This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4
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 22.4059 2461213.9059 8.78 01:56:38.03 +59:15:34.2
131.18801 -2.56317 galactic Cas Second-epoch detections are separated by 0.2" and 7.0 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 01:56:38.03 +59:15:34.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.03 +59:15:34.2: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 56 38.03 +59 15 34.2 8.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
X Cas,2461213.9059,8.78,0.05,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
X Cas 20260622.4059 8.78CV 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 22.4059 2461213.9059 12.12 02:13:57.98 +64:54:41.5
131.54013 3.42816 galactic Cas Second-epoch detections are separated by 2.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:13:57.98 +64:54:41.5 (user input) | T | P | (position from user input) J-Ks=1.116+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:57.98 +64:54:41.5: 12.97 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:57.98 +64:54:41.5: 15.14 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.64 +/- 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 22.4059* 02 13 57.98 +64 54 41.5 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.99 01:22:37.56 +58:29:18.7
127.00866 -4.13614 galactic Cas Second-epoch detections are separated by 2.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:22:37.56 +58:29:18.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:37.56 +58:29:18.7: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:37.56 +58:29:18.7: 14.74 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.74 +/- 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 22.4059* 01 22 37.56 +58 29 18.7 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,2461213.9059,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.88 01:15:31.02 +60:11:14.3
125.92355 -2.54450 galactic Cas Second-epoch detections are separated by 2.2" 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 | 01:15:31.02 +60:11:14.3 (user input) | T | P | (position from user input) J-Ks=0.490+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:31.02 +60:11:14.3: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:31.02 +60:11:14.3: 14.36 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 15 31.02 +60 11 14.3 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.87 01:06:49.17 +60:52:38.6
124.80339 -1.93845 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 | target | 01:06:49.17 +60:52:38.6 (user input) | T | P | (position from user input) J-Ks=1.040+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:49.17 +60:52:38.6: 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 01:06:49.17 +60:52:38.6: 14.54 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.54 +/- 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 22.4059* 01 06 49.17 +60 52 38.6 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.94 01:33:22.79 +61:41:09.1
127.88415 -0.78195 galactic Cas Second-epoch detections are separated by 2.2" 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 | target | 01:33:22.79 +61:41:09.1 (user input) | T | P | (position from user input) J-Ks=0.299+/-0.041 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:22.79 +61:41:09.1: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:22.79 +61:41:09.1: 14.67 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.67 +/- 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 22.4059* 01 33 22.79 +61 41 09.1 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.94,0.05,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
target 20260622.4059 11.94CV 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 22.4059 2461213.9059 11.87 01:13:56.67 +59:30:04.6
125.78872 -3.24557 galactic Cas Second-epoch detections are separated by 3.0" 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 | ATO J018.4722+59.5061 | 01:13:56.67 +59:30:04.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.313+/-0.048 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:56.67 +59:30:04.6: 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 01:13:56.67 +59:30:04.6: 14.67 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.67 +/- 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 22.4059* 01 13 56.67 +59 30 04.6 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J018.4722+59.5061,2461213.9059,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J018.4722+59.5061 20260622.4059 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.84 01:19:29.37 +60:17:35.0
126.40373 -2.38946 galactic Cas Second-epoch detections are separated by 3.5" 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 | target | 01:19:29.37 +60:17:35.0 (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 01:19:29.37 +60:17:35.0: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:29.37 +60:17:35.0: 14.45 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.45 +/- 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 22.4059* 01 19 29.37 +60 17 35.0 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.84,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.87 01:43:44.10 +58:30:28.3
129.73244 -3.67167 galactic Cas Second-epoch detections are separated by 0.7" 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 | ATO J025.9395+58.5048 | 01:43:44.10 +58:30:28.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.840+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:44.10 +58:30:28.3: 12.24 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:44.10 +58:30:28.3: 14.74 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 22.4059* 01 43 44.10 +58 30 28.3 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.9395+58.5048,2461213.9059,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.9395+58.5048 20260622.4059 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.92 01:28:02.88 +62:04:06.1
127.20503 -0.49926 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 | 01:28:02.88 +62:04:06.1 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.040 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:02.88 +62:04:06.1: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:02.88 +62:04:06.1: 14.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.39 +/- 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 22.4059* 01 28 02.88 +62 04 06.1 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260622.4059 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.85 01:14:36.05 +59:51:11.4
125.84012 -2.88772 galactic Cas Second-epoch detections are separated by 2.5" and 7.1 pix
The object was found in VSX20" Gaia DR3 414298631353868160
Type: ROT
# Max. Min./Amp. JD0 Period
16.760 G 16.880 G 1.589320000000 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 01:14:36.05 +59:51:11.4: 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 01:14:36.05 +59:51:11.4: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 14 36.05 +59 51 11.4 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 414298631353868160,2461213.9059,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 414298631353868160 20260622.4059 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.92 01:39:44.00 +57:57:02.6
129.32294 -4.32049 galactic Cas Second-epoch detections are separated by 1.3" 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 | target | 01:39:44.00 +57:57:02.6 (user input) | T | P | (position from user input) J-Ks=0.528+/-0.039 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:44.00 +57:57:02.6: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:44.00 +57:57:02.6: 14.59 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.59 +/- 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 22.4059* 01 39 44.00 +57 57 02.6 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260622.4059 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.76 01:59:39.67 +58:16:32.4
