29.69 +60:46:50.2 -- a known variable star
01:41:34.52 +59:13:59.0 -- not a known variable star
01:41:39.56 +58:27:14.6 -- not a known variable star
01:41:40.36 +62:34:09.1 -- not a known variable star
01:42:17.62 +63:24:23.7 -- not a known variable star
01:43:20.74 +61:14:37.9 -- not a known variable star
01:43:24.12 +61:12:07.8 -- a known variable star
01:43:27.31 +58:38:07.0 -- a known variable star
01:44:29.89 +65:09:23.0 -- a known variable star
01:45:00.28 +59:26:56.2 -- not a known variable star
01:45:15.39 +61:13:52.8 -- not a known variable star
01:45:19.33 +61:13:08.4 -- not a known variable star
01:45:41.64 +60:27:33.5 -- a known variable star
01:46:36.58 +64:06:19.3 -- not a known variable star
01:46:38.09 +60:08:58.0 -- not a known variable star
01:46:38.50 +60:07:33.1 -- not a known variable star
01:48:13.35 +59:51:32.6 -- a known variable star
01:48:17.78 +60:40:24.8 -- a known variable star
01:48:47.41 +58:57:20.8 -- a known variable star
01:49:03.90 +61:04:19.4 -- not a known variable star
01:49:15.82 +59:14:38.3 -- not a known variable star
01:49:40.08 +59:34:16.8 -- not a known variable star
01:50:16.38 +58:52:59.7 -- not a known variable star
01:50:39.84 +62:00:56.4 -- not a known variable star
01:50:44.27 +59:04:33.9 -- not a known variable star
01:51:09.35 +64:52:46.8 -- a known variable star
01:51:26.73 +57:51:36.7 -- not a known variable star
01:51:47.29 +58:37:55.3 -- not a known variable star
01:51:52.56 +60:27:42.9 -- not a known variable star
01:51:53.64 +63:26:20.9 -- a known variable star
01:52:03.58 +60:31:38.5 -- not a known variable star
01:52:07.30 +59:13:07.9 -- a known variable star
01:52:55.29 +60:27:25.5 -- not a known variable star
01:52:55.35 +59:33:31.4 -- a known variable star
01:53:04.68 +62:00:26.5 -- not a known variable star
01:54:07.61 +61:05:02.2 -- not a known variable star
01:55:28.44 +63:18:55.9 -- not a known variable star
01:55:46.61 +57:57:42.5 -- a known variable star
01:56:27.23 +65:22:09.4 -- not a known variable star
01:56:38.04 +59:15:34.2 -- a known variable star
01:56:43.24 +58:07:17.9 -- not a known variable star
01:56:48.73 +61:52:37.5 -- not a known variable star
01:56:50.95 +59:00:21.1 -- not a known variable star
01:56:57.38 +63:00:32.5 -- not a known variable star
01:57:26.38 +63:23:42.4 -- not a known variable star
01:57:29.26 +60:09:19.2 -- not a known variable star
01:58:46.64 +60:45:03.9 -- a known variable star
01:58:56.43 +65:19:00.3 -- not a known variable star
01:59:34.04 +63:37:09.5 -- not a known variable star
02:00:06.64 +59:00:32.8 -- not a known variable star
02:00:21.73 +64:56:38.5 -- not a known variable star
02:00:26.68 +63:04:13.4 -- a known variable star
02:00:31.55 +62:35:42.1 -- not a known variable star
02:00:32.94 +59:40:07.3 -- a known variable star
02:02:25.08 +64:38:23.8 -- a known variable star
