This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ
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 23.4308 2461214.9308 8.76 01:56:38.00 +59:15:34.1
131.18796 -2.56321 galactic Cas Second-epoch detections are separated by 0.2" and 7.5 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 01:56:38.00 +59:15:34.1: 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 01:56:38.00 +59:15:34.1: 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 23.4308* 01 56 38.00 +59 15 34.1 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,2461214.9308,8.76,0.05,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
X Cas 20260623.4308 8.76CV 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 23.4308 2461214.9308 11.80 01:34:23.32 +59:34:48.9
128.35169 -2.83877 galactic Cas Second-epoch detections are separated by 1.2" and 7.3 pix
The object was found in VSX19" Gaia DR3 509372061778119680
Type: ROT
# Max. Min./Amp. JD0 Period
14.510 G 14.540 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 01:34:23.32 +59:34:48.9: 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 01:34:23.32 +59:34:48.9: 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 23.4308* 01 34 23.32 +59 34 48.9 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
Gaia DR3 509372061778119680,2461214.9308,11.80,0.05,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 509372061778119680 20260623.4308 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 23.4308 2461214.9308 11.65 01:35:23.02 +60:03:01.8
128.39608 -2.35420 galactic Cas Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:35:23.02 +60:03:01.8 (user input) | T | P | (position from user input) J-Ks=0.844+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:23.02 +60:03:01.8: 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 01:35:23.02 +60:03:01.8: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 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 23.4308* 01 35 23.02 +60 03 01.8 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
target,2461214.9308,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.52 01:32:08.93 +61:32:09.5
127.76362 -0.95327 galactic Cas Second-epoch detections are separated by 2.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:32:08.93 +61:32:09.5 (user input) | T | P | (position from user input) J-Ks=0.472+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:08.93 +61:32:09.5: 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 01:32:08.93 +61:32:09.5: 14.37 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.37 +/- 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 23.4308* 01 32 08.93 +61 32 09.5 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,2461214.9308,11.52,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.48 02:01:50.41 +63:28:16.8
130.69710 1.66599 galactic Cas Second-epoch detections are separated by 0.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 514909580290801024 | 02:01:55.03 +63:28:35.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.540+/-0.029 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:50.41 +63:28:16.8: 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 02:01:50.41 +63:28:16.8: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 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 23.4308* 02 01 50.41 +63 28 16.8 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 514909580290801024,2461214.9308,11.48,0.05,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
Gaia DR3 514909580290801024 20260623.4308 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 23.4308 2461214.9308 11.46 01:11:16.45 +58:55:57.0
125.49444 -3.84052 galactic Cas Second-epoch detections are separated by 0.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.8423+58.9300 | 01:11:16.45 +58:55:57.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.465+/-0.043 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:16.45 +58:55:57.0: 12.09 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:16.45 +58:55:57.0: 14.20 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.73 +/- 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 23.4308* 01 11 16.45 +58 55 57.0 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 J017.8423+58.9300,2461214.9308,11.46,0.05,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
ATO J017.8423+58.9300 20260623.4308 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 23.4308 2461214.9308 11.42 01:24:44.81 +63:34:15.9
126.62829 0.93864 galactic Cas Second-epoch detections are separated by 1.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:24:44.81 +63:34:15.9 (user input) | T | P | (position from user input) J-Ks=0.478+/-0.029 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:44.81 +63:34:15.9: 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 01:24:44.81 +63:34:15.9: 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 23.4308* 01 24 44.81 +63 34 15.9 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
target,2461214.9308,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.30 01:34:22.91 +60:02:40.3
128.27371 -2.38107 galactic Cas Second-epoch detections are separated by 1.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 509770905316152320 | 01:34:26.80 +60:02:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3 1955ApJS....2..123F LF 5 +59 68
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:22.91 +60:02:40.3: 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 01:34:22.91 +60:02:40.3: 14.24 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.24 +/- 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 23.4308* 01 34 22.91 +60 02 40.3 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509770905316152320,2461214.9308,11.30,0.05,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
Gaia DR3 509770905316152320 20260623.4308 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 23.4308 2461214.9308 11.24 01:53:37.97 +64:44:09.9
129.50829 2.66143 galactic Cas Second-epoch detections are separated by 2.5" and 7.3 pix
The object was found in VSX 2" Gaia DR3 518235499886390016
Type: ROT
# Max. Min./Amp. JD0 Period
14.070 G 14.100 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 01:53:37.97 +64:44:09.9: 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 01:53:37.97 +64:44:09.9: 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 23.4308* 01 53 37.97 +64 44 09.9 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 518235499886390016,2461214.9308,11.24,0.05,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
Gaia DR3 518235499886390016 20260623.4308 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 23.4308 2461214.9308 11.29 01:12:01.02 +64:42:20.4
125.12894 1.92174 galactic Cas Second-epoch detections are separated by 3.6" and 6.5 pix
The object was found in VSX 1" ZTF J011201.03+644221.2
Type: RS
# Max. Min./Amp. JD0 Period
14.762 g Y 0.263 g 2458343.85900 3.018403700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:01.02 +64:42:20.4: 11.63 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:01.02 +64:42:20.4: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 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 23.4308* 01 12 01.02 +64 42 20.4 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 J011201.03+644221.2,2461214.9308,11.29,0.05,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
ZTF J011201.03+644221.2 20260623.4308 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 23.4308 2461214.9308 11.47 02:01:37.72 +64:49:01.8
130.31261 2.95603 galactic Cas Second-epoch detections are separated by 8.7" and 6.0 pix
The object was found in VSX11" ASASSN-V J020135.96+644901.1
Type: SR
# Max. Min./Amp. JD0 Period
14.300 V 14.510 V 2457299.00000 465.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:37.72 +64:49:01.8: 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 02:01:37.72 +64:49:01.8: 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 23.4308* 02 01 37.72 +64 49 01.8 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
ASASSN-V J020135.96+644901.1,2461214.9308,11.47,0.05,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
ASASSN-V J020135.96+644901.1 20260623.4308 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 23.4308 2461214.9308 11.30 01:30:01.21 +60:10:48.6
127.71530 -2.33276 galactic Cas Second-epoch detections are separated by 1.8" and 7.4 pix
The object was found in VSX21" 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 01:30:01.21 +60:10:48.6: 12.58 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:01.21 +60:10:48.6: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 30 01.21 +60 10 48.6 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509459713474637440,2461214.9308,11.30,0.05,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
Gaia DR3 509459713474637440 20260623.4308 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 23.4308 2461214.9308 11.35 01:57:29.29 +60:09:18.3
131.06692 -1.66929 galactic Cas Second-epoch detections are separated by 1.7" and 7.7 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 | 01:57:29.29 +60:09:18.3 (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 01:57:29.29 +60:09:18.3: 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 01:57:29.29 +60:09:18.3: 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 23.4308* 01 57 29.29 +60 09 18.3 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.39 01:32:10.95 +59:36:01.6
128.07258 -2.86401 galactic Cas Second-epoch detections are separated by 1.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J023.0277+59.5942 | 01:32:10.95 +59:36:01.6 (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 01:32:10.95 +59:36:01.6: 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 01:32:10.95 +59:36:01.6: 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 23.4308* 01 32 10.95 +59 36 01.6 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+59.5942,2461214.9308,11.39,0.05,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
ATO J023.0277+59.5942 20260623.4308 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 23.4308 2461214.9308 11.29 01:46:30.67 +66:08:35.0
128.46832 3.86507 galactic Cas Second-epoch detections are separated by 1.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:46:30.67 +66:08:35.0 (user input) | T | P | (position from user input) J-Ks=1.136+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:30.67 +66:08:35.0: 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 01:46:30.67 +66:08:35.0: 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 23.4308* 01 46 30.67 +66 08 35.0 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,2461214.9308,11.29,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.30 01:15:32.65 +60:23:09.0
125.90833 -2.34653 galactic Cas Second-epoch detections are separated by 1.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:15:32.65 +60:23:09.0 (user input) | T | P | (position from user input) J-Ks=0.906+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:32.65 +60:23:09.0: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:32.65 +60:23:09.0: 14.08 +/- 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 23.4308* 01 15 32.65 +60 23 09.0 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,2461214.9308,11.30,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.24 01:06:22.07 +62:13:32.0
124.67035 -0.59579 galactic Cas Second-epoch detections are separated by 2.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:22.07 +62:13:32.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:22.07 +62:13:32.0: 11.89 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:22.07 +62:13:32.0: 14.09 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.41 +/- 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 23.4308* 01 06 22.07 +62 13 32.0 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,2461214.9308,11.24,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.23 02:03:59.16 +59:35:03.5
132.00496 -2.00337 galactic Cas Second-epoch detections are separated by 1.8" and 7.7 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 | 02:03:59.16 +59:35:03.5 (user input) | T | P | (position from user input) J-Ks=0.306+/-0.047 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:59.16 +59:35:03.5: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:59.16 +59:35:03.5: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 02 03 59.16 +59 35 03.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,11.23,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.34 01:22:33.27 +60:44:41.8
126.72676 -1.89733 galactic Cas Second-epoch detections are separated by 1.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:22:33.27 +60:44:41.8 (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 01:22:33.27 +60:44:41.8: 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 01:22:33.27 +60:44:41.8: 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 23.4308* 01 22 33.27 +60 44 41.8 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,11.34,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.25 02:00:21.96 +58:20:17.6
131.89288 -3.32922 galactic Cas Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 505499508799542016 | 02:00:22.79 +58:20:36.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.492+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:21.96 +58:20:17.6: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:21.96 +58:20:17.6: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 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 23.4308* 02 00 21.96 +58 20 17.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505499508799542016,2461214.9308,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505499508799542016 20260623.4308 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.19 01:41:37.92 +60:05:55.2
129.15422 -2.16529 galactic Cas Second-epoch detections are separated by 2.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:41:37.92 +60:05:55.2 (user input) | T | P | (position from user input) J-Ks=0.809+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:37.92 +60:05:55.2: 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 01:41:37.92 +60:05:55.2: 13.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 41 37.92 +60 05 55.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,11.19,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.17 01:06:17.15 +57:53:07.7
124.91159 -4.92919 galactic Cas Second-epoch detections are separated by 1.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J016.5720+57.8855 | 01:06:17.15 +57:53:07.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.082+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:17.15 +57:53:07.7: 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 01:06:17.15 +57:53:07.7: 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 23.4308* 01 06 17.15 +57 53 07.7 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
ATO J016.5720+57.8855,2461214.9308,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J016.5720+57.8855 20260623.4308 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.10 01:51:45.38 +58:37:51.6
130.72838 -3.32471 galactic Cas Second-epoch detections are separated by 6.7" and 7.8 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 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 01:51:45.38 +58:37:51.6: 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 01:51:45.38 +58:37:51.6: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 51 45.38 +58 37 51.6 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 506225156418009984,2461214.9308,11.10,0.05,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
Gaia DR3 506225156418009984 20260623.4308 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 23.4308 2461214.9308 11.28 01:26:37.88 +60:38:02.5
127.23609 -1.94327 galactic Cas Second-epoch detections are separated by 2.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:26:37.88 +60:38:02.5 (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 01:26:37.88 +60:38:02.5: 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 01:26:37.88 +60:38:02.5: 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 23.4308* 01 26 37.88 +60 38 02.5 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,2461214.9308,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 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 23.4308 2461214.9308 11.21 01:41:44.40 +64:14:44.1
128.36353 1.90560 galactic Cas Second-epoch detections are separated by 0.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512898161208515840 | 01:41:38.37 +64:14:54.1 (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 01:41:44.40 +64:14:44.1: 11.90 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:44.40 +64:14:44.1: 13.77 +/- 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 23.4308* 01 41 44.40 +64 14 44.1 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 512898161208515840,2461214.9308,11.21,0.05,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 512898161208515840 20260623.4308 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 23.4308 2461214.9308 11.19 01:13:19.49 +61:29:25.8
125.54117 -1.27032 galactic Cas Second-epoch detections are separated by 1.1" and 6.9 pix
The object was found in VSX 4" Gaia DR3 522571492708068608
Type: ROT
# Max. Min./Amp. JD0 Period
14.070 G 14.120 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:19.49 +61:29:25.8: 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 01:13:19.49 +61:29:25.8: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 13 19.49 +61 29 25.8 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
Gaia DR3 522571492708068608,2461214.9308,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522571492708068608 20260623.4308 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 23.4308 2461214.9308 11.23 01:28:33.88 +62:13:51.8
127.24157 -0.32963 galactic Cas Second-epoch detections are separated by 1.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:28:33.88 +62:13:51.8 (user input) | T | P | (position from user input) J-Ks=0.597+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:33.88 +62:13:51.8: 12.35 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:33.88 +62:13:51.8: 13.69 +/- 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 23.4308* 01 28 33.88 +62 13 51.8 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,2461214.9308,11.23,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.13 01:30:00.83 +60:41:03.8
127.63924 -1.83430 galactic Cas Second-epoch detections are separated by 1.9" and 6.8 pix
The object was found in VSX18" Gaia DR3 510605576382958976
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.600 G 13.670 G 0.014413800000 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 01:30:00.83 +60:41:03.8: 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 01:30:00.83 +60:41:03.8: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 30 00.83 +60 41 03.8 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 510605576382958976,2461214.9308,11.13,0.05,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 510605576382958976 20260623.4308 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 23.4308 2461214.9308 11.13 01:35:41.78 +61:13:11.8
128.23463 -1.19531 galactic Cas Second-epoch detections are separated by 1.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:35:41.78 +61:13:11.8 (user input) | T | P | (position from user input) J-Ks=0.460+/- (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:41.78 +61:13:11.8: 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 01:35:41.78 +61:13:11.8: 13.63 +/- 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 23.4308* 01 35 41.78 +61 13 11.8 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
target,2461214.9308,11.13,0.05,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
target 20260623.4308 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 23.4308 2461214.9308 11.33 01:12:41.27 +61:18:07.5
125.48094 -1.46445 galactic Cas Second-epoch detections are separated by 1.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:41.27 +61:18:07.5 (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 01:12:41.27 +61:18:07.5: 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 01:12:41.27 +61:18:07.5: 13.98 +/- 0.06 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 23.4308* 01 12 41.27 +61 18 07.5 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,2461214.9308,11.33,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.19 02:00:06.59 +59:00:32.1
131.68371 -2.69101 galactic Cas Second-epoch detections are separated by 1.4" and 7.7 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 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 02:00:06.59 +59:00:32.1: 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 02:00:06.59 +59:00:32.1: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 23.4308* 02 00 06.59 +59 00 32.1 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 507781618204489856,2461214.9308,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507781618204489856 20260623.4308 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 23.4308 2461214.9308 11.39 01:33:08.71 +61:46:13.3
127.84307 -0.70304 galactic Cas Second-epoch detections are separated by 4.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:33:08.71 +61:46:13.3 (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 01:33:08.71 +61:46:13.3: 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 01:33:08.71 +61:46:13.3: 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 23.4308* 01 33 08.71 +61 46 13.3 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
target,2461214.9308,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 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 23.4308 2461214.9308 11.20 01:38:51.88 +59:27:14.9
128.93335 -2.86385 galactic Cas Second-epoch detections are separated by 2.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 509544685102980608 | 01:38:52.68 +59:26:46.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.615+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:51.88 +59:27:14.9: 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 01:38:51.88 +59:27:14.9: 14.08 +/- 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 23.4308* 01 38 51.88 +59 27 14.9 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 509544685102980608,2461214.9308,11.20,0.05,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 509544685102980608 20260623.4308 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 23.4308 2461214.9308 11.15 01:29:48.14 +63:19:36.6
127.22169 0.77507 galactic Cas Second-epoch detections are separated by 1.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:29:48.14 +63:19:36.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:48.14 +63:19:36.6: 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 01:29:48.14 +63:19:36.6: 13.75 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 23.4308* 01 29 48.14 +63 19 36.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.14 01:28:00.38 +61:23:58.1
127.29481 -1.16212 galactic Cas Second-epoch detections are separated by 1.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:28:00.38 +61:23:58.1 (user input) | T | P | (position from user input) J-Ks=0.956+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:00.38 +61:23:58.1: 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 01:28:00.38 +61:23:58.1: 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 23.4308* 01 28 00.38 +61 23 58.1 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,2461214.9308,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.15 01:28:07.26 +65:26:19.1
126.73511 2.83812 galactic Cas Second-epoch detections are separated by 1.4" and 6.9 pix
The object was found in VSX22" Gaia DR3 513262546232084352
Type: S
# Max. Min./Amp. JD0 Period
18.180 G 19.060 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:07.26 +65:26:19.1: 11.18 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:07.26 +65:26:19.1: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.71 +/- 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 23.4308* 01 28 07.26 +65 26 19.1 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 513262546232084352,2461214.9308,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 513262546232084352 20260623.4308 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.11 01:27:34.33 +57:48:25.8