131.81987 -3.41390 galactic Cas Second-epoch detections are separated by 1.2" 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 | target | 01:59:39.67 +58:16:32.4 (user input) | T | P | (position from user input) SpType: WD (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:39.67 +58:16:32.4: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:39.67 +58:16:32.4: 14.36 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.36 +/- 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 22.4059* 01 59 39.67 +58 16 32.4 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,2461213.9059,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.74 01:16:16.54 +59:38:19.7
126.07044 -3.08150 galactic Cas Second-epoch detections are separated by 2.9" and 7.0 pix
The object was found in VSX 3" Gaia DR3 414245786074278144
Type: ROT
# Max. Min./Amp. JD0 Period
14.400 G 14.420 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 01:16:16.54 +59:38:19.7: 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 01:16:16.54 +59:38:19.7: 14.35 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.35 +/- 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 22.4059* 01 16 16.54 +59 38 19.7 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414245786074278144,2461213.9059,11.74,0.05,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 414245786074278144 20260622.4059 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 22.4059 2461213.9059 11.80 01:26:01.63 +59:58:53.0
127.25013 -2.60004 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 | Large-amplitude variable Gaia DR2 510192022562175744 | 01:26:01.63 +59:58:53.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.507+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:01.63 +59:58:53.0: 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 01:26:01.63 +59:58:53.0: 14.76 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 26 01.63 +59 58 53.0 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 510192022562175744,2461213.9059,11.80,0.05,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
Large-amplitude variable Gaia DR2 510192022562175744 20260622.4059 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 22.4059 2461213.9059 11.78 01:11:16.45 +58:55:56.1
125.49446 -3.84077 galactic Cas Second-epoch detections are separated by 2.2" 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 | ATO J017.8423+58.9300 | 01:11:16.45 +58:55:56.1 (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 +58:55:56.1: 12.05 +/- 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 +58:55:56.1: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.69 +/- 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 22.4059* 01 11 16.45 +58 55 56.1 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.8423+58.9300,2461213.9059,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.8423+58.9300 20260622.4059 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.77 01:59:07.36 +58:48:33.4
131.61275 -2.91700 galactic Cas Second-epoch detections are separated by 3.7" 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 | 01:59:07.36 +58:48:33.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:07.36 +58:48:33.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:07.36 +58:48:33.4: 14.56 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 59 07.36 +58 48 33.4 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,2461213.9059,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.84 01:36:52.29 +58:28:35.9
128.85583 -3.87157 galactic Cas Second-epoch detections are separated by 2.5" 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 J024.2248+58.4804 | 01:36:52.29 +58:28:35.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.345+/-0.047 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:52.29 +58:28:35.9: 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 01:36:52.29 +58:28:35.9: 14.65 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.65 +/- 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 22.4059* 01 36 52.29 +58 28 35.9 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
ATO J024.2248+58.4804,2461213.9059,11.84,0.05,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
ATO J024.2248+58.4804 20260622.4059 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 22.4059 2461213.9059 11.82 01:19:08.74 +60:17:20.1
126.36179 -2.39818 galactic Cas Second-epoch detections are separated by 7.4" and 7.9 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 | 01:19:08.74 +60:17:20.1 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:08.74 +60:17:20.1: 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 01:19:08.74 +60:17:20.1: 14.69 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 19 08.74 +60 17 20.1 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.58 01:23:56.64 +62:15:29.2
126.70486 -0.37527 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 | 01:23:56.64 +62:15:29.2 (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 01:23:56.64 +62:15:29.2: 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 01:23:56.64 +62:15:29.2: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 23 56.64 +62 15 29.2 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260622.4059 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.91 01:41:12.20 +60:00:52.4
129.11791 -2.25813 galactic Cas Second-epoch detections are separated by 0.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:41:12.20 +60:00:52.4 (user input) | T | P | (position from user input) J-Ks=0.973+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:12.20 +60:00:52.4: 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 01:41:12.20 +60:00:52.4: 14.67 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.67 +/- 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 22.4059* 01 41 12.20 +60 00 52.4 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.76 01:16:20.25 +58:49:31.5
126.15701 -3.89032 galactic Cas Second-epoch detections are separated by 1.2" 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 J019.0953+58.8254 | 01:16:20.25 +58:49:31.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.089+/-0.090 (A)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:20.25 +58:49:31.5: 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 01:16:20.25 +58:49:31.5: 14.65 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.65 +/- 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 22.4059* 01 16 20.25 +58 49 31.5 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J019.0953+58.8254,2461213.9059,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J019.0953+58.8254 20260622.4059 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.73 01:32:34.60 +60:01:12.0
128.05507 -2.44190 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 | 01:32:34.60 +60:01:12.0 (user input) | T | P | (position from user input) J-Ks=0.925+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:34.60 +60:01:12.0: 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 01:32:34.60 +60:01:12.0: 14.25 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.25 +/- 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 22.4059* 01 32 34.60 +60 01 12.0 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
target,2461213.9059,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.71 02:15:20.97 +63:07:35.0