02:03:59.13 +59:34:48.0 -- not a known variable star
02:04:06.48 +60:14:18.0 -- not a known variable star
02:05:14.98 +63:02:37.2 -- a known variable star
02:07:53.85 +58:37:40.7 -- not a known variable star
02:08:22.88 +64:18:53.9 -- not a known variable star
02:08:50.63 +59:21:19.7 -- not a known variable star
02:09:40.63 +60:06:56.2 -- not a known variable star
02:12:28.07 +59:37:07.8 -- a known variable star
02:13:06.76 +59:49:48.1 -- not a known variable star
02:13:37.67 +61:10:28.1 -- not a known variable star
02:14:26.26 +61:46:49.0 -- a known variable star
02:15:03.70 +58:28:54.2 -- a known variable star
02:16:07.78 +58:18:14.4 -- a known variable star
02:16:27.39 +64:52:49.7 -- not a known variable star
02:19:30.65 +64:32:24.3 -- not a known variable star
02:21:38.04 +65:44:28.6 -- not a known variable star
Found 142 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
197 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 197 (excluding asteroids and hot pixels, 142 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)2461211.91975792 -observatory V36
07:37:51.20 +21:39:48.0 Mercury (0.9mag)
08:42:40.45 +20:15:56.5 Venus (-4.0mag)
03:25:19.66 +18:15:42.7 Mars (1.3mag)
07:58:52.65 +21:03:59.2 Jupiter (-1.8mag)
00:52:29.61 +03:05:09.8 Saturn (0.8mag)
04:03:02.92 +20:33:32.0 Uranus (5.8mag)
00:16:43.08 +00:19:50.9 Neptune (7.8mag)
20:32:34.28 -23:09:23.7 Pluto (14.5mag)
10:45:48.45 +06:14:37.6 Moon (-9.9mag)
-rw-r--r-- 1 apache apache 361 Jun 20 07:22 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461211.91975792:
07:58:50.15 +21:04:09.3 Io (6.2mag)
07:58:58.64 +21:03:38.7 Europa (6.3mag)
07:59:00.44 +21:03:29.9 Ganymede (5.6mag)
07:59:15.62 +21:02:50.2 Callisto (6.9mag)
07:58:26.79 +20:41:57.2 Himalia (15.6mag)
07:58:56.59 +21:03:46.0 Thebe (16.6mag)
07:58:06.43 +20:52:22.8 Elara (17.6mag)
08:01:38.90 +21:08:59.9 Pasiphae (17.8mag)
08:04:53.74 +21:06:43.8 Carme (18.9mag)
00:52:23.91 +03:05:38.6 Titan (8.6mag)
00:52:34.18 +03:05:13.6 Rhea (9.9mag)
00:52:43.44 +03:07:32.5 Iapetus (11.3mag)
00:52:32.95 +03:05:38.1 Hyperion (14.6mag)
00:52:56.52 +03:05:19.4 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jun 20 07:22 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461211.91975792:
17:28:22.11 -35:30:03.0 JWST
18:33:58.23 +21:22:48.9 Chandra
04:10:02.89 +55:47:42.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 20 07:22 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461211.91975792 -observatory V36
18:34:15.09 -33:28:19.0 13.6mag P/2010 H2 (Vales)
06:05:38.09 -67:59:41.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:53:35.25 +32:08:08.3 17.6mag C/2017 K2 (PANSTARRS)
17:09:54.02 +15:49:48.1 17.9mag C/2021 G2 (ATLAS)
23:13:41.25 -35:57:21.4 15.9mag P/2021 N1 (ZTF)
23:09:04.79 +31:59:51.7 17.2mag C/2022 E2 (ATLAS)
05:48:55.65 +27:00:44.3 16.6mag C/2022 N2 (PANSTARRS)