127.74684 -4.72638 galactic Cas Second-epoch detections are separated by 4.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413087553653222272 | 01:27:32.01 +57:48:40.0 (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 01:27:34.33 +57:48:25.8: 12.37 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:34.33 +57:48:25.8: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 23.4308* 01 27 34.33 +57 48 25.8 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 413087553653222272,2461214.9308,11.11,0.05,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
Gaia DR3 413087553653222272 20260623.4308 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 23.4308 2461214.9308 11.19 01:21:45.41 +58:34:15.4
126.88588 -4.06785 galactic Cas Second-epoch detections are separated by 3.3" and 6.9 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 01:21:45.41 +58:34:15.4: 12.66 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:45.41 +58:34:15.4: 13.92 +/- 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 23.4308* 01 21 45.41 +58 34 15.4 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
ZTF J012144.11+583432.6,2461214.9308,11.19,0.05,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
ZTF J012144.11+583432.6 20260623.4308 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 23.4308 2461214.9308 11.14 01:47:51.52 +61:11:12.3
129.67803 -0.94383 galactic Cas Second-epoch detections are separated by 2.9" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511214048684134528 | 01:47:54.00 +61:10:49.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.225+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:51.52 +61:11:12.3: 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 01:47:51.52 +61:11:12.3: 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 23.4308* 01 47 51.52 +61 11 12.3 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 511214048684134528,2461214.9308,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511214048684134528 20260623.4308 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.10 01:24:54.97 +59:41:48.6
127.14919 -2.90050 galactic Cas Second-epoch detections are separated by 3.5" and 7.7 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 | 01:24:54.97 +59:41:48.6 (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 01:24:54.97 +59:41:48.6: 12.98 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:54.97 +59:41:48.6: 13.98 +/- 0.06 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 23.4308* 01 24 54.97 +59 41 48.6 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,2461214.9308,11.10,0.05,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 20260623.4308 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 23.4308 2461214.9308 10.99 01:09:25.09 +64:35:19.3
124.86013 1.78428 galactic Cas Second-epoch detections are separated by 1.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:09:25.09 +64:35:19.3 (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 01:09:25.09 +64:35:19.3: 12.50 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:25.09 +64:35:19.3: 13.85 +/- 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 23.4308* 01 09 25.09 +64 35 19.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 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 23.4308 2461214.9308 11.15 01:07:39.07 +59:59:18.1
124.96047 -2.81951 galactic Cas Second-epoch detections are separated by 2.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:39.07 +59:59:18.1 (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 01:07:39.07 +59:59:18.1: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.07 +59:59:18.1: 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 23.4308* 01 07 39.07 +59 59 18.1 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,2461214.9308,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.10 01:07:00.18 +61:28:29.6
124.78958 -1.34071 galactic Cas Second-epoch detections are separated by 1.5" and 6.8 pix
The object was found in VSX15" Gaia DR3 522542355648755328
Type: L
# Max. Min./Amp. JD0 Period
17.340 G 17.500 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 01:07:00.18 +61:28:29.6: 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 01:07:00.18 +61:28:29.6: 13.51 +/- 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 23.4308* 01 07 00.18 +61 28 29.6 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 522542355648755328,2461214.9308,11.10,0.05,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
Gaia DR3 522542355648755328 20260623.4308 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 23.4308 2461214.9308 11.06 01:36:49.12 +62:46:52.0
128.09435 0.36511 galactic Cas Second-epoch detections are separated by 2.2" and 7.1 pix
The object was found in VSX15" Gaia DR3 512426436360507392
Type: L
# Max. Min./Amp. JD0 Period
13.400 G 13.620 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:49.12 +62:46:52.0: 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 01:36:49.12 +62:46:52.0: 13.62 +/- 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 23.4308* 01 36 49.12 +62 46 52.0 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 512426436360507392,2461214.9308,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512426436360507392 20260623.4308 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.01 01:25:27.62 +59:27:15.4
127.24935 -3.13197 galactic Cas Second-epoch detections are separated by 0.3" and 7.2 pix
The object was found in VSX 4" 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 01:25:27.62 +59:27:15.4: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:27.62 +59:27:15.4: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 25 27.62 +59 27 15.4 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510073344036983552,2461214.9308,11.01,0.05,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
Gaia DR3 510073344036983552 20260623.4308 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 23.4308 2461214.9308 11.01 01:40:18.28 +61:21:04.8
128.75562 -0.96665 galactic Cas Second-epoch detections are separated by 0.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:40:18.28 +61:21:04.8 (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 01:40:18.28 +61:21:04.8: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:18.28 +61:21:04.8: 13.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 23.4308* 01 40 18.28 +61 21 04.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 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 23.4308 2461214.9308 10.96 01:09:24.50 +58:01:47.9
125.31711 -4.75853 galactic Cas Second-epoch detections are separated by 1.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:09:24.50 +58:01:47.9 (user input) | T | P | (position from user input) J-Ks=0.462+/-0.041 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:24.50 +58:01:47.9: 12.54 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:24.50 +58:01:47.9: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 09 24.50 +58 01 47.9 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
target,2461214.9308,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 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 23.4308 2461214.9308 11.18 01:40:10.62 +64:37:21.8
128.12584 2.24361 galactic Cas Second-epoch detections are separated by 5.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:40:10.62 +64:37:21.8 (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 01:40:10.62 +64:37:21.8: 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 01:40:10.62 +64:37:21.8: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 40 10.62 +64 37 21.8 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,2461214.9308,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.03 01:10:43.68 +60:59:19.2
125.26979 -1.79549 galactic Cas Second-epoch detections are separated by 0.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:10:43.68 +60:59:19.2 (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 01:10:43.68 +60:59:19.2: 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 01:10:43.68 +60:59:19.2: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 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 23.4308* 01 10 43.68 +60 59 19.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 10.96 01:13:27.25 +59:57:16.9
125.68783 -2.79919 galactic Cas Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:13:27.25 +59:57:16.9 (user input) | T | P | (position from user input) J-Ks=0.257+/-0.049 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:27.25 +59:57:16.9: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:27.25 +59:57:16.9: 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 23.4308* 01 13 27.25 +59 57 16.9 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
target,2461214.9308,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 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 23.4308 2461214.9308 10.83 01:43:26.18 +58:38:20.1
129.66781 -3.55113 galactic Cas Second-epoch detections are separated by 1.3" and 7.5 pix
The object was found in VSX17" 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 01:43:26.18 +58:38:20.1: 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 01:43:26.18 +58:38:20.1: 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 23.4308* 01 43 26.18 +58 38 20.1 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 506084487648397824,2461214.9308,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506084487648397824 20260623.4308 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 10.96 01:29:02.62 +58:46:08.5
127.80087 -3.74676 galactic Cas Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J012906.85+584639.3 | 01:29:06.84 +58:46:39.2 (Gaia DR3) | L (local) | (local) | Gaia3var=VARIABLE J-Ks=0.828+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:02.62 +58:46:08.5: 12.74 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:02.62 +58:46:08.5: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 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 23.4308* 01 29 02.62 +58 46 08.5 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
ASASSN-V J012906.85+584639.3,2461214.9308,10.96,0.05,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
ASASSN-V J012906.85+584639.3 20260623.4308 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 23.4308 2461214.9308 10.89 01:28:32.98 +61:12:19.4
127.38704 -1.34493 galactic Cas Second-epoch detections are separated by 1.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | PQ Cas | 01:28:36.18 +61:12:07.5 (Gaia DR3) | SR (local) | 2458436.69130 (local) | Gaia3var=VARIABLE SpType: S 1975AbaOB..47....3D [D75b] Star 4
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:32.98 +61:12:19.4: 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 01:28:32.98 +61:12:19.4: 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 23.4308* 01 28 32.98 +61 12 19.4 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
PQ Cas,2461214.9308,10.89,0.05,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
PQ Cas 20260623.4308 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 23.4308 2461214.9308 10.99 01:35:27.50 +60:33:47.1
128.31807 -1.84749 galactic Cas Second-epoch detections are separated by 2.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 01:35:27.50 +60:33:47.1: 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 01:35:27.50 +60:33:47.1: 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 23.4308* 01 35 27.50 +60 33 47.1 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
Gaia DR3 509811625915787136,2461214.9308,10.99,0.05,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 509811625915787136 20260623.4308 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 23.4308 2461214.9308 10.95 01:34:16.41 +60:57:35.2
128.10882 -1.48068 galactic Cas Second-epoch detections are separated by 2.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:34:16.41 +60:57:35.2 (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 01:34:16.41 +60:57:35.2: 12.59 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:16.41 +60:57:35.2: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 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 23.4308* 01 34 16.41 +60 57 35.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 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 23.4308 2461214.9308 10.95 01:11:50.59 +58:25:22.0
125.60833 -4.34289 galactic Cas Second-epoch detections are separated by 3.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.9730+58.4179 | 01:11:52.82 +58:25:17.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.764+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:50.59 +58:25:22.0: 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 01:11:50.59 +58:25:22.0: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 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 23.4308* 01 11 50.59 +58 25 22.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.9730+58.4179,2461214.9308,10.95,0.05,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
ATO J017.9730+58.4179 20260623.4308 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 23.4308 2461214.9308 10.86 02:07:26.11 +59:18:26.5
132.50417 -2.14464 galactic Cas Second-epoch detections are separated by 1.2" and 7.7 pix
The object was found in VSX 6" Gaia DR3 507097855110998912
Type: ROT
# Max. Min./Amp. JD0 Period
18.340 G 18.650 G 3.249360000000
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 02:07:26.11 +59:18:26.5: 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 02:07:26.11 +59:18:26.5: 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 23.4308* 02 07 26.11 +59 18 26.5 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 507097855110998912,2461214.9308,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507097855110998912 20260623.4308 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 10.73 01:26:36.86 +59:41:34.8
127.36230 -2.87582 galactic Cas Second-epoch detections are separated by 2.9" and 7.5 pix
The object was found in VSX 1" Gaia DR3 510083239641443712
Type: ROT
# Max. Min./Amp. JD0 Period
13.540 G 13.590 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 01:26:36.86 +59:41:34.8: 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 01:26:36.86 +59:41:34.8: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 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 23.4308* 01 26 36.86 +59 41 34.8 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510083239641443712,2461214.9308,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510083239641443712 20260623.4308 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 10.70 01:17:15.43 +58:35:37.4
126.29902 -4.10913 galactic Cas Second-epoch detections are separated by 1.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:15.43 +58:35:37.4: 12.77 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:15.43 +58:35:37.4: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 17 15.43 +58 35 37.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J019.3185+58.5958,2461214.9308,10.70,0.05,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
ATO J019.3185+58.5958 20260623.4308 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 23.4308 2461214.9308 10.91 01:29:42.06 +61:54:40.5
127.41981 -0.62663 galactic Cas Second-epoch detections are separated by 1.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510818331883633920 | 01:29:42.46 +61:55:01.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.251+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:42.06 +61:54:40.5: 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 01:29:42.06 +61:54:40.5: 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 23.4308* 01 29 42.06 +61 54 40.5 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 510818331883633920,2461214.9308,10.91,0.05,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 510818331883633920 20260623.4308 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 23.4308 2461214.9308 10.74 01:06:25.99 +61:41:31.6
124.70900 -1.12789 galactic Cas Second-epoch detections are separated by 3.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:25.99 +61:41:31.6 (user input) | T | P | (position from user input) J-Ks=0.921+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:25.99 +61:41:31.6: 10.49 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:25.99 +61:41:31.6: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.93 +/- 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 23.4308* 01 06 25.99 +61 41 31.6 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
target,2461214.9308,10.74,0.05,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 20260623.4308 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 23.4308 2461214.9308 10.63 01:22:28.43 +61:07:37.6
126.67101 -1.51912 galactic Cas Second-epoch detections are separated by 2.3" and 7.3 pix
The object was found in VSX20" Gaia DR3 510501328936368640
Type: RS
# Max. Min./Amp. JD0 Period
13.970 G 14.040 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:28.43 +61:07:37.6: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:28.43 +61:07:37.6: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 22 28.43 +61 07 37.6 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 510501328936368640,2461214.9308,10.63,0.05,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
Gaia DR3 510501328936368640 20260623.4308 10.63CV 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 23.4308 2461214.9308 10.72 01:11:33.69 +62:10:04.4
125.27853 -0.61214 galactic Cas Second-epoch detections are separated by 2.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:11:33.69 +62:10:04.4 (user input) | T | P | (position from user input) J-Ks=0.218+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:33.69 +62:10:04.4: 13.39 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:33.69 +62:10:04.4: 13.09 +/- 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 23.4308* 01 11 33.69 +62 10 04.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,10.72,0.05,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
target 20260623.4308 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 23.4308 2461214.9308 10.56 01:20:45.20 +57:55:10.6
126.83000 -4.73009 galactic Cas Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 01:20:45.20 +57:55:10.6: 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 01:20:45.20 +57:55:10.6: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 23.4308* 01 20 45.20 +57 55 10.6 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 413797116609704704,2461214.9308,10.56,0.05,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 413797116609704704 20260623.4308 10.56CV 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 23.4308 2461214.9308 10.62 01:19:08.81 +60:33:58.7
126.33211 -2.12238 galactic Cas Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 01:19:08.81 +60:33:58.7: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:08.81 +60:33:58.7: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 19 08.81 +60 33 58.7 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 510378080556092032,2461214.9308,10.62,0.05,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
Gaia DR3 510378080556092032 20260623.4308 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 23.4308 2461214.9308 10.52 01:31:30.69 +62:00:58.6
127.61422 -0.49061 galactic Cas Second-epoch detections are separated by 1.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 510793489784142080 | 01:31:30.04 +62:01:32.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.454+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:30.69 +62:00:58.6: 11.42 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:30.69 +62:00:58.6: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 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 23.4308* 01 31 30.69 +62 00 58.6 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
Large-amplitude variable Gaia DR2 510793489784142080,2461214.9308,10.52,0.05,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
Large-amplitude variable Gaia DR2 510793489784142080 20260623.4308 10.52CV 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 23.4308 2461214.9308 10.26 01:37:25.55 +63:41:28.2
128.00122 1.27297 galactic Cas Second-epoch detections are separated by 1.7" and 7.3 pix
The object was found in VSX 1" ASASSN-V J013725.59+634128.8
Type: DCEP
# Max. Min./Amp. JD0 Period
13.174 r Y 0.560 r 2457052.73600 3.238890000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:25.55 +63:41:28.2: 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 01:37:25.55 +63:41:28.2: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 23.4308* 01 37 25.55 +63 41 28.2 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013725.59+634128.8,2461214.9308,10.26,0.05,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
ASASSN-V J013725.59+634128.8 20260623.4308 10.26CV 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 23.4308 2461214.9308 9.93 01:35:24.90 +60:39:15.3
128.29733 -1.75855 galactic Cas Second-epoch detections are separated by 0.1" and 7.2 pix
The object was found in VSX 7" 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 01:35:24.90 +60:39:15.3: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:24.90 +60:39:15.3: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 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 23.4308* 01 35 24.90 +60 39 15.3 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 509819081975016960,2461214.9308,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509819081975016960 20260623.4308 9.93CV 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 23.4308 2461214.9308 9.90 01:28:26.76 +60:23:27.4
127.49133 -2.15277 galactic Cas Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510221984265315200 | 01:28:28.01 +60:23:13.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.247+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:26.76 +60:23:27.4: 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 01:28:26.76 +60:23:27.4: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 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 23.4308* 01 28 26.76 +60 23 27.4 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 510221984265315200,2461214.9308,9.90,0.05,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 510221984265315200 20260623.4308 9.90CV 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 23.4308 2461214.9308 9.69 01:30:43.78 +60:47:34.4
127.70942 -1.71387 galactic Cas Second-epoch detections are separated by 1.1" and 7.3 pix
The object was found in VSX 1" Gaia DR3 510607049549022848
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.370 G 12.390 G 1.920160000000 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 01:30:43.78 +60:47:34.4: 12.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:43.78 +60:47:34.4: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 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 23.4308* 01 30 43.78 +60 47 34.4 9.7 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 510607049549022848,2461214.9308,9.69,0.05,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 510607049549022848 20260623.4308 9.69CV 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 23.4308 2461214.9308 9.33 01:52:09.02 +58:27:40.5
130.81803 -3.47784 galactic Cas Second-epoch detections are separated by 1.9" and 7.8 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 506205674446445952 | 01:52:09.03 +58:27:25.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.384+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:09.02 +58:27:40.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:09.02 +58:27:40.5: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 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 23.4308* 01 52 09.02 +58 27 40.5 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