132.24949 1.78270 galactic Cas Second-epoch detections are separated by 0.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:15:20.97 +63:07:35.0 (user input) | T | P | (position from user input) J-Ks=0.177+/-0.041 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:20.97 +63:07:35.0: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:20.97 +63:07:35.0: 14.25 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 02 15 20.97 +63 07 35.0 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
target,2461213.9059,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 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 22.4059 2461213.9059 11.56 01:08:06.01 +61:33:37.1
124.91482 -1.24728 galactic Cas Second-epoch detections are separated by 5.1" and 8.1 pix
The object was found in VSX23" Gaia DR3 522537614010556928
Type: ROT
# Max. Min./Amp. JD0 Period
16.000 G 16.030 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 01:08:06.01 +61:33:37.1: 12.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:06.01 +61:33:37.1: 14.23 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.23 +/- 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 22.4059* 01 08 06.01 +61 33 37.1 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522537614010556928,2461213.9059,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522537614010556928 20260622.4059 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.80 01:43:24.05 +61:12:07.1
129.14960 -1.04091 galactic Cas Second-epoch detections are separated by 1.9" and 7.0 pix
The object was found in VSX 1" Gaia DR3 511249649679966976
Type: ROT
# Max. Min./Amp. JD0 Period
14.700 G 14.730 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:24.05 +61:12:07.1: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:24.05 +61:12:07.1: 14.82 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.82 +/- 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 22.4059* 01 43 24.05 +61 12 07.1 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511249649679966976,2461213.9059,11.80,0.05,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 511249649679966976 20260622.4059 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 22.4059 2461213.9059 11.54 01:06:16.00 +57:53:25.1
124.90876 -4.92451 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 | ATO J016.5720+57.8855 | 01:06:16.00 +57:53:25.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.781+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:16.00 +57:53:25.1: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:16.00 +57:53:25.1: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 06 16.00 +57 53 25.1 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J016.5720+57.8855,2461213.9059,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J016.5720+57.8855 20260622.4059 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.61 01:47:11.11 +58:16:20.0
130.22474 -3.80797 galactic Cas Second-epoch detections are separated by 4.4" 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 506003364304536448 | 01:47:15.99 +58:16:15.9 (Gaia DR3) | DSCT/GDOR (local) | F (local) | Gaia3var=VARIABLE J-Ks=0.509+/-0.038 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:11.11 +58:16:20.0: 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 01:47:11.11 +58:16:20.0: 14.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 47 11.11 +58 16 20.0 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506003364304536448,2461213.9059,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506003364304536448 20260622.4059 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.72 01:49:03.19 +60:18:50.1
130.01182 -1.76344 galactic Cas Second-epoch detections are separated by 2.8" and 7.2 pix
The object was found in VSX 2" Gaia DR3 508151466431224704
Type: ROT
# Max. Min./Amp. JD0 Period
14.750 G 14.780 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 01:49:03.19 +60:18:50.1: 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 01:49:03.19 +60:18:50.1: 14.54 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.54 +/- 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 22.4059* 01 49 03.19 +60 18 50.1 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 508151466431224704,2461213.9059,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508151466431224704 20260622.4059 11.72CV 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 22.4059 2461213.9059 11.54 01:12:41.15 +61:18:07.7
125.48070 -1.46441 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 | target | 01:12:41.15 +61:18:07.7 (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 01:12:41.15 +61:18:07.7: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:41.15 +61:18:07.7: 14.00 +/- 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 22.4059* 01 12 41.15 +61 18 07.7 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
target,2461213.9059,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.70 01:41:20.99 +58:11:50.9
129.48639 -4.03768 galactic Cas Second-epoch detections are separated by 1.7" 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 J025.3435+58.1901 | 01:41:20.99 +58:11:50.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.725+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:20.99 +58:11:50.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:20.99 +58:11:50.9: 14.73 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.73 +/- 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 22.4059* 01 41 20.99 +58 11 50.9 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.3435+58.1901,2461213.9059,11.70,0.05,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 J025.3435+58.1901 20260622.4059 11.70CV 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 22.4059 2461213.9059 11.67 02:00:30.18 +62:28:28.3
130.81657 0.66478 galactic Cas Second-epoch detections are separated by 4.6" 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 508839142234060544 | 02:00:35.69 +62:28:19.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.387+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:30.18 +62:28:28.3: 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 02:00:30.18 +62:28:28.3: 14.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.22 +/- 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 22.4059* 02 00 30.18 +62 28 28.3 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508839142234060544,2461213.9059,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508839142234060544 20260622.4059 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.63 02:12:28.25 +62:23:03.9
132.16922 0.97486 galactic Cas Second-epoch detections are separated by 1.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:12:28.25 +62:23:03.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:12:28.25 +62:23:03.9: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:12:28.25 +62:23:03.9: 14.55 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.55 +/- 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 22.4059* 02 12 28.25 +62 23 03.9 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 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 22.4059 2461213.9059 11.55 01:30:58.15 +59:29:29.4
127.93744 -2.99551 galactic Cas Second-epoch detections are separated by 4.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:30:58.15 +59:29:29.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:58.15 +59:29:29.4: 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 01:30:58.15 +59:29:29.4: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 30 58.15 +59 29 29.4 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,2461213.9059,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.52 01:24:44.68 +63:34:17.1