09:38:57.02 +30:37:32.3 16.7mag C/2022 QE78 (ATLAS)
08:57:25.23 +04:26:47.7 17.7mag C/2022 R6 (PANSTARRS)
18:20:07.35 +21:42:10.1 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:15:27.22 -11:04:21.6 17.6mag P/2023 B1 (PANSTARRS)
22:08:14.64 +67:11:00.6 17.8mag C/2023 H5 (Lemmon)
17:15:59.29 -07:56:43.5 13.7mag C/2023 R1 (PANSTARRS)
13:17:38.84 +80:07:17.1 18.0mag C/2023 X2 (Lemmon)
07:28:13.87 +64:45:57.0 17.8mag C/2024 A1 (ATLAS)
07:05:21.96 +28:48:34.1 14.0mag C/2024 E1 (Wierzchos)
15:28:12.47 +14:26:42.6 17.4mag C/2024 G6 (ATLAS)
20:03:22.21 +34:38:21.8 13.9mag C/2024 J3 (ATLAS)
04:30:14.73 -14:58:24.6 15.9mag C/2024 T5 (ATLAS)
06:17:10.96 +32:23:58.2 17.9mag C/2025 J1 (Borisov)
11:32:04.41 +52:00:03.3 17.8mag C/2025 L1 (ATLAS)
06:58:03.26 -11:28:35.5 15.2mag C/2025 R3 (PANSTARRS)
09:35:01.03 +23:06:28.2 17.8mag C/2025 V2 (Rankin)
12:40:13.34 +04:33:13.0 17.1mag C/2025 Y1 (ATLAS)
17:48:11.27 +77:23:32.4 17.7mag C/2026 A2 (Bok)
02:20:30.37 +44:12:53.0 16.3mag C/2026 B2 (Sun-Gao)
11:15:03.54 +00:05:06.6 16.7mag A/2026 E1
20:45:30.48 -09:58:11.7 8.1mag 10P/Tempel
11:05:28.06 -01:12:36.2 16.0mag 29P/Schwassmann-Wachmann
03:30:30.76 +27:13:32.6 17.7mag 47P/Ashbrook-Jackson
09:26:02.06 +20:11:12.6 16.9mag 63P/Wild
00:36:37.42 -05:41:18.5 15.6mag 65P/Gunn
07:23:11.06 +34:17:50.1 17.2mag 76P/West-Kohoutek-Ikemura
03:38:52.32 +18:37:23.0 13.8mag 78P/Gehrels
01:46:11.73 +07:20:08.5 15.8mag 88P/Howell
05:33:50.47 +30:54:00.7 15.4mag 93P/Lovas
03:18:36.70 +29:22:59.8 17.3mag 114P/Wiseman-Skiff
07:20:00.29 +32:25:48.3 15.5mag 123P/West-Hartley
10:11:45.23 +09:26:42.7 16.6mag 124P/Mrkos
04:19:12.48 +19:59:10.3 16.3mag 128P/Shoemaker-Holt
04:57:45.53 +19:31:27.2 17.8mag 131P/Mueller
06:47:39.70 +16:55:50.9 16.2mag 141P/Machholz
06:51:15.26 +17:52:18.7 16.1mag 141P-A/Machholz
05:53:16.02 +17:17:31.5 13.0mag 141P-D/Machholz
03:05:55.99 -23:07:40.5 16.4mag 161P/Hartley-IRAS
04:22:40.16 +28:21:01.4 15.0mag 162P/SidingSpring
19:32:29.45 +05:44:48.5 16.2mag 169P/NEAT
00:50:50.00 +04:43:10.9 17.8mag 220P/McNaught
16:43:40.68 -08:05:59.9 16.6mag 235P/LINEAR
08:02:04.00 +34:51:02.5 17.7mag 240P/NEAT
01:04:45.70 +02:53:04.4 16.1mag 260P/McNaught
04:38:20.20 +34:30:41.0 17.5mag 295P/LINEAR
00:55:40.34 +03:21:49.8 17.9mag 320P/McNaught
15:10:28.79 +07:31:59.9 17.5mag 391P/Kowalski
08:17:11.14 +20:23:45.6 17.9mag 450P/LONEOS
07:19:52.50 +40:47:56.5 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 20 07:22 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 07:22 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 07:22 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
00:50:45.142 -71:38:36.96 AT 2026oyp 2026-06-11.37 10.5
14:38:02.268 +18:37:59.98 AT 2026oyo 2026-06-02.91 19.7
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
-rw-r--r-- 1 apache apache 30K Jun 20 07:22 tns_transients_list.txt