Gaia DR3 506205674446445952,2461214.9308,9.33,0.05,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
Gaia DR3 506205674446445952 20260623.4308 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 23.4308 2461214.9308 8.46 01:19:35.43 +60:03:33.3
126.44172 -2.62051 galactic Cas Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510326059911501184 | 01:19:36.00 +60:03:49.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1935BSD...C01....0S BSD 8- 783 J-Ks=0.314+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:35.43 +60:03:33.3: 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 01:19:35.43 +60:03:33.3: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 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 23.4308* 01 19 35.43 +60 03 33.3 8.5 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 510326059911501184,2461214.9308,8.46,0.05,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 510326059911501184 20260623.4308 8.46CV 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 23.4308 2461214.9308 7.71 01:35:37.53 +61:16:49.4
128.21591 -1.13720 galactic Cas Second-epoch detections are separated by 1.6" and 7.0 pix
The object was found in VSX 9" Gaia DR3 509978579881384704
Type: E
# Max. Min./Amp. JD0 Period
12.390 G 12.580 G 1.177150000000 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 01:35:37.53 +61:16:49.4: 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 01:35:37.53 +61:16:49.4: 10.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.23 +/- 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 23.4308* 01 35 37.53 +61 16 49.4 7.7 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 509978579881384704,2461214.9308,7.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509978579881384704 20260623.4308 7.71CV 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 23.4308 2461214.9308 9.79 01:23:31.46 +58:41:47.7
127.09949 -3.91529 galactic Cas Second-epoch detections are separated by 0.8" and 7.3 pix
The object was found in VSX23" 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 01:23:31.46 +58:41:47.7: 12.09 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:31.46 +58:41:47.7: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.50 +/- 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 23.4308* 01 23 31.46 +58 41 47.7 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413949673852809088,2461214.9308,9.79,0.05,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
Gaia DR3 413949673852809088 20260623.4308 9.79CV 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 23.4308 2461214.9308 10.54 01:18:28.19 +58:11:23.1
126.49911 -4.49465 galactic Cas Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 01:18:28.19 +58:11:23.1: 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 01:18:28.19 +58:11:23.1: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 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 23.4308* 01 18 28.19 +58 11 23.1 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J019.6245+58.1745,2461214.9308,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J019.6245+58.1745 20260623.4308 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 10.69 01:24:45.35 +63:08:25.9
126.68480 0.51181 galactic Cas Second-epoch detections are separated by 1.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | V1319 Cas | 01:24:40.42 +63:08:29.7 (Gaia DR3) | EB (local) | 2.804870000000 (local) | Gaia3var=VARIABLE SpType: OB 1954BOTT....1i..21G [GG54] 14 J-Ks=1.109+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:45.35 +63:08:25.9: 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 01:24:45.35 +63:08:25.9: 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 23.4308* 01 24 45.35 +63 08 25.9 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
V1319 Cas,2461214.9308,10.69,0.05,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
V1319 Cas 20260623.4308 10.69CV 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 23.4308 2461214.9308 10.76 01:51:09.37 +64:52:46.3
129.21815 2.73916 galactic Cas Second-epoch detections are separated by 1.0" and 7.2 pix
The object was found in VSX 3" 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 01:51:09.37 +64:52:46.3: 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 01:51:09.37 +64:52:46.3: 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 23.4308* 01 51 09.37 +64 52 46.3 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 518229967963921664,2461214.9308,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518229967963921664 20260623.4308 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 10.78 01:46:23.30 +61:12:57.6
129.49877 -0.95318 galactic Cas Second-epoch detections are separated by 2.4" and 7.5 pix
The object was found in VSX21" Gaia DR3 511217282805374208
Type: ROT
# Max. Min./Amp. JD0 Period
18.220 G 18.350 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:23.30 +61:12:57.6: 12.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:23.30 +61:12:57.6: 13.81 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 46 23.30 +61 12 57.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511217282805374208,2461214.9308,10.78,0.05,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 511217282805374208 20260623.4308 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 23.4308 2461214.9308 10.87 01:22:23.76 +61:13:50.9
126.64924 -1.41730 galactic Cas Second-epoch detections are separated by 1.8" and 7.3 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 01:22:23.76 +61:13:50.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:23.76 +61:13:50.9: 15.68 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.68 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 22 23.76 +61 13 50.9 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
NSVS J0122238+611352,2461214.9308,10.87,0.05,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
NSVS J0122238+611352 20260623.4308 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 23.4308 2461214.9308 10.84 01:36:16.35 +60:12:25.1
128.47835 -2.18107 galactic Cas Second-epoch detections are separated by 0.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 509768332640107392 | 01:36:16.56 +60:11:46.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:16.35 +60:12:25.1: 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 01:36:16.35 +60:12:25.1: 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 23.4308* 01 36 16.35 +60 12 25.1 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509768332640107392,2461214.9308,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509768332640107392 20260623.4308 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 10.95 02:01:03.66 +64:43:34.0
130.27865 2.85211 galactic Cas Second-epoch detections are separated by 0.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:01:03.66 +64:43:34.0 (user input) | T | P | (position from user input) J-Ks=0.437+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:03.66 +64:43:34.0: 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 02:01:03.66 +64:43:34.0: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 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 23.4308* 02 01 03.66 +64 43 34.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 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 23.4308 2461214.9308 11.00 02:15:10.56 +58:07:01.4
133.82491 -2.97267 galactic Per Second-epoch detections are separated by 1.3" and 7.8 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 J033.7918+58.1304 | 02:15:08.45 +58:07:26.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:10.56 +58:07:01.4: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:10.56 +58:07:01.4: 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 23.4308* 02 15 10.56 +58 07 01.4 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
ATO J033.7918+58.1304,2461214.9308,11.00,0.05,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
ATO J033.7918+58.1304 20260623.4308 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 23.4308 2461214.9308 10.99 02:00:32.81 +59:40:06.4
131.56341 -2.04014 galactic Cas Second-epoch detections are separated by 2.0" and 7.8 pix
The object was found in VSX 3" 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 02:00:32.81 +59:40:06.4: 11.51 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.81 +59:40:06.4: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 23.4308* 02 00 32.81 +59 40 06.4 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J020033.07+594008.7,2461214.9308,10.99,0.05,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
ZTF J020033.07+594008.7 20260623.4308 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 23.4308 2461214.9308 10.95 01:06:55.55 +59:18:56.6
124.91039 -3.49652 galactic Cas Second-epoch detections are separated by 1.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:55.55 +59:18:56.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.55 +59:18:56.6: 13.13 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.55 +59:18:56.6: 13.85 +/- 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 23.4308* 01 06 55.55 +59 18 56.6 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
target,2461214.9308,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 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 23.4308 2461214.9308 10.89 01:17:24.25 +57:40:30.3
126.41114 -5.02115 galactic Cas Second-epoch detections are separated by 1.6" and 7.4 pix
The object was found in VSX19" Gaia DR3 413455924410764672
Type: ROT
# Max. Min./Amp. JD0 Period
15.590 G 15.640 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 01:17:24.25 +57:40:30.3: 12.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:24.25 +57:40:30.3: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 17 24.25 +57 40 30.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413455924410764672,2461214.9308,10.89,0.05,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 413455924410764672 20260623.4308 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 23.4308 2461214.9308 10.95 01:13:39.02 +58:10:50.7
125.86574 -4.56441 galactic Cas Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 01:13:39.02 +58:10:50.7: 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 01:13:39.02 +58:10:50.7: 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 23.4308* 01 13 39.02 +58 10 50.7 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J018.4234+58.1762,2461214.9308,10.95,0.05,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
ATO J018.4234+58.1762 20260623.4308 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 23.4308 2461214.9308 11.03 01:09:22.62 +57:26:31.0
125.35420 -5.34541 galactic Cas Second-epoch detections are separated by 1.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 01:09:22.62 +57:26:31.0: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.62 +57:26:31.0: 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 23.4308* 01 09 22.62 +57 26 31.0 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.3204+57.4562,2461214.9308,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.3204+57.4562 20260623.4308 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 10.98 01:38:04.13 +58:10:23.7
129.06502 -4.14214 galactic Cas Second-epoch detections are separated by 2.6" and 7.6 pix
The object was found in VSX23" Gaia DR3 508962699851411840
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
16.190 G 16.240 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:04.13 +58:10:23.7: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:04.13 +58:10:23.7: 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 23.4308* 01 38 04.13 +58 10 23.7 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508962699851411840,2461214.9308,10.98,0.05,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
Gaia DR3 508962699851411840 20260623.4308 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 23.4308 2461214.9308 11.07 01:36:50.75 +59:55:48.5
128.59711 -2.44121 galactic Cas Second-epoch detections are separated by 1.1" and 7.3 pix
The object was found in VSX 0" Gaia DR3 509760361181182976
Type: ROT
# Max. Min./Amp. JD0 Period
13.870 G 13.910 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:50.75 +59:55:48.5: 12.76 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:50.75 +59:55:48.5: 14.03 +/- 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 23.4308* 01 36 50.75 +59 55 48.5 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 509760361181182976,2461214.9308,11.07,0.05,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 509760361181182976 20260623.4308 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 23.4308 2461214.9308 11.06 01:26:05.59 +59:01:15.6
127.38745 -3.55062 galactic Cas Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.5231+59.0209 | 01:26:05.59 +59:01:15.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.314+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.59 +59:01:15.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.59 +59:01:15.6: 13.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 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 23.4308* 01 26 05.59 +59 01 15.6 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
ATO J021.5231+59.0209,2461214.9308,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.5231+59.0209 20260623.4308 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.07 01:51:26.83 +57:51:35.5
130.86758 -4.08432 galactic Per Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 01:51:26.83 +57:51:35.5: 12.85 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:26.83 +57:51:35.5: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 23.4308* 01 51 26.83 +57 51 35.5 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 506162862211871616,2461214.9308,11.07,0.05,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 506162862211871616 20260623.4308 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 23.4308 2461214.9308 11.04 02:16:40.51 +65:04:35.2
131.75922 3.67581 galactic Cas Second-epoch detections are separated by 1.3" and 7.1 pix
The object was found in VSX 9" Gaia DR3 515525925273268480
Type: ROT
# Max. Min./Amp. JD0 Period
15.530 G 15.550 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 02:16:40.51 +65:04:35.2: 12.92 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:40.51 +65:04:35.2: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 23.4308* 02 16 40.51 +65 04 35.2 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
Gaia DR3 515525925273268480,2461214.9308,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 515525925273268480 20260623.4308 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.12 01:38:05.76 +61:04:13.9
128.54593 -1.29162 galactic Cas Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:38:05.76 +61:04:13.9 (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 01:38:05.76 +61:04:13.9: 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 01:38:05.76 +61:04:13.9: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 38 05.76 +61 04 13.9 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,11.12,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.12 01:07:29.62 +63:10:59.6
124.74162 0.36790 galactic Cas Second-epoch detections are separated by 1.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:29.62 +63:10:59.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:29.62 +63:10:59.6: 11.49 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:29.62 +63:10:59.6: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 23.4308* 01 07 29.62 +63 10 59.6 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,2461214.9308,11.12,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.19 02:16:08.08 +58:18:13.4
133.88484 -2.75541 galactic Per Second-epoch detections are separated by 0.2" and 7.6 pix
The object was found in VSX 0" 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 02:16:08.08 +58:18:13.4: 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 02:16:08.08 +58:18:13.4: 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 23.4308* 02 16 08.08 +58 18 13.4 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 458762778499159168,2461214.9308,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458762778499159168 20260623.4308 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 23.4308 2461214.9308 11.10 01:56:57.31 +63:00:31.0
130.28641 1.07618 galactic Cas Second-epoch detections are separated by 1.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:56:57.31 +63:00:31.0 (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 01:56:57.31 +63:00:31.0: 13.11 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:57.31 +63:00:31.0: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.92 +/- 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 23.4308* 01 56 57.31 +63 00 31.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461214.9308,11.10,0.05,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 20260623.4308 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 23.4308 2461214.9308 10.96 01:32:05.61 +61:59:26.9
127.68566 -0.50512 galactic Cas Second-epoch detections are separated by 2.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510798197068398848 | 01:32:04.51 +61:59:00.7 (Gaia DR3) | DSCT/GDOR (local) | A (local) | Gaia3var=VARIABLE SpType: F5 1960IzKry..24..160B [B60] +61 281 J-Ks=0.127+/-0.036 (A)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:05.61 +61:59:26.9: 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 01:32:05.61 +61:59:26.9: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 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 23.4308* 01 32 05.61 +61 59 26.9 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 510798197068398848,2461214.9308,10.96,0.05,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 510798197068398848 20260623.4308 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 23.4308 2461214.9308 11.28 01:28:13.20 +58:35:17.9
127.72081 -3.94102 galactic Cas Second-epoch detections are separated by 1.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413183142447748352 | 01:28:16.87 +58:35:38.5 (Gaia DR3) | ROT (local) | M (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.983+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:13.20 +58:35:17.9: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:13.20 +58:35:17.9: 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 23.4308* 01 28 13.20 +58 35 17.9 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 413183142447748352,2461214.9308,11.28,0.05,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 413183142447748352 20260623.4308 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 23.4308 2461214.9308 11.02 01:22:11.01 +59:09:03.3
126.87191 -3.48543 galactic Cas Second-epoch detections are separated by 1.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413976852405588480 | 01:22:13.31 +59:08:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1960IzKry..24..160B [B60] +58 184 J-Ks=0.462+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:11.01 +59:09:03.3: 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 01:22:11.01 +59:09:03.3: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 23.4308* 01 22 11.01 +59 09 03.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413976852405588480,2461214.9308,11.02,0.05,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 413976852405588480 20260623.4308 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 23.4308 2461214.9308 11.24 02:15:04.06 +58:28:54.3
133.69523 -2.63146 galactic Per Second-epoch detections are separated by 0.6" and 7.7 pix
The object was found in VSX 1" 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 02:15:04.06 +58:28:54.3: 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 02:15:04.06 +58:28:54.3: 13.76 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 23.4308* 02 15 04.06 +58 28 54.3 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 506806798067617152,2461214.9308,11.24,0.05,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
Gaia DR3 506806798067617152 20260623.4308 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 23.4308 2461214.9308 11.08 01:20:13.59 +65:31:28.2
125.91084 2.81940 galactic Cas Second-epoch detections are separated by 1.6" and 6.6 pix
The object was found in VSX 1" V0897 Cas
Type: M
# Max. Min./Amp. JD0 Period
11.000 w < 13.600 w 2453559.60000 480.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:13.59 +65:31:28.2: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:13.59 +65:31:28.2: 16.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 20 13.59 +65 31 28.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0897 Cas,2461214.9308,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0897 Cas 20260623.4308 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.06 01:44:03.40 +61:54:43.7
129.08311 -0.32956 galactic Cas Second-epoch detections are separated by 0.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511486800591720192 | 01:44:01.89 +61:55:16.8 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: B1V 1999A&AS..136..313S Cl* NGC 654 Sto 94 J-Ks=12.609+/- (unrealisitic color!)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:03.40 +61:54:43.7: 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 01:44:03.40 +61:54:43.7: 13.94 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 44 03.40 +61 54 43.7 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
Gaia DR3 511486800591720192,2461214.9308,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511486800591720192 20260623.4308 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.22 01:28:07.23 +59:53:49.6
127.52168 -2.64734 galactic Cas Second-epoch detections are separated by 2.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510182298766565376 | 01:28:11.24 +59:54:05.3 (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 01:28:07.23 +59:53:49.6: 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 01:28:07.23 +59:53:49.6: 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 23.4308* 01 28 07.23 +59 53 49.6 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 510182298766565376,2461214.9308,11.22,0.05,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 510182298766565376 20260623.4308 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 23.4308 2461214.9308 10.94 01:08:59.21 +60:47:21.2
125.07271 -2.00956 galactic Cas Second-epoch detections are separated by 4.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 01:08:59.21 +60:47:21.2: 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 01:08:59.21 +60:47:21.2: 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 23.4308* 01 08 59.21 +60 47 21.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522440066710315904,2461214.9308,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522440066710315904 20260623.4308 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 23.4308 2461214.9308 11.16 01:50:39.82 +62:00:55.6
129.81910 -0.06176 galactic Cas Second-epoch detections are separated by 1.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 01:50:39.82 +62:00:55.6: 13.28 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:39.82 +62:00:55.6: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 01 50 39.82 +62 00 55.6 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 511356332360621440,2461214.9308,11.16,0.05,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 511356332360621440 20260623.4308 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 23.4308 2461214.9308 11.11 01:57:46.60 +59:59:17.5
131.14409 -1.82159 galactic Cas Second-epoch detections are separated by 1.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:57:46.60 +59:59:17.5 (user input) | T | P | (position from user input) J-Ks=1.192+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:46.60 +59:59:17.5: 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 01:57:46.60 +59:59:17.5: 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 23.4308* 01 57 46.60 +59 59 17.5 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,2461214.9308,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 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 23.4308 2461214.9308 11.20 01:51:13.62 +59:13:47.9