126.62800 0.93894 galactic Cas Second-epoch detections are separated by 3.3" 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 | 01:24:44.68 +63:34:17.1 (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 01:24:44.68 +63:34:17.1: 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 01:24:44.68 +63:34:17.1: 14.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 24 44.68 +63 34 17.1 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.52,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.54 01:32:09.12 +61:32:10.9
127.76393 -0.95283 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 | target | 01:32:09.12 +61:32:10.9 (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 01:32:09.12 +61:32:10.9: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:09.12 +61:32:10.9: 14.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.16 +/- 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 22.4059* 01 32 09.12 +61 32 10.9 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.53 01:48:26.29 +60:22:28.9
129.92418 -1.72092 galactic Cas Second-epoch detections are separated by 4.3" 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 506654584430151168 | 01:48:21.28 +60:22:36.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.812+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:26.29 +60:22:28.9: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:26.29 +60:22:28.9: 14.33 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.33 +/- 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 22.4059* 01 48 26.29 +60 22 28.9 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506654584430151168,2461213.9059,11.53,0.05,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 506654584430151168 20260622.4059 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 22.4059 2461213.9059 11.52 01:13:34.72 +58:01:48.7
125.86931 -4.71522 galactic Cas Second-epoch detections are separated by 2.7" 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 | ATO J018.3748+58.0330 | 01:13:34.72 +58:01:48.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.078+/-0.053 (A)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:34.72 +58:01:48.7: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:34.72 +58:01:48.7: 14.09 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.09 +/- 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 22.4059* 01 13 34.72 +58 01 48.7 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 J018.3748+58.0330,2461213.9059,11.52,0.05,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
ATO J018.3748+58.0330 20260622.4059 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 22.4059 2461213.9059 11.65 01:05:53.86 +59:06:25.2
124.79095 -3.71255 galactic Cas Second-epoch detections are separated by 2.3" 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 | 01:05:53.86 +59:06:25.2 (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 01:05:53.86 +59:06:25.2: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:53.86 +59:06:25.2: 14.39 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.39 +/- 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 22.4059* 01 05 53.86 +59 06 25.2 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.65,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.58 01:45:17.42 +62:09:43.0
129.17348 -0.05543 galactic Cas Second-epoch detections are separated by 2.7" 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 | 01:45:17.42 +62:09:43.0 (user input) | T | P | (position from user input) J-Ks=0.890+/-0.044 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:17.42 +62:09:43.0: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:17.42 +62:09:43.0: 14.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.36 +/- 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 22.4059* 01 45 17.42 +62 09 43.0 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260622.4059 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.32 01:53:37.98 +64:44:10.2
129.50829 2.66151 galactic Cas Second-epoch detections are separated by 1.8" and 7.0 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 01:53:37.98 +64:44:10.2: 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 01:53:37.98 +64:44:10.2: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 53 37.98 +64 44 10.2 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
Gaia DR3 518235499886390016,2461213.9059,11.32,0.05,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 518235499886390016 20260622.4059 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 22.4059 2461213.9059 11.49 01:33:12.85 +61:16:55.2
127.92994 -1.18369 galactic Cas Second-epoch detections are separated by 1.8" 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 | 01:33:12.85 +61:16:55.2 (user input) | T | P | (position from user input) J-Ks=0.549+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:12.85 +61:16:55.2: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:12.85 +61:16:55.2: 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 22.4059* 01 33 12.85 +61 16 55.2 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.49,0.05,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
target 20260622.4059 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 22.4059 2461213.9059 11.41 01:57:29.35 +60:09:19.2
131.06698 -1.66901 galactic Cas Second-epoch detections are separated by 2.8" 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 | 01:57:29.35 +60:09:19.2 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:29.35 +60:09:19.2: 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 01:57:29.35 +60:09:19.2: 14.10 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 57 29.35 +60 09 19.2 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.41,0.05,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
target 20260622.4059 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 22.4059 2461213.9059 11.62 01:52:02.35 +59:36:20.4
130.53697 -2.36828 galactic Cas Second-epoch detections are separated by 1.3" 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 | 01:52:02.35 +59:36:20.4 (user input) | T | P | (position from user input) J-Ks=0.457+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:02.35 +59:36:20.4: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:02.35 +59:36:20.4: 14.44 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 52 02.35 +59 36 20.4 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,2461213.9059,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.52 01:42:02.51 +59:46:32.9
129.26740 -2.47202 galactic Cas Second-epoch detections are separated by 3.9" 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 | target | 01:42:02.51 +59:46:32.9 (user input) | T | P | (position from user input) J-Ks=1.106+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:02.51 +59:46:32.9: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:02.51 +59:46:32.9: 14.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.09 +/- 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 22.4059* 01 42 02.51 +59 46 32.9 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.52,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.26 01:08:25.45 +59:48:03.8
125.06942 -3.00018 galactic Cas Second-epoch detections are separated by 0.6" 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 | 01:08:25.45 +59:48:03.8 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:25.45 +59:48:03.8: 12.34 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:25.45 +59:48:03.8: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 08 25.45 +59 48 03.8 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,2461213.9059,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.39 01:36:47.04 +59:24:04.7
128.68220 -2.96322 galactic Cas Second-epoch detections are separated by 2.9" 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 | 01:36:47.04 +59:24:04.7 (user input) | T | P | (position from user input) J-Ks=0.996+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:47.04 +59:24:04.7: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:47.04 +59:24:04.7: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 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 22.4059* 01 36 47.04 +59 24 04.7 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.39,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.34 01:20:38.69 +59:28:19.0
126.63920 -3.18941 galactic Cas Second-epoch detections are separated by 2.2" and 7.5 pix
The object was found in VSX 1" Gaia DR3 414043785174768640
Type: VAR
# Max. Min./Amp. JD0 Period
14.160 G 14.190 G 0.319087000000 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 01:20:38.69 +59:28:19.0: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:38.69 +59:28:19.0: 14.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.07 +/- 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 22.4059* 01 20 38.69 +59 28 19.0 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 414043785174768640,2461213.9059,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 414043785174768640 20260622.4059 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 22.4059 2461213.9059 11.31 01:17:26.20 +61:54:16.6
125.98808 -0.81277 galactic Cas Second-epoch detections are separated by 3.3" 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 | 01:17:26.20 +61:54:16.6 (user input) | T | P | (position from user input) J-Ks=0.409+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:26.20 +61:54:16.6: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:26.20 +61:54:16.6: 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 22.4059* 01 17 26.20 +61 54 16.6 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
target,2461213.9059,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.49 01:32:10.96 +59:36:02.6
128.07256 -2.86374 galactic Cas Second-epoch detections are separated by 2.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J023.0277+59.5942 | 01:32:10.96 +59:36:02.6 (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 01:32:10.96 +59:36:02.6: 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 01:32:10.96 +59:36:02.6: 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 22.4059* 01 32 10.96 +59 36 02.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J023.0277+59.5942,2461213.9059,11.49,0.05,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 J023.0277+59.5942 20260622.4059 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 22.4059 2461213.9059 11.36 01:22:33.22 +60:44:43.0
126.72661 -1.89701 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 | target | 01:22:33.22 +60:44:43.0 (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 01:22:33.22 +60:44:43.0: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:33.22 +60:44:43.0: 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 22.4059* 01 22 33.22 +60 44 43.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.36,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.35 01:18:32.34 +57:50:16.0
126.54541 -4.84370 galactic Cas Second-epoch detections are separated by 1.7" and 7.6 pix
The object was found in VSX11" Gaia DR3 413838790671438848
Type: ROT
# Max. Min./Amp. JD0 Period
17.740 G 17.880 G 1.952940000000
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 01:18:32.34 +57:50:16.0: 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 01:18:32.34 +57:50:16.0: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 18 32.34 +57 50 16.0 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 413838790671438848,2461213.9059,11.35,0.05,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
Gaia DR3 413838790671438848 20260622.4059 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 22.4059 2461213.9059 11.52 02:11:00.59 +60:08:50.5
132.68552 -1.20887 galactic Cas Second-epoch detections are separated by 3.6" 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 | 02:11:00.59 +60:08:50.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:00.59 +60:08:50.5: 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 02:11:00.59 +60:08:50.5: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 02 11 00.59 +60 08 50.5 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,2461213.9059,11.52,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.40 01:47:04.41 +59:18:56.1
129.98641 -2.79200 galactic Cas Second-epoch detections are separated by 2.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:47:04.41 +59:18:56.1 (user input) | T | P | (position from user input) J-Ks=0.500+/-0.079 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:04.41 +59:18:56.1: 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 01:47:04.41 +59:18:56.1: 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 22.4059* 01 47 04.41 +59 18 56.1 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.38 01:32:41.63 +60:27:01.5
128.00084 -2.01466 galactic Cas Second-epoch detections are separated by 2.4" and 7.4 pix
The object was found in VSX19" Gaia DR3 509836085739801344
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.010 G 13.070 G 0.150333900000 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 01:32:41.63 +60:27:01.5: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:41.63 +60:27:01.5: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 32 41.63 +60 27 01.5 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 509836085739801344,2461213.9059,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509836085739801344 20260622.4059 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.33 01:12:09.67 +58:47:54.3
125.61960 -3.96515 galactic Cas Second-epoch detections are separated by 3.0" 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 | target | 01:12:09.67 +58:47:54.3 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:09.67 +58:47:54.3: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:09.67 +58:47:54.3: 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 22.4059* 01 12 09.67 +58 47 54.3 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,2461213.9059,11.33,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.26 01:21:45.28 +58:34:14.7
126.88562 -4.06808 galactic Cas Second-epoch detections are separated by 4.8" and 8.1 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 01:21:45.28 +58:34:14.7: 12.70 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:45.28 +58:34:14.7: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 21 45.28 +58 34 14.7 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
ZTF J012144.11+583432.6,2461213.9059,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J012144.11+583432.6 20260622.4059 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.16 01:08:39.03 +60:32:42.2
125.04807 -2.25595 galactic Cas Second-epoch detections are separated by 1.6" 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 | 01:08:39.03 +60:32:42.2 (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 01:08:39.03 +60:32:42.2: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:39.03 +60:32:42.2: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 08 39.03 +60 32 42.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 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 22.4059 2461213.9059 11.21 01:10:05.00 +57:48:02.6