130.52336 -2.75768 galactic Cas Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506527487754339200 | 01:51:14.87 +59:13:19.2 (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 01:51:13.62 +59:13:47.9: 11.42 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:13.62 +59:13:47.9: 14.13 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.51 +/- 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 23.4308* 01 51 13.62 +59 13 47.9 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 506527487754339200,2461214.9308,11.20,0.05,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 506527487754339200 20260623.4308 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 23.4308 2461214.9308 11.30 01:51:05.54 +61:32:11.2
129.97778 -0.51654 galactic Cas Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:51:05.54 +61:32:11.2 (user input) | T | P | (position from user input) J-Ks=1.341+/-0.032 (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 01:51:05.54 +61:32:11.2: 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 01:51:05.54 +61:32:11.2: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.16 +/- 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 23.4308* 01 51 05.54 +61 32 11.2 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,2461214.9308,11.30,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.33 01:08:11.88 +62:14:21.0
124.88229 -0.56910 galactic Cas Second-epoch detections are separated by 2.5" and 6.7 pix
The object was found in VSX 3" Gaia DR3 522685876279259136
Type: ROT
# Max. Min./Amp. JD0 Period
14.350 G 14.370 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 01:08:11.88 +62:14:21.0: 12.14 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:11.88 +62:14:21.0: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 23.4308* 01 08 11.88 +62 14 21.0 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 522685876279259136,2461214.9308,11.33,0.05,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 522685876279259136 20260623.4308 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 23.4308 2461214.9308 11.21 01:27:14.37 +59:29:18.5
127.46891 -3.06753 galactic Cas Second-epoch detections are separated by 2.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510070767059145728 | 01:27:10.59 +59:29:36.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1961AbaOB..26...35K [KB61] +59 61 J-Ks=0.726+/-0.051 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:14.37 +59:29:18.5: 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 01:27:14.37 +59:29:18.5: 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 23.4308* 01 27 14.37 +59 29 18.5 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 510070767059145728,2461214.9308,11.21,0.05,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 510070767059145728 20260623.4308 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 23.4308 2461214.9308 11.17 01:10:04.93 +60:32:46.6
125.22370 -2.24248 galactic Cas Second-epoch detections are separated by 2.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 426345911537396096 | 01:10:02.14 +60:33:00.9 (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: F8 1935BSD...C01....0S BSD 8-1180
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:04.93 +60:32:46.6: 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 01:10:04.93 +60:32:46.6: 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 23.4308* 01 10 04.93 +60 32 46.6 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
Large-amplitude variable Gaia DR2 426345911537396096,2461214.9308,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 426345911537396096 20260623.4308 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.27 02:02:32.31 +58:06:03.4
132.23267 -3.48110 galactic Per Second-epoch detections are separated by 1.8" and 7.7 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 505442853895424256 | 02:02:33.95 +58:05:25.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.216+/-0.041 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:32.31 +58:06:03.4: 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 02:02:32.31 +58:06:03.4: 14.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 23.4308* 02 02 32.31 +58 06 03.4 11.3 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 505442853895424256,2461214.9308,11.27,0.05,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
Gaia DR3 505442853895424256 20260623.4308 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 23.4308 2461214.9308 11.36 01:51:52.69 +60:27:42.8
130.31827 -1.54019 galactic Cas Second-epoch detections are separated by 2.0" and 7.7 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 | 01:51:52.69 +60:27:42.8 (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 01:51:52.69 +60:27:42.8: 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 01:51:52.69 +60:27:42.8: 14.26 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.26 +/- 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 23.4308* 01 51 52.69 +60 27 42.8 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,2461214.9308,11.36,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.21 02:10:20.55 +63:36:42.3
131.56530 2.07041 galactic Cas Second-epoch detections are separated by 2.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:10:20.55 +63:36:42.3 (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 02:10:20.55 +63:36:42.3: 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 02:10:20.55 +63:36:42.3: 13.79 +/- 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 23.4308* 02 10 20.55 +63 36 42.3 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,2461214.9308,11.21,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.29 01:45:15.64 +59:38:17.5
129.69310 -2.52515 galactic Cas Second-epoch detections are separated by 1.4" and 7.5 pix
The object was found in VSX 2" Gaia DR3 506514018736899840
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.340 G 14.370 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 01:45:15.64 +59:38:17.5: 12.54 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:15.64 +59:38:17.5: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 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 23.4308* 01 45 15.64 +59 38 17.5 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 506514018736899840,2461214.9308,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506514018736899840 20260623.4308 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 23.4308 2461214.9308 11.22 01:44:31.82 +58:44:31.7
129.78629 -3.42125 galactic Cas Second-epoch detections are separated by 0.6" and 7.2 pix
The object was found in VSX13" Gaia DR3 506449830443978496
Type: ROT
# Max. Min./Amp. JD0 Period
18.630 G 18.850 G 6.663000000000
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 01:44:31.82 +58:44:31.7: 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 01:44:31.82 +58:44:31.7: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 23.4308* 01 44 31.82 +58 44 31.7 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 506449830443978496,2461214.9308,11.22,0.05,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 506449830443978496 20260623.4308 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 23.4308 2461214.9308 11.32 01:29:39.26 +63:18:45.7
127.20735 0.75863 galactic Cas Second-epoch detections are separated by 2.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512422794227736704 | 01:29:32.93 +63:18:37.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8Ib 1987ApJS...64..241S NGC 559 14
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:39.26 +63:18:45.7: 12.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:39.26 +63:18:45.7: 14.13 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.13 +/- 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 23.4308* 01 29 39.26 +63 18 45.7 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
Gaia DR3 512422794227736704,2461214.9308,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512422794227736704 20260623.4308 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 23.4308 2461214.9308 11.21 01:52:55.21 +59:33:30.7
130.65653 -2.38796 galactic Cas Second-epoch detections are separated by 0.9" and 7.3 pix
The object was found in VSX16" 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 01:52:55.21 +59:33:30.7: 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 01:52:55.21 +59:33:30.7: 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 23.4308* 01 52 55.21 +59 33 30.7 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 506553498077188608,2461214.9308,11.21,0.05,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 506553498077188608 20260623.4308 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 23.4308 2461214.9308 11.29 01:51:02.82 +59:06:43.0
130.52800 -2.87785 galactic Cas Second-epoch detections are separated by 2.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506520821965175424 | 01:51:02.15 +59:07:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:02.82 +59:06:43.0: 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 01:51:02.82 +59:06:43.0: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 23.4308* 01 51 02.82 +59 06 43.0 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 506520821965175424,2461214.9308,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506520821965175424 20260623.4308 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 23.4308 2461214.9308 11.41 02:01:06.65 +64:35:46.1
130.31849 2.72826 galactic Cas Second-epoch detections are separated by 5.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 518077479449762560 | 02:01:07.64 +64:35:03.8 (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 02:01:06.65 +64:35:46.1: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:06.65 +64:35:46.1: 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 23.4308* 02 01 06.65 +64 35 46.1 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 518077479449762560,2461214.9308,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518077479449762560 20260623.4308 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.23 02:02:24.46 +64:38:24.6
130.44063 2.80807 galactic Cas Second-epoch detections are separated by 4.1" and 7.5 pix
The object was found in VSX10" 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 02:02:24.46 +64:38:24.6: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:24.46 +64:38:24.6: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 23.4308* 02 02 24.46 +64 38 24.6 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
ASASSN-V J020225.96+643822.9,2461214.9308,11.23,0.05,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
ASASSN-V J020225.96+643822.9 20260623.4308 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 23.4308 2461214.9308 11.24 01:19:28.88 +59:54:37.8
126.44436 -2.76986 galactic Cas Second-epoch detections are separated by 1.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510323036254643328 | 01:19:24.22 +59:54:27.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B6 1935BSD...C01....0S BSD 8- 782 J-Ks=0.995+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:28.88 +59:54:37.8: 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 01:19:28.88 +59:54:37.8: 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 23.4308* 01 19 28.88 +59 54 37.8 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
Gaia DR3 510323036254643328,2461214.9308,11.24,0.05,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
Gaia DR3 510323036254643328 20260623.4308 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 23.4308 2461214.9308 11.37 01:51:40.28 +60:56:17.5
130.18327 -1.08270 galactic Cas Second-epoch detections are separated by 2.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 508195305151165312 | 01:51:34.71 +60:55:58.1 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.600+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:40.28 +60:56:17.5: 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 01:51:40.28 +60:56:17.5: 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 23.4308* 01 51 40.28 +60 56 17.5 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
Gaia DR3 508195305151165312,2461214.9308,11.37,0.05,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 508195305151165312 20260623.4308 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 23.4308 2461214.9308 11.53 01:19:08.05 +60:33:40.4
126.33111 -2.12760 galactic Cas Second-epoch detections are separated by 1.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510378080556092032 | 01:19:06.00 +60:34:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.495+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:08.05 +60:33:40.4: 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 01:19:08.05 +60:33:40.4: 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 23.4308* 01 19 08.05 +60 33 40.4 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 510378080556092032,2461214.9308,11.53,0.05,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
Gaia DR3 510378080556092032 20260623.4308 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 23.4308 2461214.9308 11.45 01:33:30.69 +58:02:22.8
128.49334 -4.37705 galactic Cas Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J023.3712+58.0394 | 01:33:30.69 +58:02:22.8 (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 +58:02:22.8: 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 01:33:30.69 +58:02:22.8: 14.24 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 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 23.4308* 01 33 30.69 +58 02 22.8 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 J023.3712+58.0394,2461214.9308,11.45,0.05,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 J023.3712+58.0394 20260623.4308 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 23.4308 2461214.9308 11.53 02:13:18.57 +61:26:42.4
132.55400 0.11231 galactic Cas Second-epoch detections are separated by 1.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:13:18.57 +61:26:42.4 (user input) | T | P | (position from user input) J-Ks=0.493+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:18.57 +61:26:42.4: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:18.57 +61:26:42.4: 14.21 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.21 +/- 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 23.4308* 02 13 18.57 +61 26 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
target,2461214.9308,11.53,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.53 01:44:33.57 +60:39:30.2
129.39746 -1.54478 galactic Cas Second-epoch detections are separated by 2.4" and 6.6 pix
The object was found in VSX17" Gaia DR3 509678172685831040
Type: ROT
# Max. Min./Amp. JD0 Period
15.830 G 15.870 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 01:44:33.57 +60:39:30.2: 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 01:44:33.57 +60:39:30.2: 14.31 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.31 +/- 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 23.4308* 01 44 33.57 +60 39 30.2 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
Gaia DR3 509678172685831040,2461214.9308,11.53,0.05,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
Gaia DR3 509678172685831040 20260623.4308 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 23.4308 2461214.9308 11.33 01:26:28.36 +59:41:35.6
127.34454 -2.87803 galactic Cas Second-epoch detections are separated by 3.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 01:26:28.36 +59:41:35.6: 12.85 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:28.36 +59:41:35.6: 14.04 +/- 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 23.4308* 01 26 28.36 +59 41 35.6 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 J021.6536+59.6928,2461214.9308,11.33,0.05,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 J021.6536+59.6928 20260623.4308 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 23.4308 2461214.9308 11.49 01:33:43.64 +59:31:30.7
128.27803 -2.90688 galactic Cas Second-epoch detections are separated by 3.1" and 7.7 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 J023.4238+59.5237 | 01:33:43.64 +59:31:30.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.433+/-0.037 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:43.64 +59:31:30.7: 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 01:33:43.64 +59:31:30.7: 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 23.4308* 01 33 43.64 +59 31 30.7 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 J023.4238+59.5237,2461214.9308,11.49,0.05,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
ATO J023.4238+59.5237 20260623.4308 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 23.4308 2461214.9308 11.59 01:58:11.48 +63:55:12.7
130.18897 1.99299 galactic Cas Second-epoch detections are separated by 2.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 517938833598880256 | 01:58:09.93 +63:54:46.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.964+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:11.48 +63:55:12.7: 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 01:58:11.48 +63:55:12.7: 14.40 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.40 +/- 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 23.4308* 01 58 11.48 +63 55 12.7 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
Gaia DR3 517938833598880256,2461214.9308,11.59,0.05,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 517938833598880256 20260623.4308 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 23.4308 2461214.9308 11.59 02:13:40.76 +65:08:14.4
131.44035 3.63307 galactic Cas Second-epoch detections are separated by 4.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:13:40.76 +65:08:14.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:40.76 +65:08:14.4: 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 02:13:40.76 +65:08:14.4: 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 23.4308* 02 13 40.76 +65 08 14.4 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,2461214.9308,11.59,0.05,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 20260623.4308 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 23.4308 2461214.9308 11.66 01:21:24.18 +62:18:31.1
126.40546 -0.36085 galactic Cas Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510994391181101440 | 01:21:22.41 +62:19:11.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9 1935BSD...C01....0S BSD 8-1812 J-Ks=0.395+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:24.18 +62:18:31.1: 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 01:21:24.18 +62:18:31.1: 14.66 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.66 +/- 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 23.4308* 01 21 24.18 +62 18 31.1 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
Gaia DR3 510994391181101440,2461214.9308,11.66,0.05,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 510994391181101440 20260623.4308 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 23.4308 2461214.9308 11.74 01:36:30.14 +60:46:39.5
128.40716 -1.61415 galactic Cas Second-epoch detections are separated by 2.1" and 7.1 pix
The object was found in VSX 2" Gaia DR3 509914155368970240
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.240 G 15.280 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 01:36:30.14 +60:46:39.5: 12.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:30.14 +60:46:39.5: 14.57 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.57 +/- 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 23.4308* 01 36 30.14 +60 46 39.5 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
Gaia DR3 509914155368970240,2461214.9308,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509914155368970240 20260623.4308 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 11.63 01:35:34.09 +61:18:03.4
128.20562 -1.11812 galactic Cas Second-epoch detections are separated by 1.3" and 7.0 pix
The object was found in VSX16" Gaia DR3 509979370155337088
Type: RS
# Max. Min./Amp. JD0 Period
16.450 G 16.560 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 01:35:34.09 +61:18:03.4: 13.11 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:34.09 +61:18:03.4: 14.69 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.41 +/- 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 23.4308* 01 35 34.09 +61 18 03.4 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 509979370155337088,2461214.9308,11.63,0.05,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
Gaia DR3 509979370155337088 20260623.4308 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 23.4308 2461214.9308 11.71 01:46:38.22 +60:09:00.0
129.75449 -1.98852 galactic Cas Second-epoch detections are separated by 3.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.6591+60.1406 | 01:46:38.19 +60:08:26.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.752+/-0.039 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.22 +60:09:00.0: 13.32 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:38.22 +60:09:00.0: 14.40 +/- 0.10 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 23.4308* 01 46 38.22 +60 09 00.0 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 J026.6591+60.1406,2461214.9308,11.71,0.05,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 J026.6591+60.1406 20260623.4308 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 23.4308 2461214.9308 11.63 01:37:08.39 +57:44:50.9
129.01969 -4.58307 galactic Cas Second-epoch detections are separated by 1.6" and 7.5 pix
The object was found in VSX 8" ZTF J013709.04+574444.3
Type: EW
# Max. Min./Amp. JD0 Period
18.009 r Y 0.323 r 2458379.91190 0.418442000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:08.39 +57:44:50.9: 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 01:37:08.39 +57:44:50.9: 14.44 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.44 +/- 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 23.4308* 01 37 08.39 +57 44 50.9 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
ZTF J013709.04+574444.3,2461214.9308,11.63,0.05,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
ZTF J013709.04+574444.3 20260623.4308 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 23.4308 2461214.9308 11.84 01:26:31.51 +62:18:32.6
126.99575 -0.28552 galactic Cas Second-epoch detections are separated by 1.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:26:31.51 +62:18:32.6 (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 01:26:31.51 +62:18:32.6: 11.56 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:31.51 +62:18:32.6: 14.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 23.4308* 01 26 31.51 +62 18 32.6 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,2461214.9308,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.4308 2461214.9308 12.01 01:27:06.73 +61:26:15.0
127.18358 -1.13941 galactic Cas Second-epoch detections are separated by 1.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:27:06.73 +61:26:15.0 (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 01:27:06.73 +61:26:15.0: 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 01:27:06.73 +61:26:15.0: 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 23.4308* 01 27 06.73 +61 26 15.0 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,2461214.9308,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260623.4308 12.01CV 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
## 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: 2461214.93112515 23.06.2026 10:20:39.213 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
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): 25326
Objects passed selection criteria: 25188
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 18097.2
Average stars matched: 16690.8 (92.2281 %)
Memory usage VmPeak: 128528 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 21 14:44:16 CDT 2026
VaST build number 1.0rc89-107-g3b0f95a5
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 23 06:13:27 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: 2461214.93112515 23.06.2026 10:20:39.213 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 345
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: 147 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): 188809
Objects passed selection criteria: 188328
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 143891
Average stars matched: 132022 (91.7514 %)
Memory usage VmPeak: 2000612 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 21 14:44:16 CDT 2026
VaST build number 1.0rc89-107-g3b0f95a5
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 23 06:20:00 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_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.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_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.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: 2461214.93053812
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cas-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_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits'
wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.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_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
Image size: 937.5'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: 01:42:54.955 +62:00:15.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:54.955 +62:00:15.93
Angular distance between the image centers 0.0549 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
Image size: 937.5'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: 01:42:58.703 +62:00:49.76 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:58.703 +62:00:49.76
Angular distance between the image centers 0.0653 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:42:54.955 +62:00:15.93
Second-epoch second image center 01:42:58.703 +62:00:49.76
Angular distance between the image centers 0.01192 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.wDdTazXlWg
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.l6y3LRfxUM
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_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits &> /tmp/tmp.DgZ5CpO2am
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits &> /tmp/tmp.RBxjKQ6nbf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.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 3 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_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
14.4 mag. fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
14.4 mag. fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.6 (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.wDdTazXlWg (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_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/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
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, bad_region=8115, passed=31559
Got 31559 stars (including 20507 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 272 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 181 matched stars entering correct_measured_positions(), 127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 166 matched stars entering correct_measured_positions(), 5658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.17"
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 329 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 253 matched stars entering correct_measured_positions(), 5719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.16"
Accuracy estimation diagnostic: 250 matched stars entering correct_measured_positions(), 8204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.77"
Excluding outliers - 250 stars left (next iteration limit 182)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=250 sigma_overall_arcsec=18.752 sigma_q1_arcsec=37.068 sigma_q2_arcsec=15.069 sigma_q3_arcsec=23.291 sigma_q4_arcsec=16.683 n_q1=21 n_q2=98 n_q3=46 n_q4=85 worst_quadrant_to_overall_ratio=1.977
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.l6y3LRfxUM (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_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/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
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, bad_region=8179, passed=31681
Got 31681 stars (including 20613 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 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 23244 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 23245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 23245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 975 stars left (next iteration limit 1072)
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=975 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.464 sigma_q2_arcsec=0.388 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.289 n_q1=173 n_q2=179 n_q3=388 n_q4=235 worst_quadrant_to_overall_ratio=1.235
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.DgZ5CpO2am (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_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.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_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.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_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1335, bad_region=3834, passed=17004
Got 17004 stars (including 12101 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits.wcscat
util/solve_plate_with_UCAC5 got 17004 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 13632 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 13629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 13628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits N_match=969 sigma_overall_arcsec=0.549 sigma_q1_arcsec=0.486 sigma_q2_arcsec=0.509 sigma_q3_arcsec=0.665 sigma_q4_arcsec=0.571 n_q1=322 n_q2=272 n_q3=254 n_q4=121 worst_quadrant_to_overall_ratio=1.212
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.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.RBxjKQ6nbf (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_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.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_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.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_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1317, bad_region=3702, passed=16384
Got 16384 stars (including 11619 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits.wcscat
util/solve_plate_with_UCAC5 got 16384 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 13160 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 13162 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 13162 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits N_match=971 sigma_overall_arcsec=0.539 sigma_q1_arcsec=0.523 sigma_q2_arcsec=0.487 sigma_q3_arcsec=0.666 sigma_q4_arcsec=0.542 n_q1=325 n_q2=285 n_q3=242 n_q4=119 worst_quadrant_to_overall_ratio=1.235
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.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=18.752 worst_q_ratio=1.977
ref2=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=0.376 worst_q_ratio=1.235
new1=fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits sigma_overall=0.549 worst_q_ratio=1.212
new2=fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits sigma_overall=0.539 worst_q_ratio=1.235
reference average sigma_overall=9.564 worst_q_ratio=1.606
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 (250 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 8.01 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 (975 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 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456_astrometric_residuals.png (969 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.52 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457_astrometric_residuals.png (971 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-19-48_20.00sec_5.00C_LIGHT_0456.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Cas-03-Q2b1x1_060604_TTUQ2b1x1_3926635_eMSIiiFZ/wcs_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:24.36 +60:39:45.4: 12.77 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.00 +59:15:34.1: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:24.36 +60:39:45.4: 11.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.01
Forced photometry filter REJECTED candidate at 01:33:24.36 +60:39:45.4: ref_mag=11.21 +/- 0.01 new_mean_mag=10.9451 delta=0.26 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.00 +59:15:34.1: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter KEPT candidate at 01:56:38.00 +59:15:34.1: ref_mag=9.75 +/- 0.00 new_mean_mag=8.7525 delta=1.00 (need > 0.90)
Adding exclusion_list_local.txt__out20109.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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 53064_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 53064_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
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Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 08339_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:33:41.86 +59:42:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247704_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247704_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247711_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247711_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247716_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247716_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247718_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247718_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247721_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247721_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:46:32.09 +57:52:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247724_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247724_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247725_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247725_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:09:23.49 +61:36:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247726_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247726_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247727_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247727_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247729_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247729_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247734_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247734_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247736_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247736_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247741_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247741_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247742_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247742_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247743_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247743_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247744_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247744_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247748_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247748_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247750_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247750_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247751_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247751_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247754_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247754_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:30:06.63 +61:51:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247757_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247757_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247760_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247760_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247762_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247762_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247767_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247767_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247768_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247768_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247769_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247769_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247771_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247771_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247774_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247774_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:33:01.82 +59:16:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247779_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247779_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:12:31.15 +61:17:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247780_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247780_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247782_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247782_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247783_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247783_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247784_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247784_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247787_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247787_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 247788_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247788_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247789_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247789_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247795_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247795_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247798_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247798_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247799_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247799_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247800_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247800_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247801_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247801_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:29:22.41 +63:18:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247804_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247804_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247805_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247805_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 247812_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247812_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247815_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247815_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247816_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247816_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:07:41.85 +60:54:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247823_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247823_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:00:46.23 +57:54:03.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247824_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247824_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247833_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247833_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247834_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247834_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247838_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247838_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247839_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247839_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247842_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247842_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247843_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247843_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247844_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247844_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247848_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247848_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247851_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247851_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247852_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247852_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247853_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247853_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247855_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247855_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247856_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247856_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247858_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247858_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:14:01.38 +57:40:45.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247862_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247862_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247863_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247863_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:07:34.97 +57:33:09.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247865_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247865_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247868_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247868_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:39:24.13 +58:23:05.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247869_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247869_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247873_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247873_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247874_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247874_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:09:09.04 +61:37:29.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247875_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247875_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:37:10.05 +58:51:06.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247883_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247883_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247885_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247885_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:44:27.94 +60:41:22.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247887_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247887_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247890_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247890_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247892_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247892_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247894_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247894_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:01:30.71 +65:05:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247896_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247896_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247898_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247898_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247899_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247899_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247904_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247904_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:32:22.02 +60:27:29.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247907_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247907_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247909_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247909_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:19:24.20 +58:26:39.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247910_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247910_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:07:34.09 +60:52:43.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247912_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247912_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:15:54.31 +64:24:53.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247918_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247918_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:25:15.48 +64:40:34.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247920_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247920_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:39:04.40 +61:53:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247924_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247924_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:14:45.24 +60:30:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247925_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247925_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247932_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247932_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:07:08.02 +57:44:35.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247935_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247935_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:25:26.58 +60:57:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247936_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247936_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:43:51.74 +61:53:59.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247938_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247938_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247939_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247939_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247941_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247941_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:43:59.18 +61:55:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247942_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247942_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:55:14.63 +59:32:02.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247943_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247943_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:16:20.67 +62:42:27.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247944_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247944_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247946_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247946_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:20:24.39 +59:10:24.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247948_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247948_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:19:48.76 +61:38:14.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247951_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247951_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247955_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247955_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:22:08.40 +60:22:45.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247956_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 247956_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:44:58.39 +57:57:47.