125.42324 -4.98081 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 | 01:10:05.00 +57:48:02.6 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:05.00 +57:48:02.6: 12.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:05.00 +57:48:02.6: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 10 05.00 +57 48 02.6 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,2461213.9059,11.21,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.31 01:30:39.42 +59:02:43.7
127.96604 -3.44240 galactic Cas Second-epoch detections are separated by 0.8" and 7.1 pix
The object was found in VSX23" Gaia DR3 509249363151279232
Type: RS
# Max. Min./Amp. JD0 Period
15.470 G 15.520 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 01:30:39.42 +59:02:43.7: 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 01:30:39.42 +59:02:43.7: 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 22.4059* 01 30 39.42 +59 02 43.7 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 509249363151279232,2461213.9059,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509249363151279232 20260622.4059 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.09 01:10:43.79 +60:59:19.0
125.27002 -1.79553 galactic Cas Second-epoch detections are separated by 0.1" 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 | target | 01:10:43.79 +60:59:19.0 (user input) | T | P | (position from user input) J-Ks=0.354+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:43.79 +60:59:19.0: 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 01:10:43.79 +60:59:19.0: 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 22.4059* 01 10 43.79 +60 59 19.0 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,2461213.9059,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.18 01:12:59.89 +57:33:53.5
125.83169 -5.18545 galactic Cas Second-epoch detections are separated by 2.2" 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 | target | 01:12:59.89 +57:33:53.5 (user input) | T | P | (position from user input) J-Ks=0.836+/-0.053 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:59.89 +57:33:53.5: 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 01:12:59.89 +57:33:53.5: 13.76 +/- 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 22.4059* 01 12 59.89 +57 33 53.5 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,2461213.9059,11.18,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.12 01:06:59.51 +61:28:40.4
124.78806 -1.33779 galactic Cas Second-epoch detections are separated by 3.5" and 7.9 pix
The object was found in VSX 7" 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 01:06:59.51 +61:28:40.4: 12.76 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:59.51 +61:28:40.4: 13.62 +/- 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 22.4059* 01 06 59.51 +61 28 40.4 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522542355648755328,2461213.9059,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522542355648755328 20260622.4059 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 22.4059 2461213.9059 11.21 01:07:36.77 +58:09:25.4
125.07112 -4.64749 galactic Cas Second-epoch detections are separated by 1.1" 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 | 01:07:36.77 +58:09:25.4 (user input) | T | P | (position from user input) J-Ks=0.277+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:36.77 +58:09:25.4: 12.58 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:36.77 +58:09:25.4: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 07 36.77 +58 09 25.4 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.21,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.19 01:59:41.75 +63:32:25.4
130.44809 1.66913 galactic Cas Second-epoch detections are separated by 6.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:59:41.75 +63:32:25.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:41.75 +63:32:25.4: 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 01:59:41.75 +63:32:25.4: 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 22.4059* 01 59 41.75 +63 32 25.4 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.19,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.27 01:13:19.97 +61:29:38.9
125.54182 -1.26661 galactic Cas Second-epoch detections are separated by 3.5" and 7.7 pix
The object was found in VSX17" Gaia DR3 522571492708068608
Type: ROT
# Max. Min./Amp. JD0 Period
14.070 G 14.120 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:19.97 +61:29:38.9: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:19.97 +61:29:38.9: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 13 19.97 +61 29 38.9 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 522571492708068608,2461213.9059,11.27,0.05,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 522571492708068608 20260622.4059 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 22.4059 2461213.9059 11.16 01:36:49.02 +62:46:52.5
128.09414 0.36521 galactic Cas Second-epoch detections are separated by 2.5" and 7.2 pix
The object was found in VSX16" 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 01:36:49.02 +62:46:52.5: 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 01:36:49.02 +62:46:52.5: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 22.4059* 01 36 49.02 +62 46 52.5 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 512426436360507392,2461213.9059,11.16,0.05,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 512426436360507392 20260622.4059 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 22.4059 2461213.9059 11.02 01:06:13.06 +59:33:47.0
124.80579 -3.25491 galactic Cas Second-epoch detections are separated by 0.2" 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 | 01:06:13.06 +59:33:47.0 (user input) | T | P | (position from user input) J-Ks=0.462+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:13.06 +59:33:47.0: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:13.06 +59:33:47.0: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 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 22.4059* 01 06 13.06 +59 33 47.0 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 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 22.4059 2461213.9059 11.29 01:30:00.97 +60:10:50.2
127.71474 -2.33240 galactic Cas Second-epoch detections are separated by 0.2" and 7.0 pix
The object was found in VSX22" Gaia DR3 509459713474637440
Type: VAR
# Max. Min./Amp. JD0 Period
13.340 G 13.370 G 0.014865300000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:00.97 +60:10:50.2: 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 01:30:00.97 +60:10:50.2: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 22.4059* 01 30 00.97 +60 10 50.2 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
Gaia DR3 509459713474637440,2461213.9059,11.29,0.05,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 509459713474637440 20260622.4059 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 22.4059 2461213.9059 11.11 01:43:27.45 +58:38:06.5
129.67128 -3.55428 galactic Cas Second-epoch detections are separated by 1.4" and 7.1 pix
The object was found in VSX 1" Gaia DR3 506084487648397824
Type: ROT
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:27.45 +58:38:06.5: 12.68 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:27.45 +58:38:06.5: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 43 27.45 +58 38 06.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506084487648397824,2461213.9059,11.11,0.05,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 506084487648397824 20260622.4059 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 22.4059 2461213.9059 11.09 01:51:47.42 +58:37:58.5