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247958_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 247958_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248835_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 248835_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251456_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 251456_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:28:00.45 +61:19:58.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251472_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 251472_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:44:02.07 +61:53:57.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251938_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 251938_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:38:00.45 +57:56:45.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252105_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 252105_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:19:11.14 +58:20:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252977_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 252977_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:17:59.22 +57:47:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254066_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 254066_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:26:46.70 +57:46:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254171_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 254171_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 254233_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 254233_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:26:41.03 +60:46:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254251_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 254251_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:28:15.45 +58:44:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254721_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 254721_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:58:16.34 +59:38:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255618_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 255618_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:46:33.60 +61:16:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255726_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 255726_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:18:14.18 +61:44:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256646_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 256646_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:43:53.10 +61:53:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256838_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 256838_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:44:17.72 +61:53:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257147_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 257147_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:06:39.09 +64:09:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257335_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 257335_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:20:11.03 +58:12:09.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 257470_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 257470_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:21:28.04 +57:48:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257526_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 257526_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:33:59.42 +58:28:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257907_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 257907_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:16:08.75 +58:49:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257912_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 257912_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:11:22.95 +61:21:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258059_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 258059_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:00:36.74 +58:30:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258062_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 258062_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:44:32.35 +58:45:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258215_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 258215_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:13:30.51 +58:34:25.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 258316_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 258316_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:44:01.89 +61:52:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259005_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 259005_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:02:54.79 +64:24:59.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259249_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 259249_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:15:58.91 +63:12:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259306_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 259306_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:26:15.46 +60:37:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259667_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 259667_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:04:26.78 +65:05:52.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259669_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 259669_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:10:23.83 +60:01:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259735_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 259735_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:33:23.15 +57:44:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259796_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 259796_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
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Considering the candidate 259880_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 259880_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:08:30.64 +58:24:18.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 260142_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 260142_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 260145_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 260145_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:27:02.21 +58:03:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260307_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 260307_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:34:10.42 +62:09:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260645_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 260645_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:39:00.00 +61:11:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260673_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 260673_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:19:03.81 +63:57:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260713_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 260713_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:43:07.05 +58:57:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260737_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 260737_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:13:35.95 +57:52:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260748_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 260748_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:37:44.93 +64:45:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260761_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 260761_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:06:45.30 +59:50:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260878_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 260878_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:58:40.16 +59:15:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260933_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 260933_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:42:33.07 +63:52:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261025_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 261025_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:16:36.26 +64:57:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261076_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 261076_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:58:04.22 +57:58:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261281_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 261281_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:35:50.61 +61:27:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261313_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 261313_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:37:13.41 +58:38:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261333_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 261333_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:26:35.98 +57:57:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261722_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 261722_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 261723_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 261723_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:59:06.02 +59:55:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261741_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 261741_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:02:54.04 +60:15:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261781_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 261781_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:16:12.84 +62:42:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262002_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 262002_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:16:05.24 +58:49:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262350_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 262350_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:14:29.89 +63:16:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262469_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 262469_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:01:15.24 +59:23:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262663_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 262663_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 262714_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 262714_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:17:21.67 +59:22:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262741_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 262741_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 262902_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 262902_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 263004_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263004_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:06:23.52 +62:44:02.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263099_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263099_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:38:12.01 +61:01:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263174_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263174_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:43:12.86 +64:00:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263278_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263278_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:14:00.25 +61:42:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263300_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263300_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:38:07.78 +61:01:37.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263353_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263353_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:07:25.04 +57:54:58.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263380_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 263380_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263408_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263408_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:38:33.80 +60:47:23.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263437_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 263437_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263788_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263788_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:16:02.21 +58:50:00.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263836_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263836_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:02:50.46 +60:13:59.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263920_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263920_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:23:07.58 +61:11:24.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263938_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263938_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:44:56.76 +59:46:24.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263956_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263956_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:55:21.58 +59:25:59.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263957_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263957_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:48:39.87 +59:09:18.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263972_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 263972_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:18:04.28 +65:36:25.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264146_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 264146_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:55:52.91 +64:15:25.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264216_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 264216_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:42:28.41 +58:17:47.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264224_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 264224_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:56:15.97 +60:00:36.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264416_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 264416_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264433_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 264433_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:02:16.76 +62:49:58.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264467_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 264467_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:03:25.24 +57:50:13.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264484_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 264484_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:37:13.12 +58:38:18.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264589_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 264589_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:34:34.66 +65:48:56.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264619_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 264619_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:43:03.34 +58:57:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264662_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 264662_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264872_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 264872_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:35:07.82 +63:17:11.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264888_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 264888_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:52:48.75 +60:28:35.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264916_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 264916_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:46:18.49 +60:59:19.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265021_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 265021_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265075_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 265075_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:19:41.60 +62:51:05.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265246_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 265246_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:54:34.85 +59:52:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265248_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 265248_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265312_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 265312_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:42:26.70 +59:34:01.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265357_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 265357_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:54:06.22 +61:05:12.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265415_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 265415_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:16:37.33 +64:56:43.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265441_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 265441_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265468_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 265468_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:14:58.49 +60:30:24.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265494_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 265494_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:42:54.84 +64:01:47.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265495_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 265495_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265526_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 265526_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:21:29.03 +63:55:32.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265543_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 265543_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265557_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 265557_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265628_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 265628_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:38:06.53 +58:10:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265654_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 265654_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:55:22.07 +64:02:57.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265776_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 265776_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265864_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 265864_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:04:34.21 +58:32:27.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266213_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 266213_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266352_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 266352_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:31:29.05 +58:12:04.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266356_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 266356_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:16:02.58 +60:36:56.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266406_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 266406_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:14:21.75 +59:59:51.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266433_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 266433_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:08:33.13 +63:34:25.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266473_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 266473_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:37:41.62 +58:37:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266637_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 266637_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266682_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 266682_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:43:11.70 +60:34:29.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266683_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 266683_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266708_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 266708_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266759_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 266759_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266929_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 266929_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:33:46.89 +62:31:24.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267009_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 267009_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267031_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 267031_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:27:04.04 +64:43:35.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267051_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 267051_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267118_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 267118_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267209_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 267209_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:44:32.19 +61:36:37.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267386_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 267386_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267403_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 267403_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267599_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 267599_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:31:48.36 +64:21:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267623_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 267623_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:58:14.02 +60:03:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267834_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 267834_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:29:49.71 +58:44:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267845_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 267845_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 267896_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 267896_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267926_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 267926_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:14:00.70 +59:02:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268136_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 268136_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268167_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 268167_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:27:56.54 +62:46:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268212_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 268212_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268241_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 268241_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:20:50.43 +58:20:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268277_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 268277_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:37:55.38 +58:08:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268385_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 268385_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268405_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 268405_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:56:25.40 +62:05:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268430_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 268430_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:34:42.73 +58:42:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268435_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 268435_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 268445_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 268445_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 268483_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 268483_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 268525_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 268525_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268558_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 268558_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268634_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 268634_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:55:05.10 +59:57:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268662_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 268662_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:17:01.86 +63:21:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268889_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 268889_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:20:49.44 +64:40:20.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 268898_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 268898_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 269508_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 269508_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269593_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 269593_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269603_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 269603_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269696_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 269696_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 269761_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 269761_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:25:18.63 +62:14:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269832_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 269832_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:02:40.34 +59:57:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270036_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 270036_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 270234_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 270234_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:15:16.88 +59:21:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270388_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 270388_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 270427_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 270427_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 270441_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 270441_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 270473_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 270473_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 270512_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 270512_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 270590_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 270590_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:41:13.28 +62:53:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270615_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 270615_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:48:35.17 +58:41:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270869_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 270869_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:23:20.29 +62:03:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271202_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 271202_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:31:48.44 +64:22:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271266_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 271266_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:41:41.20 +57:56:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271321_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 271321_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 271491_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 271491_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 271519_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 271519_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 272052_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 272052_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 272151_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 272151_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 272304_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 272304_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 272550_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 272550_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 272802_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 272802_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:40:47.22 +65:05:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 273097_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 273097_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 273275_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 273275_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 273288_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 273288_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 273424_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 273424_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 273531_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 273531_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 274048_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 274048_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 274163_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 274163_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:48:21.36 +62:53:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 274798_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 274798_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 274837_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 274837_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 275366_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 275366_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 275563_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 275563_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 275766_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 275766_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 275816_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 275816_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 276120_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 276120_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 276719_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
Preparing report for the candidate 276719_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
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Considering the candidate 156692_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 156692_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:56:38.02 +59:15:34.1 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 70271_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:20:32.48 +62:32:01.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 112593_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:21:55.13 +61:20:57.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 72532_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:45:35.69 +63:07:02.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 233956_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 233956_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 02:18:51.98 +62:48:14.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457
The candidate 39378_fd_Cas-03-Q2b1x1_2026-06-23_05-20-39_20.00sec_4.90C_LIGHT_0457 did not pass the final checks
**** FOUND 01:47:55.70 +64:32:55.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 351s
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 ####
01:56:38.00 +59:15:34.1
01:34:23.32 +59:34:48.9
01:35:23.02 +60:03:01.8
01:32:08.93 +61:32:09.5
02:01:50.41 +63:28:16.8
01:11:16.45 +58:55:57.0
01:24:44.81 +63:34:15.9
01:34:22.91 +60:02:40.3
01:53:37.97 +64:44:09.9
01:12:01.02 +64:42:20.4
02:01:37.72 +64:49:01.8
01:30:01.21 +60:10:48.6
01:57:29.29 +60:09:18.3
01:32:10.95 +59:36:01.6
01:46:30.67 +66:08:35.0
01:15:32.65 +60:23:09.0
01:06:22.07 +62:13:32.0
02:03:59.16 +59:35:03.5
01:22:33.27 +60:44:41.8
02:00:21.96 +58:20:17.6
01:41:37.92 +60:05:55.2
01:06:17.15 +57:53:07.7
01:51:45.38 +58:37:51.6
01:26:37.88 +60:38:02.5
01:41:44.40 +64:14:44.1
01:13:19.49 +61:29:25.8
01:28:33.88 +62:13:51.8
01:30:00.83 +60:41:03.8
01:35:41.78 +61:13:11.8
01:12:41.27 +61:18:07.5
02:00:06.59 +59:00:32.1
01:33:08.71 +61:46:13.3
01:38:51.88 +59:27:14.9
01:29:48.14 +63:19:36.6
01:28:00.38 +61:23:58.1
01:28:07.26 +65:26:19.1
01:27:34.33 +57:48:25.8
01:21:45.41 +58:34:15.4
01:47:51.52 +61:11:12.3
01:24:54.97 +59:41:48.6
01:09:25.09 +64:35:19.3
01:07:39.07 +59:59:18.1
01:07:00.18 +61:28:29.6
01:36:49.12 +62:46:52.0
01:25:27.62 +59:27:15.4
01:40:18.28 +61:21:04.8
01:09:24.50 +58:01:47.9
01:40:10.62 +64:37:21.8
01:10:43.68 +60:59:19.2
01:13:27.25 +59:57:16.9
01:43:26.18 +58:38:20.1
01:29:02.62 +58:46:08.5
01:28:32.98 +61:12:19.4
01:35:27.50 +60:33:47.1
01:34:16.41 +60:57:35.2
01:11:50.59 +58:25:22.0
02:07:26.11 +59:18:26.5
01:26:36.86 +59:41:34.8
01:17:15.43 +58:35:37.4
01:29:42.06 +61:54:40.5
01:06:25.99 +61:41:31.6
01:22:28.43 +61:07:37.6
01:11:33.69 +62:10:04.4
01:20:45.20 +57:55:10.6
01:19:08.81 +60:33:58.7
01:31:30.69 +62:00:58.6
01:37:25.55 +63:41:28.2
01:35:24.90 +60:39:15.3
01:28:26.76 +60:23:27.4
01:30:43.78 +60:47:34.4
01:52:09.02 +58:27:40.5
01:19:35.43 +60:03:33.3
01:35:37.53 +61:16:49.4
01:23:31.46 +58:41:47.7
01:18:28.19 +58:11:23.1
01:24:45.35 +63:08:25.9
01:51:09.37 +64:52:46.3
01:46:23.30 +61:12:57.6
01:22:23.76 +61:13:50.9
01:36:16.35 +60:12:25.1
02:01:03.66 +64:43:34.0
02:15:10.56 +58:07:01.4
02:00:32.81 +59:40:06.4
01:06:55.55 +59:18:56.6
01:17:24.25 +57:40:30.3
01:13:39.02 +58:10:50.7
01:09:22.62 +57:26:31.0
01:38:04.13 +58:10:23.7
01:36:50.75 +59:55:48.5
01:26:05.59 +59:01:15.6
01:51:26.83 +57:51:35.5
02:16:40.51 +65:04:35.2
01:38:05.76 +61:04:13.9
01:07:29.62 +63:10:59.6
02:16:08.08 +58:18:13.4
01:56:57.31 +63:00:31.0
01:32:05.61 +61:59:26.9
01:28:13.20 +58:35:17.9
01:22:11.01 +59:09:03.3
02:15:04.06 +58:28:54.3
01:20:13.59 +65:31:28.2
01:44:03.40 +61:54:43.7
01:28:07.23 +59:53:49.6
01:08:59.21 +60:47:21.2
01:50:39.82 +62:00:55.6
01:57:46.60 +59:59:17.5
01:51:13.62 +59:13:47.9
01:51:05.54 +61:32:11.2
01:08:11.88 +62:14:21.0
01:27:14.37 +59:29:18.5
01:10:04.93 +60:32:46.6
02:02:32.31 +58:06:03.4
01:51:52.69 +60:27:42.8
02:10:20.55 +63:36:42.3
01:45:15.64 +59:38:17.5
01:44:31.82 +58:44:31.7
01:29:39.26 +63:18:45.7
01:52:55.21 +59:33:30.7
01:51:02.82 +59:06:43.0
02:01:06.65 +64:35:46.1
02:02:24.46 +64:38:24.6
01:19:28.88 +59:54:37.8
01:51:40.28 +60:56:17.5
01:19:08.05 +60:33:40.4
01:33:30.69 +58:02:22.8
02:13:18.57 +61:26:42.4
01:44:33.57 +60:39:30.2
01:26:28.36 +59:41:35.6
01:33:43.64 +59:31:30.7
01:58:11.48 +63:55:12.7
02:13:40.76 +65:08:14.4
01:21:24.18 +62:18:31.1
01:36:30.14 +60:46:39.5
01:35:34.09 +61:18:03.4
01:46:38.22 +60:09:00.0
01:37:08.39 +57:44:50.9
01:26:31.51 +62:18:32.6
01:27:06.73 +61:26:15.0
########### 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 ####
01:56:38.00 +59:15:34.1
01:34:23.32 +59:34:48.9
01:35:23.02 +60:03:01.8
01:32:08.93 +61:32:09.5
02:01:50.41 +63:28:16.8
01:11:16.45 +58:55:57.0
01:24:44.81 +63:34:15.9
01:34:22.91 +60:02:40.3
01:53:37.97 +64:44:09.9
01:12:01.02 +64:42:20.4
02:01:37.72 +64:49:01.8
01:30:01.21 +60:10:48.6
01:57:29.29 +60:09:18.3
01:32:10.95 +59:36:01.6
01:46:30.67 +66:08:35.0
01:15:32.65 +60:23:09.0
01:06:22.07 +62:13:32.0
02:03:59.16 +59:35:03.5
01:22:33.27 +60:44:41.8
02:00:21.96 +58:20:17.6
01:41:37.92 +60:05:55.2
01:06:17.15 +57:53:07.7
01:51:45.38 +58:37:51.6
01:26:37.88 +60:38:02.5
01:41:44.40 +64:14:44.1
01:13:19.49 +61:29:25.8
01:28:33.88 +62:13:51.8
01:30:00.83 +60:41:03.8
01:35:41.78 +61:13:11.8
01:12:41.27 +61:18:07.5
02:00:06.59 +59:00:32.1
01:33:08.71 +61:46:13.3
01:38:51.88 +59:27:14.9
01:29:48.14 +63:19:36.6
01:28:00.38 +61:23:58.1
01:28:07.26 +65:26:19.1
01:27:34.33 +57:48:25.8
01:21:45.41 +58:34:15.4
01:47:51.52 +61:11:12.3
01:24:54.97 +59:41:48.6
01:09:25.09 +64:35:19.3
01:07:39.07 +59:59:18.1
01:07:00.18 +61:28:29.6
01:36:49.12 +62:46:52.0
01:25:27.62 +59:27:15.4
01:40:18.28 +61:21:04.8
01:09:24.50 +58:01:47.9
01:40:10.62 +64:37:21.8
01:10:43.68 +60:59:19.2
01:13:27.25 +59:57:16.9
01:43:26.18 +58:38:20.1
01:29:02.62 +58:46:08.5
01:28:32.98 +61:12:19.4
01:35:27.50 +60:33:47.1
01:34:16.41 +60:57:35.2
01:11:50.59 +58:25:22.0
02:07:26.11 +59:18:26.5
01:26:36.86 +59:41:34.8
01:17:15.43 +58:35:37.4
01:29:42.06 +61:54:40.5
01:06:25.99 +61:41:31.6
01:22:28.43 +61:07:37.6
01:11:33.69 +62:10:04.4
01:20:45.20 +57:55:10.6
01:19:08.81 +60:33:58.7
01:31:30.69 +62:00:58.6
01:37:25.55 +63:41:28.2
01:35:24.90 +60:39:15.3
01:28:26.76 +60:23:27.4
01:30:43.78 +60:47:34.4
01:52:09.02 +58:27:40.5
01:19:35.43 +60:03:33.3
01:35:37.53 +61:16:49.4
01:23:31.46 +58:41:47.7
01:18:28.19 +58:11:23.1
01:24:45.35 +63:08:25.9
01:51:09.37 +64:52:46.3
01:46:23.30 +61:12:57.6
01:22:23.76 +61:13:50.9
01:36:16.35 +60:12:25.1
02:01:03.66 +64:43:34.0
02:15:10.56 +58:07:01.4
02:00:32.81 +59:40:06.4
01:06:55.55 +59:18:56.6
01:17:24.25 +57:40:30.3
01:13:39.02 +58:10:50.7
01:09:22.62 +57:26:31.0
01:38:04.13 +58:10:23.7
01:36:50.75 +59:55:48.5
01:26:05.59 +59:01:15.6
01:51:26.83 +57:51:35.5
02:16:40.51 +65:04:35.2
01:38:05.76 +61:04:13.9
01:07:29.62 +63:10:59.6
02:16:08.08 +58:18:13.4
01:56:57.31 +63:00:31.0
01:32:05.61 +61:59:26.9
01:28:13.20 +58:35:17.9
01:22:11.01 +59:09:03.3
02:15:04.06 +58:28:54.3
01:20:13.59 +65:31:28.2
01:44:03.40 +61:54:43.7
01:28:07.23 +59:53:49.6
01:08:59.21 +60:47:21.2
01:50:39.82 +62:00:55.6
01:57:46.60 +59:59:17.5
01:51:13.62 +59:13:47.9
01:51:05.54 +61:32:11.2
01:08:11.88 +62:14:21.0
01:27:14.37 +59:29:18.5
01:10:04.93 +60:32:46.6
02:02:32.31 +58:06:03.4
01:51:52.69 +60:27:42.8
02:10:20.55 +63:36:42.3
01:45:15.64 +59:38:17.5
01:44:31.82 +58:44:31.7
01:29:39.26 +63:18:45.7
01:52:55.21 +59:33:30.7
01:51:02.82 +59:06:43.0
02:01:06.65 +64:35:46.1
02:02:24.46 +64:38:24.6
01:19:28.88 +59:54:37.8
01:51:40.28 +60:56:17.5
01:19:08.05 +60:33:40.4
01:33:30.69 +58:02:22.8
02:13:18.57 +61:26:42.4
01:44:33.57 +60:39:30.2
01:26:28.36 +59:41:35.6
01:33:43.64 +59:31:30.7
01:58:11.48 +63:55:12.7
02:13:40.76 +65:08:14.4
01:21:24.18 +62:18:31.1
01:36:30.14 +60:46:39.5
01:35:34.09 +61:18:03.4
01:46:38.22 +60:09:00.0
01:37:08.39 +57:44:50.9
01:26:31.51 +62:18:32.6
01:27:06.73 +61:26:15.0
###################################################################################
01:56:38.00 +59:15:34.1 -- not an asteroid (will add it to exclusion list)
01:34:23.32 +59:34:48.9 -- not an asteroid (will add it to exclusion list)
01:35:23.02 +60:03:01.8 -- not an asteroid (will add it to exclusion list)
01:32:08.93 +61:32:09.5 -- not an asteroid (will add it to exclusion list)
02:01:50.41 +63:28:16.8 -- not an asteroid (will add it to exclusion list)
01:11:16.45 +58:55:57.0 -- not an asteroid (will add it to exclusion list)
01:24:44.81 +63:34:15.9 -- not an asteroid (will add it to exclusion list)
01:34:22.91 +60:02:40.3 -- not an asteroid (will add it to exclusion list)
01:53:37.97 +64:44:09.9 -- not an asteroid (will add it to exclusion list)
01:12:01.02 +64:42:20.4 -- not an asteroid (will add it to exclusion list)
02:01:37.72 +64:49:01.8 -- not an asteroid (will add it to exclusion list)
01:30:01.21 +60:10:48.6 -- not an asteroid (will add it to exclusion list)
01:57:29.29 +60:09:18.3 -- not an asteroid (will add it to exclusion list)
01:32:10.95 +59:36:01.6 -- not an asteroid (will add it to exclusion list)
01:46:30.67 +66:08:35.0 -- not an asteroid (will add it to exclusion list)
01:15:32.65 +60:23:09.0 -- not an asteroid (will add it to exclusion list)
01:06:22.07 +62:13:32.0 -- not an asteroid (will add it to exclusion list)
02:03:59.16 +59:35:03.5 -- not an asteroid (will add it to exclusion list)
01:22:33.27 +60:44:41.8 -- not an asteroid (will add it to exclusion list)
02:00:21.96 +58:20:17.6 -- not an asteroid (will add it to exclusion list)
01:41:37.92 +60:05:55.2 -- not an asteroid (will add it to exclusion list)
01:06:17.15 +57:53:07.7 -- not an asteroid (will add it to exclusion list)
01:51:45.38 +58:37:51.6 -- not an asteroid (will add it to exclusion list)
01:26:37.88 +60:38:02.5 -- not an asteroid (will add it to exclusion list)
01:41:44.40 +64:14:44.1 -- not an asteroid (will add it to exclusion list)
01:13:19.49 +61:29:25.8 -- not an asteroid (will add it to exclusion list)
01:28:33.88 +62:13:51.8 -- not an asteroid (will add it to exclusion list)
01:30:00.83 +60:41:03.8 -- not an asteroid (will add it to exclusion list)
01:35:41.78 +61:13:11.8 -- not an asteroid (will add it to exclusion list)
01:12:41.27 +61:18:07.5 -- not an asteroid (will add it to exclusion list)
02:00:06.59 +59:00:32.1 -- not an asteroid (will add it to exclusion list)
01:33:08.71 +61:46:13.3 -- not an asteroid (will add it to exclusion list)
01:38:51.88 +59:27:14.9 -- not an asteroid (will add it to exclusion list)
01:29:48.14 +63:19:36.6 -- not an asteroid (will add it to exclusion list)
01:28:00.38 +61:23:58.1 -- not an asteroid (will add it to exclusion list)
01:28:07.26 +65:26:19.1 -- not an asteroid (will add it to exclusion list)
01:27:34.33 +57:48:25.8 -- not an asteroid (will add it to exclusion list)
01:21:45.41 +58:34:15.4 -- not an asteroid (will add it to exclusion list)
01:47:51.52 +61:11:12.3 -- not an asteroid (will add it to exclusion list)
01:24:54.97 +59:41:48.6 -- not an asteroid (will add it to exclusion list)
01:09:25.09 +64:35:19.3 -- not an asteroid (will add it to exclusion list)
01:07:39.07 +59:59:18.1 -- not an asteroid (will add it to exclusion list)
01:07:00.18 +61:28:29.6 -- not an asteroid (will add it to exclusion list)
01:36:49.12 +62:46:52.0 -- not an asteroid (will add it to exclusion list)
01:25:27.62 +59:27:15.4 -- not an asteroid (will add it to exclusion list)
01:40:18.28 +61:21:04.8 -- not an asteroid (will add it to exclusion list)
01:09:24.50 +58:01:47.9 -- not an asteroid (will add it to exclusion list)
01:40:10.62 +64:37:21.8 -- not an asteroid (will add it to exclusion list)
01:10:43.68 +60:59:19.2 -- not an asteroid (will add it to exclusion list)
01:13:27.25 +59:57:16.9 -- not an asteroid (will add it to exclusion list)
01:43:26.18 +58:38:20.1 -- not an asteroid (will add it to exclusion list)
01:29:02.62 +58:46:08.5 -- not an asteroid (will add it to exclusion list)
01:28:32.98 +61:12:19.4 -- not an asteroid (will add it to exclusion list)
01:35:27.50 +60:33:47.1 -- not an asteroid (will add it to exclusion list)
01:34:16.41 +60:57:35.2 -- not an asteroid (will add it to exclusion list)
01:11:50.59 +58:25:22.0 -- not an asteroid (will add it to exclusion list)
02:07:26.11 +59:18:26.5 -- not an asteroid (will add it to exclusion list)
01:26:36.86 +59:41:34.8 -- not an asteroid (will add it to exclusion list)
01:17:15.43 +58:35:37.4 -- not an asteroid (will add it to exclusion list)
01:29:42.06 +61:54:40.5 -- not an asteroid (will add it to exclusion list)
01:06:25.99 +61:41:31.6 -- not an asteroid (will add it to exclusion list)
01:22:28.43 +61:07:37.6 -- not an asteroid (will add it to exclusion list)
01:11:33.69 +62:10:04.4 -- not an asteroid (will add it to exclusion list)
01:20:45.20 +57:55:10.6 -- not an asteroid (will add it to exclusion list)
01:19:08.81 +60:33:58.7 -- not an asteroid (will add it to exclusion list)
01:31:30.69 +62:00:58.6 -- not an asteroid (will add it to exclusion list)
01:37:25.55 +63:41:28.2 -- not an asteroid (will add it to exclusion list)
01:35:24.90 +60:39:15.3 -- not an asteroid (will add it to exclusion list)
01:28:26.76 +60:23:27.4 -- not an asteroid (will add it to exclusion list)
01:30:43.78 +60:47:34.4 -- not an asteroid (will add it to exclusion list)
01:52:09.02 +58:27:40.5 -- not an asteroid (will add it to exclusion list)
01:19:35.43 +60:03:33.3 -- not an asteroid (will add it to exclusion list)
01:35:37.53 +61:16:49.4 -- not an asteroid (will add it to exclusion list)
01:23:31.46 +58:41:47.7 -- not an asteroid (will add it to exclusion list)
01:18:28.19 +58:11:23.1 -- not an asteroid (will add it to exclusion list)
01:24:45.35 +63:08:25.9 -- not an asteroid (will add it to exclusion list)
01:51:09.37 +64:52:46.3 -- not an asteroid (will add it to exclusion list)
01:46:23.30 +61:12:57.6 -- not an asteroid (will add it to exclusion list)
01:22:23.76 +61:13:50.9 -- not an asteroid (will add it to exclusion list)
01:36:16.35 +60:12:25.1 -- not an asteroid (will add it to exclusion list)
02:01:03.66 +64:43:34.0 -- not an asteroid (will add it to exclusion list)
02:15:10.56 +58:07:01.4 -- not an asteroid (will add it to exclusion list)
02:00:32.81 +59:40:06.4 -- not an asteroid (will add it to exclusion list)
01:06:55.55 +59:18:56.6 -- not an asteroid (will add it to exclusion list)
01:17:24.25 +57:40:30.3 -- not an asteroid (will add it to exclusion list)
01:13:39.02 +58:10:50.7 -- not an asteroid (will add it to exclusion list)
01:09:22.62 +57:26:31.0 -- not an asteroid (will add it to exclusion list)
01:38:04.13 +58:10:23.7 -- not an asteroid (will add it to exclusion list)
01:36:50.75 +59:55:48.5 -- not an asteroid (will add it to exclusion list)
01:26:05.59 +59:01:15.6 -- not an asteroid (will add it to exclusion list)
01:51:26.83 +57:51:35.5 -- not an asteroid (will add it to exclusion list)
02:16:40.51 +65:04:35.2 -- not an asteroid (will add it to exclusion list)
01:38:05.76 +61:04:13.9 -- not an asteroid (will add it to exclusion list)
01:07:29.62 +63:10:59.6 -- not an asteroid (will add it to exclusion list)
02:16:08.08 +58:18:13.4 -- not an asteroid (will add it to exclusion list)
01:56:57.31 +63:00:31.0 -- not an asteroid (will add it to exclusion list)
01:32:05.61 +61:59:26.9 -- not an asteroid (will add it to exclusion list)
01:28:13.20 +58:35:17.9 -- not an asteroid (will add it to exclusion list)
01:22:11.01 +59:09:03.3 -- not an asteroid (will add it to exclusion list)
02:15:04.06 +58:28:54.3 -- not an asteroid (will add it to exclusion list)
01:20:13.59 +65:31:28.2 -- not an asteroid (will add it to exclusion list)
01:44:03.40 +61:54:43.7 -- not an asteroid (will add it to exclusion list)
01:28:07.23 +59:53:49.6 -- not an asteroid (will add it to exclusion list)
01:08:59.21 +60:47:21.2 -- not an asteroid (will add it to exclusion list)
01:50:39.82 +62:00:55.6 -- not an asteroid (will add it to exclusion list)
01:57:46.60 +59:59:17.5 -- not an asteroid (will add it to exclusion list)
01:51:13.62 +59:13:47.9 -- not an asteroid (will add it to exclusion list)
01:51:05.54 +61:32:11.2 -- not an asteroid (will add it to exclusion list)
01:08:11.88 +62:14:21.0 -- not an asteroid (will add it to exclusion list)
01:27:14.37 +59:29:18.5 -- not an asteroid (will add it to exclusion list)
01:10:04.93 +60:32:46.6 -- not an asteroid (will add it to exclusion list)
02:02:32.31 +58:06:03.4 -- not an asteroid (will add it to exclusion list)
01:51:52.69 +60:27:42.8 -- not an asteroid (will add it to exclusion list)
02:10:20.55 +63:36:42.3 -- not an asteroid (will add it to exclusion list)