130.73225 -3.32182 galactic Cas Second-epoch detections are separated by 1.7" 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 506225156418009984 | 01:51:45.68 +58:37:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.890+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:47.42 +58:37:58.5: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:47.42 +58:37:58.5: 13.98 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 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 22.4059* 01 51 47.42 +58 37 58.5 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 506225156418009984,2461213.9059,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506225156418009984 20260622.4059 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.27 01:56:13.05 +59:33:49.7
131.06076 -2.28167 galactic Cas Second-epoch detections are separated by 2.5" 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 | 01:56:13.05 +59:33:49.7 (user input) | T | P | (position from user input) J-Ks=0.814+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:13.05 +59:33:49.7: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:13.05 +59:33:49.7: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 56 13.05 +59 33 49.7 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 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 22.4059 2461213.9059 11.24 02:03:04.99 +57:50:13.7
132.37450 -3.71513 galactic Per Second-epoch detections are separated by 2.9" and 7.1 pix
The object was found in VSX23" ASASSN-V J020303.97+575035.2
Type: SR
# Max. Min./Amp. JD0 Period
13.810 V 14.190 V 2458279.67980 113.240657400000
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 02:03:04.99 +57:50:13.7: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:04.99 +57:50:13.7: 13.88 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 22.4059* 02 03 04.99 +57 50 13.7 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
ASASSN-V J020303.97+575035.2,2461213.9059,11.24,0.05,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
ASASSN-V J020303.97+575035.2 20260622.4059 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 22.4059 2461213.9059 11.04 01:24:54.86 +59:41:45.2
127.14909 -2.90147 galactic Cas Second-epoch detections are separated by 3.9" 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 | target | 01:24:54.86 +59:41:45.2 (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 01:24:54.86 +59:41:45.2: 12.88 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:54.86 +59:41:45.2: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 24 54.86 +59 41 45.2 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,2461213.9059,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 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 22.4059 2461213.9059 11.14 01:25:27.57 +59:27:15.1
127.24926 -3.13206 galactic Cas Second-epoch detections are separated by 0.7" and 7.2 pix
The object was found in VSX 5" Gaia DR3 510073344036983552
Type: ROT
# Max. Min./Amp. JD0 Period
14.460 G 14.520 G 1.820050000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:27.57 +59:27:15.1: 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 01:25:27.57 +59:27:15.1: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 25 27.57 +59 27 15.1 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
Gaia DR3 510073344036983552,2461213.9059,11.14,0.05,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 510073344036983552 20260622.4059 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 22.4059 2461213.9059 10.97 01:18:31.18 +60:17:31.5
126.28426 -2.40327 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 510355643647241856 | 01:18:31.14 +60:17:06.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.354+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:31.18 +60:17:31.5: 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 01:18:31.18 +60:17:31.5: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 18 31.18 +60 17 31.5 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510355643647241856,2461213.9059,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510355643647241856 20260622.4059 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.10 01:12:00.91 +64:42:20.0
125.12875 1.92161 galactic Cas Second-epoch detections are separated by 0.5" and 7.4 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 01:12:00.91 +64:42:20.0: 11.73 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:00.91 +64:42:20.0: 13.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 22.4059* 01 12 00.91 +64 42 20.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J011201.03+644221.2,2461213.9059,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011201.03+644221.2 20260622.4059 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 22.4059 2461213.9059 10.99 01:07:01.45 +59:43:01.3
124.89858 -3.09519 galactic Cas Second-epoch detections are separated by 1.9" 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 426209670869309056 | 01:07:01.24 +59:42:31.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.817+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:01.45 +59:43:01.3: 12.86 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:01.45 +59:43:01.3: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 07 01.45 +59 43 01.3 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 426209670869309056,2461213.9059,10.99,0.05,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 426209670869309056 20260622.4059 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 22.4059 2461213.9059 11.08 01:07:39.20 +59:59:18.4
124.96074 -2.81941 galactic Cas Second-epoch detections are separated by 1.9" 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 | target | 01:07:39.20 +59:59:18.4 (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 01:07:39.20 +59:59:18.4: 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 01:07:39.20 +59:59:18.4: 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 22.4059* 01 07 39.20 +59 59 18.4 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.08,0.05,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
target 20260622.4059 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 22.4059 2461213.9059 11.10 02:00:21.98 +58:20:18.3
131.89287 -3.32902 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 | 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 02:00:21.98 +58:20:18.3: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:21.98 +58:20:18.3: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 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 22.4059* 02 00 21.98 +58 20 18.3 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 505499508799542016,2461213.9059,11.10,0.05,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 505499508799542016 20260622.4059 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 22.4059 2461213.9059 10.91 01:34:16.42 +60:57:34.8
128.10886 -1.48079 galactic Cas Second-epoch detections are separated by 1.5" 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 | target | 01:34:16.42 +60:57:34.8 (user input) | T | P | (position from user input) J-Ks=0.888+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:16.42 +60:57:34.8: 12.54 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:16.42 +60:57:34.8: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 34 16.42 +60 57 34.8 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 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 22.4059 2461213.9059 11.04 02:00:23.29 +64:54:51.9
130.15953 3.01468 galactic Cas Second-epoch detections are separated by 4.3" 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 | target | 02:00:23.29 +64:54:51.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:23.29 +64:54:51.9: 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 02:00:23.29 +64:54:51.9: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 02 00 23.29 +64 54 51.9 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,2461213.9059,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 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 22.4059 2461213.9059 10.78 01:07:31.78 +61:28:29.6