01:45:15.64 +59:38:17.5 -- not an asteroid (will add it to exclusion list)
01:44:31.82 +58:44:31.7 -- not an asteroid (will add it to exclusion list)
01:29:39.26 +63:18:45.7 -- not an asteroid (will add it to exclusion list)
01:52:55.21 +59:33:30.7 -- not an asteroid (will add it to exclusion list)
01:51:02.82 +59:06:43.0 -- not an asteroid (will add it to exclusion list)
02:01:06.65 +64:35:46.1 -- not an asteroid (will add it to exclusion list)
02:02:24.46 +64:38:24.6 -- not an asteroid (will add it to exclusion list)
01:19:28.88 +59:54:37.8 -- not an asteroid (will add it to exclusion list)
01:51:40.28 +60:56:17.5 -- not an asteroid (will add it to exclusion list)
01:19:08.05 +60:33:40.4 -- not an asteroid (will add it to exclusion list)
01:33:30.69 +58:02:22.8 -- not an asteroid (will add it to exclusion list)
02:13:18.57 +61:26:42.4 -- not an asteroid (will add it to exclusion list)
01:44:33.57 +60:39:30.2 -- not an asteroid (will add it to exclusion list)
01:26:28.36 +59:41:35.6 -- not an asteroid (will add it to exclusion list)
01:33:43.64 +59:31:30.7 -- not an asteroid (will add it to exclusion list)
01:58:11.48 +63:55:12.7 -- not an asteroid (will add it to exclusion list)
02:13:40.76 +65:08:14.4 -- not an asteroid (will add it to exclusion list)
01:21:24.18 +62:18:31.1 -- not an asteroid (will add it to exclusion list)
01:36:30.14 +60:46:39.5 -- not an asteroid (will add it to exclusion list)
01:35:34.09 +61:18:03.4 -- not an asteroid (will add it to exclusion list)
01:46:38.22 +60:09:00.0 -- not an asteroid (will add it to exclusion list)
01:37:08.39 +57:44:50.9 -- not an asteroid (will add it to exclusion list)
01:26:31.51 +62:18:32.6 -- not an asteroid (will add it to exclusion list)
01:27:06.73 +61:26:15.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:06:17.15 +57:53:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:22.07 +62:13:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:25.99 +61:41:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:55.55 +59:18:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:00.18 +61:28:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:29.62 +63:10:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.07 +59:59:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:11.88 +62:14:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:59.21 +60:47:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:22.62 +57:26:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:24.50 +58:01:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:25.09 +64:35:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:04.93 +60:32:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:43.68 +60:59:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:16.45 +58:55:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:33.69 +62:10:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:50.59 +58:25:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:01.02 +64:42:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:41.27 +61:18:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:19.49 +61:29:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:27.25 +59:57:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:39.02 +58:10:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:32.65 +60:23:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:15.43 +58:35:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:24.25 +57:40:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:28.19 +58:11:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:08.05 +60:33:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:08.81 +60:33:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:28.88 +59:54:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:35.43 +60:03:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:13.59 +65:31:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:45.20 +57:55:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:24.18 +62:18:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:45.41 +58:34:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:11.01 +59:09:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:23.76 +61:13:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:28.43 +61:07:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:33.27 +60:44:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:31.46 +58:41:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:44.81 +63:34:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:45.35 +63:08:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:54.97 +59:41:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:27.62 +59:27:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:05.59 +59:01:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:28.36 +59:41:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:31.51 +62:18:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:36.86 +59:41:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:37.88 +60:38:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:06.73 +61:26:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:14.37 +59:29:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:34.33 +57:48:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:00.38 +61:23:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:07.23 +59:53:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:07.26 +65:26:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:13.20 +58:35:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:26.76 +60:23:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:32.98 +61:12:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:33.88 +62:13:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:02.62 +58:46:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:39.26 +63:18:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:42.06 +61:54:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:48.14 +63:19:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:00.83 +60:41:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:01.21 +60:10:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:43.78 +60:47:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:30.69 +62:00:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:05.61 +61:59:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:08.93 +61:32:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:10.95 +59:36:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:08.71 +61:46:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:30.69 +58:02:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:43.64 +59:31:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:16.41 +60:57:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:22.91 +60:02:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:23.32 +59:34:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:23.02 +60:03:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:24.90 +60:39:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:27.50 +60:33:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:34.09 +61:18:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:37.53 +61:16:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:41.78 +61:13:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:16.35 +60:12:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:30.14 +60:46:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:49.12 +62:46:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:50.75 +59:55:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:08.39 +57:44:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:25.55 +63:41:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:04.13 +58:10:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:05.76 +61:04:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:51.88 +59:27:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:10.62 +64:37:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:18.28 +61:21:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:37.92 +60:05:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:44.40 +64:14:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:26.18 +58:38:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:03.40 +61:54:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:31.82 +58:44:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:33.57 +60:39:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:15.64 +59:38:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:23.30 +61:12:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:30.67 +66:08:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.22 +60:09:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:51.52 +61:11:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:39.82 +62:00:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:02.82 +59:06:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:05.54 +61:32:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:09.37 +64:52:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:13.62 +59:13:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:26.83 +57:51:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:40.28 +60:56:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:45.38 +58:37:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:52.69 +60:27:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:09.02 +58:27:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:55.21 +59:33:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:37.97 +64:44:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:38.00 +59:15:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:57.31 +63:00:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:29.29 +60:09:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:46.60 +59:59:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:11.48 +63:55:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:06.59 +59:00:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:21.96 +58:20:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:32.81 +59:40:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:03.66 +64:43:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:06.65 +64:35:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:37.72 +64:49:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:50.41 +63:28:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:24.46 +64:38:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:32.31 +58:06:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:59.16 +59:35:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:26.11 +59:18:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:20.55 +63:36:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:18.57 +61:26:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:40.76 +65:08:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:04.06 +58:28:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:10.56 +58:07:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:08.08 +58:18:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:40.51 +65:04:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:06:17.15 +57:53:07.7 -- not a known variable star
01:06:22.07 +62:13:32.0 -- not a known variable star
01:06:25.99 +61:41:31.6 -- not a known variable star
01:06:55.55 +59:18:56.6 -- not a known variable star
01:07:00.18 +61:28:29.6 -- a known variable star
01:07:29.62 +63:10:59.6 -- not a known variable star
01:07:39.07 +59:59:18.1 -- not a known variable star
01:08:11.88 +62:14:21.0 -- a known variable star
01:08:59.21 +60:47:21.2 -- not a known variable star
01:09:22.62 +57:26:31.0 -- not a known variable star
01:09:24.50 +58:01:47.9 -- not a known variable star
01:09:25.09 +64:35:19.3 -- not a known variable star
01:10:04.93 +60:32:46.6 -- not a known variable star
01:10:43.68 +60:59:19.2 -- not a known variable star
01:11:16.45 +58:55:57.0 -- not a known variable star
01:11:33.69 +62:10:04.4 -- not a known variable star
01:11:50.59 +58:25:22.0 -- not a known variable star
01:12:01.02 +64:42:20.4 -- a known variable star
01:12:41.27 +61:18:07.5 -- not a known variable star
01:13:19.49 +61:29:25.8 -- a known variable star
01:13:27.25 +59:57:16.9 -- not a known variable star
01:13:39.02 +58:10:50.7 -- not a known variable star
01:15:32.65 +60:23:09.0 -- not a known variable star
01:17:15.43 +58:35:37.4 -- not a known variable star
01:17:24.25 +57:40:30.3 -- a known variable star
01:18:28.19 +58:11:23.1 -- not a known variable star
01:19:08.05 +60:33:40.4 -- not a known variable star
01:19:08.81 +60:33:58.7 -- not a known variable star
01:19:28.88 +59:54:37.8 -- not a known variable star
01:19:35.43 +60:03:33.3 -- not a known variable star
01:20:13.59 +65:31:28.2 -- a known variable star
01:20:45.20 +57:55:10.6 -- not a known variable star
01:21:24.18 +62:18:31.1 -- not a known variable star
01:21:45.41 +58:34:15.4 -- a known variable star
01:22:11.01 +59:09:03.3 -- not a known variable star
01:22:23.76 +61:13:50.9 -- a known variable star
01:22:28.43 +61:07:37.6 -- a known variable star
01:22:33.27 +60:44:41.8 -- not a known variable star
01:23:31.46 +58:41:47.7 -- a known variable star
01:24:44.81 +63:34:15.9 -- not a known variable star
01:24:45.35 +63:08:25.9 -- not a known variable star
01:24:54.97 +59:41:48.6 -- not a known variable star
01:25:27.62 +59:27:15.4 -- a known variable star
01:26:05.59 +59:01:15.6 -- not a known variable star
01:26:28.36 +59:41:35.6 -- not a known variable star
01:26:31.51 +62:18:32.6 -- not a known variable star
01:26:36.86 +59:41:34.8 -- a known variable star
01:26:37.88 +60:38:02.5 -- not a known variable star
01:27:06.73 +61:26:15.0 -- not a known variable star
01:27:14.37 +59:29:18.5 -- not a known variable star
01:27:34.33 +57:48:25.8 -- not a known variable star
01:28:00.38 +61:23:58.1 -- not a known variable star
01:28:07.23 +59:53:49.6 -- not a known variable star
01:28:07.26 +65:26:19.1 -- a known variable star
01:28:13.20 +58:35:17.9 -- not a known variable star
01:28:26.76 +60:23:27.4 -- not a known variable star
01:28:32.98 +61:12:19.4 -- not a known variable star
01:28:33.88 +62:13:51.8 -- not a known variable star
01:29:02.62 +58:46:08.5 -- not a known variable star
01:29:39.26 +63:18:45.7 -- not a known variable star
01:29:42.06 +61:54:40.5 -- not a known variable star
01:29:48.14 +63:19:36.6 -- not a known variable star
01:30:00.83 +60:41:03.8 -- a known variable star
01:30:01.21 +60:10:48.6 -- a known variable star
01:30:43.78 +60:47:34.4 -- a known variable star
01:31:30.69 +62:00:58.6 -- not a known variable star
01:32:05.61 +61:59:26.9 -- not a known variable star
01:32:08.93 +61:32:09.5 -- not a known variable star
01:32:10.95 +59:36:01.6 -- not a known variable star
01:33:08.71 +61:46:13.3 -- not a known variable star
01:33:30.69 +58:02:22.8 -- not a known variable star
01:33:43.64 +59:31:30.7 -- not a known variable star
01:34:16.41 +60:57:35.2 -- not a known variable star
01:34:22.91 +60:02:40.3 -- not a known variable star
01:34:23.32 +59:34:48.9 -- a known variable star
01:35:23.02 +60:03:01.8 -- not a known variable star
01:35:24.90 +60:39:15.3 -- a known variable star
01:35:27.50 +60:33:47.1 -- not a known variable star
01:35:34.09 +61:18:03.4 -- a known variable star
01:35:37.53 +61:16:49.4 -- a known variable star
01:35:41.78 +61:13:11.8 -- not a known variable star
01:36:16.35 +60:12:25.1 -- not a known variable star
01:36:30.14 +60:46:39.5 -- a known variable star
01:36:49.12 +62:46:52.0 -- a known variable star
01:36:50.75 +59:55:48.5 -- a known variable star
01:37:08.39 +57:44:50.9 -- a known variable star
01:37:25.55 +63:41:28.2 -- a known variable star
01:38:04.13 +58:10:23.7 -- a known variable star
01:38:05.76 +61:04:13.9 -- not a known variable star
01:38:51.88 +59:27:14.9 -- not a known variable star
01:40:10.62 +64:37:21.8 -- not a known variable star
01:40:18.28 +61:21:04.8 -- not a known variable star
01:41:37.92 +60:05:55.2 -- not a known variable star
01:41:44.40 +64:14:44.1 -- not a known variable star
01:43:26.18 +58:38:20.1 -- a known variable star
01:44:03.40 +61:54:43.7 -- not a known variable star
01:44:31.82 +58:44:31.7 -- a known variable star
01:44:33.57 +60:39:30.2 -- a known variable star
01:45:15.64 +59:38:17.5 -- a known variable star
01:46:23.30 +61:12:57.6 -- a known variable star
01:46:30.67 +66:08:35.0 -- not a known variable star
01:46:38.22 +60:09:00.0 -- not a known variable star
01:47:51.52 +61:11:12.3 -- not a known variable star
01:50:39.82 +62:00:55.6 -- not a known variable star
01:51:02.82 +59:06:43.0 -- not a known variable star
01:51:05.54 +61:32:11.2 -- not a known variable star
01:51:09.37 +64:52:46.3 -- a known variable star
01:51:13.62 +59:13:47.9 -- not a known variable star
01:51:26.83 +57:51:35.5 -- not a known variable star
01:51:40.28 +60:56:17.5 -- not a known variable star
01:51:45.38 +58:37:51.6 -- not a known variable star
01:51:52.69 +60:27:42.8 -- not a known variable star
01:52:09.02 +58:27:40.5 -- not a known variable star
01:52:55.21 +59:33:30.7 -- a known variable star
01:53:37.97 +64:44:09.9 -- a known variable star
01:56:38.00 +59:15:34.1 -- a known variable star
01:56:57.31 +63:00:31.0 -- not a known variable star
01:57:29.29 +60:09:18.3 -- not a known variable star
01:57:46.60 +59:59:17.5 -- not a known variable star
01:58:11.48 +63:55:12.7 -- not a known variable star
02:00:06.59 +59:00:32.1 -- not a known variable star
02:00:21.96 +58:20:17.6 -- not a known variable star
02:00:32.81 +59:40:06.4 -- a known variable star
02:01:03.66 +64:43:34.0 -- not a known variable star
02:01:06.65 +64:35:46.1 -- not a known variable star
02:01:37.72 +64:49:01.8 -- a known variable star
02:01:50.41 +63:28:16.8 -- not a known variable star
02:02:24.46 +64:38:24.6 -- a known variable star
02:02:32.31 +58:06:03.4 -- not a known variable star
02:03:59.16 +59:35:03.5 -- not a known variable star
02:07:26.11 +59:18:26.5 -- a known variable star
02:10:20.55 +63:36:42.3 -- not a known variable star
02:13:18.57 +61:26:42.4 -- not a known variable star
02:13:40.76 +65:08:14.4 -- not a known variable star
02:15:04.06 +58:28:54.3 -- a known variable star
02:15:10.56 +58:07:01.4 -- not a known variable star
02:16:08.08 +58:18:13.4 -- a known variable star
02:16:40.51 +65:04:35.2 -- a known variable star
Found 96 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
138 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 138 (excluding asteroids and hot pixels, 96 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)2461214.93053812 -observatory V36
07:44:42.40 +20:41:35.0 Mercury (1.1mag)
08:56:48.91 +19:17:40.5 Venus (-4.0mag)
03:34:10.43 +18:49:15.1 Mars (1.3mag)
08:01:30.99 +20:56:39.1 Jupiter (-1.8mag)
00:53:08.60 +03:08:25.1 Saturn (0.8mag)
04:03:43.31 +20:35:24.9 Uranus (5.8mag)
00:16:48.89 +00:20:18.2 Neptune (7.8mag)
20:32:20.84 -23:10:39.4 Pluto (14.5mag)
13:02:34.13 -11:23:48.0 Moon (-10.8mag)
-rw-r--r-- 1 apache apache 362 Jun 23 06:13 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461214.93053812:
08:01:28.33 +20:56:47.1 Io (6.1mag)
08:01:42.57 +20:56:00.7 Europa (6.3mag)
08:01:19.24 +20:57:21.7 Ganymede (5.6mag)
08:01:59.83 +20:55:03.1 Callisto (6.9mag)
08:00:54.92 +20:35:17.0 Himalia (15.6mag)
08:01:29.16 +20:56:46.6 Thebe (16.6mag)
08:00:30.31 +20:44:37.8 Elara (17.6mag)
08:04:25.18 +21:00:00.8 Pasiphae (17.8mag)
08:07:23.14 +20:59:41.5 Carme (18.9mag)
00:52:57.51 +03:08:29.6 Titan (8.6mag)
00:53:09.06 +03:08:14.4 Rhea (9.9mag)
00:53:15.16 +03:10:31.8 Iapetus (11.3mag)
00:52:59.53 +03:08:50.5 Hyperion (14.6mag)
00:53:31.63 +03:08:08.3 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jun 23 06:13 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461214.93053812:
17:29:42.67 -35:19:14.4 JWST
19:32:12.19 -02:30:09.0 Chandra
10:18:01.58 -57:34:47.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 23 06:13 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461214.93053812 -observatory V36
18:31:47.14 -33:38:43.1 13.7mag P/2010 H2 (Vales)
06:08:39.44 -67:59:46.9 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:54:42.03 +32:10:46.6 17.6mag C/2017 K2 (PANSTARRS)
17:08:45.72 +15:54:22.6 17.9mag C/2021 G2 (ATLAS)
23:42:53.57 -29:54:44.0 15.7mag P/2021 N1 (ZTF)
23:07:56.01 +32:04:29.7 17.2mag C/2022 E2 (ATLAS)
05:52:32.78 +27:00:38.2 16.6mag C/2022 N2 (PANSTARRS)
09:41:20.67 +30:30:17.2 16.7mag C/2022 QE78 (ATLAS)
08:59:12.26 +04:33:06.1 17.8mag C/2022 R6 (PANSTARRS)
18:18:07.00 +21:41:08.1 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:14:39.25 -11:06:12.0 17.6mag P/2023 B1 (PANSTARRS)
22:06:02.82 +67:18:28.4 17.8mag C/2023 H5 (Lemmon)
17:08:37.94 -08:16:04.0 13.7mag C/2023 R1 (PANSTARRS)
13:18:48.94 +79:23:26.9 18.0mag C/2023 X2 (Lemmon)
07:32:52.22 +64:53:34.4 17.8mag C/2024 A1 (ATLAS)
07:09:40.39 +29:00:59.0 14.1mag C/2024 E1 (Wierzchos)
15:26:09.50 +14:37:30.0 17.5mag C/2024 G6 (ATLAS)
20:00:30.11 +35:26:48.2 13.9mag C/2024 J3 (ATLAS)
22:01:54.09 +43:10:35.8 18.0mag C/2024 R4 (PANSTARRS)
04:33:13.71 -14:45:46.1 15.9mag C/2024 T5 (ATLAS)
06:19:53.97 +31:53:34.1 17.9mag C/2025 J1 (Borisov)
11:32:12.08 +51:48:42.7 17.9mag C/2025 L1 (ATLAS)
07:00:50.11 -11:39:04.6 15.4mag C/2025 R3 (PANSTARRS)
09:37:56.75 +23:01:44.2 17.8mag C/2025 V2 (Rankin)
12:40:36.47 +04:29:25.2 17.1mag C/2025 Y1 (ATLAS)
17:40:32.53 +77:48:54.8 17.6mag C/2026 A2 (Bok)
02:24:55.75 +44:23:24.1 16.4mag C/2026 B2 (Sun-Gao)
11:16:20.02 +00:53:02.5 16.7mag A/2026 E1
20:50:45.86 -10:30:06.3 8.0mag 10P/Tempel
11:06:30.00 -01:17:26.6 16.1mag 29P/Schwassmann-Wachmann
03:35:04.94 +27:35:48.1 17.8mag 47P/Ashbrook-Jackson
09:32:25.68 +19:16:41.1 16.9mag 63P/Wild
00:38:44.32 -05:33:23.8 15.6mag 65P/Gunn
07:32:57.02 +34:23:58.7 17.3mag 76P/West-Kohoutek-Ikemura
03:46:12.57 +18:55:06.6 13.8mag 78P/Gehrels
01:52:05.33 +07:53:31.5 15.9mag 88P/Howell
05:43:22.98 +30:56:52.2 15.4mag 93P/Lovas
03:27:43.06 +29:44:40.1 17.2mag 114P/Wiseman-Skiff
07:27:19.77 +32:13:41.0 15.4mag 123P/West-Hartley
10:17:09.43 +08:10:51.6 16.6mag 124P/Mrkos
04:24:09.60 +20:08:27.9 16.3mag 128P/Shoemaker-Holt
05:03:39.66 +19:35:40.3 17.8mag 131P/Mueller
06:58:50.98 +16:25:17.4 16.6mag 141P/Machholz
07:02:46.20 +17:47:49.4 16.5mag 141P-A/Machholz
06:06:59.85 +17:24:09.3 13.4mag 141P-D/Machholz
03:07:49.17 -22:46:48.3 16.2mag 161P/Hartley-IRAS
04:33:04.19 +29:20:48.3 15.1mag 162P/SidingSpring
19:30:17.54 +06:53:25.5 16.0mag 169P/NEAT
00:58:40.07 +05:13:25.0 17.8mag 220P/McNaught
16:41:57.23 -08:04:34.1 16.7mag 235P/LINEAR
08:08:43.45 +34:39:13.9 17.7mag 240P/NEAT
01:12:51.23 +04:14:48.5 16.0mag 260P/McNaught
04:46:59.95 +34:56:46.7 17.5mag 295P/LINEAR
15:09:34.10 +07:21:01.0 17.5mag 391P/Kowalski
08:19:44.81 +20:17:54.7 17.9mag 450P/LONEOS
07:24:44.89 +40:34:08.8 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 23 06:13 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 23 06:13 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 23 06:13 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:12:56.050 -00:47:40.71 AT 2026pft 2026-06-02.72 20.75
14:00:08.000 -00:22:03.52 AT 2026pfs 2026-06-02.72 21.39
13:48:40.890 +01:37:22.75 AT 2026pfr 2026-06-02.72 20.72
13:49:23.100 -00:28:17.60 AT 2026pfq 2026-06-02.71 21.6
13:40:58.320 -00:10:56.98 AT 2026pfp 2026-06-02.71 20.87
13:30:45.650 +03:46:42.75 AT 2026pfo 2026-06-02.71 21.48
13:09:47.460 +01:51:23.52 AT 2026pfn 2026-06-02.70 20.7
13:04:27.660 +01:03:38.69 AT 2026pfm 2026-06-02.70 20.61
13:02:48.460 -00:02:57.35 AT 2026pfl 2026-06-02.70 20.42
13:32:29.920 -00:51:10.16 AT 2026pfk 2026-06-08.70 21.85
22:56:19.417 -34:42:19.31 AT 2026pfj 2026-05-18.41 20.44
17:18:30.019 +34:15:44.23 AT 2026pfi 2026-06-14.39 21
14:56:10.823 +09:51:29.24 AT 2026pfh 2026-05-12.12 20.36
14:14:37.201 +14:25:05.82 AT 2026pfg 2026-06-14.19 19.2685
23:15:33.309 +78:21:30.20 AT 2026pff 2026-06-04.38 20.0549
21:04:19.065 -12:09:15.14 AT 2026pfe 2026-05-14.45 20.4546
22:12:18.808 +78:44:00.16 AT 2026pfd 2026-06-04.38 20.0909
20:22:23.781 +14:16:24.43 AT 2026pfc 2026-06-11.40 20.7598
22:15:43.151 +19:13:42.63 AT 2026pfb 2026-06-14.54 20.6
18:54:55.933 +32:59:51.61 AT 2026pfa 2026-06-10.35 21.0115
-rw-r--r-- 1 apache apache 30K Jun 23 06:13 tns_transients_list.txt