124.85235 -1.33684 galactic Cas Second-epoch detections are separated by 2.1" 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 | 01:07:31.78 +61:28:29.6 (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 01:07:31.78 +61:28:29.6: 12.82 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:31.78 +61:28:29.6: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 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 22.4059* 01 07 31.78 +61 28 29.6 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
target,2461213.9059,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 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 22.4059 2461213.9059 10.61 01:31:23.12 +59:33:43.4
127.97878 -2.91768 galactic Cas Second-epoch detections are separated by 2.1" 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 | ATO J022.8294+59.5638 | 01:31:23.12 +59:33:43.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.833+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:23.12 +59:33:43.4: 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 01:31:23.12 +59:33:43.4: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 31 23.12 +59 33 43.4 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J022.8294+59.5638,2461213.9059,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.8294+59.5638 20260622.4059 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 10.11 01:23:22.18 +60:18:16.6
126.88016 -2.32212 galactic Cas Second-epoch detections are separated by 1.6" and 7.5 pix
The object was found in ASASSN-V 1" ASASSN-V J012322.23+601815.3
Type: SR
MeanMag 13.9 m Amp. 0.58 m Period 154.4455167 d
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 01:23:22.18 +60:18:16.6: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:22.18 +60:18:16.6: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 22.4059* 01 23 22.18 +60 18 16.6 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461213.9059,10.11,0.05,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
VARIABLE_NAME 20260622.4059 10.11CV 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 22.4059 2461213.9059 10.13 01:57:04.38 +58:53:27.3
131.33527 -2.90581 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 | Gaia DR3 506288893734057856 | 01:57:03.38 +58:53:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.729+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:04.38 +58:53:27.3: 13.13 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:04.38 +58:53:27.3: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 22.4059* 01 57 04.38 +58 53 27.3 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506288893734057856,2461213.9059,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506288893734057856 20260622.4059 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 10.46 01:18:28.11 +58:11:23.7
126.49892 -4.49450 galactic Cas Second-epoch detections are separated by 1.8" 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 | ATO J019.6245+58.1745 | 01:18:29.87 +58:10:59.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G8III 1951UppAn...2j...1B NGC 457 236 J-Ks=0.371+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:28.11 +58:11:23.7: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:28.11 +58:11:23.7: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 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 22.4059* 01 18 28.11 +58 11 23.7 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J019.6245+58.1745,2461213.9059,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J019.6245+58.1745 20260622.4059 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 10.90 01:32:05.63 +61:59:26.8
127.68570 -0.50514 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 | 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 01:32:05.63 +61:59:26.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:05.63 +61:59:26.8: 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 22.4059* 01 32 05.63 +61 59 26.8 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510798197068398848,2461213.9059,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510798197068398848 20260622.4059 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 10.98 01:44:02.95 +61:54:45.6
129.08214 -0.32922 galactic Cas Second-epoch detections are separated by 7.8" 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
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:02.95 +61:54:45.6: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:02.95 +61:54:45.6: 13.98 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.98 +/- 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 22.4059* 01 44 02.95 +61 54 45.6 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511486800591720192,2461213.9059,10.98,0.05,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 511486800591720192 20260622.4059 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 22.4059 2461213.9059 10.96 01:08:36.65 +60:44:55.0
125.02962 -2.05317 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 | Gaia DR3 426363744241527552 | 01:08:34.66 +60:44:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8: 1935BSD...C01....0S BSD 8-1144
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:36.65 +60:44:55.0: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:36.65 +60:44:55.0: 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 22.4059* 01 08 36.65 +60 44 55.0 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
Gaia DR3 426363744241527552,2461213.9059,10.96,0.05,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 426363744241527552 20260622.4059 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 22.4059 2461213.9059 10.95 01:22:23.83 +61:13:51.2
126.64937 -1.41720 galactic Cas Second-epoch detections are separated by 2.3" and 7.5 pix
The object was found in VSX 0" 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 01:22:23.83 +61:13:51.2: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:23.83 +61:13:51.2: 15.71 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.71 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 22 23.83 +61 13 51.2 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
NSVS J0122238+611352,2461213.9059,10.95,0.05,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
NSVS J0122238+611352 20260622.4059 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 22.4059 2461213.9059 10.96 01:18:48.45 +64:12:21.9
125.90456 1.49242 galactic Cas Second-epoch detections are separated by 2.0" 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 | 01:18:48.45 +64:12:21.9 (user input) | T | P | (position from user input) J-Ks=0.908+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:48.45 +64:12:21.9: 11.70 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:48.45 +64:12:21.9: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 22.4059* 01 18 48.45 +64 12 21.9 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,2461213.9059,10.96,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.01 01:13:38.99 +58:10:51.5
125.86566 -4.56420 galactic Cas Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 01:13:38.99 +58:10:51.5: 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 01:13:38.99 +58:10:51.5: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 22.4059* 01 13 38.99 +58 10 51.5 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
ATO J018.4234+58.1762,2461213.9059,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J018.4234+58.1762 20260622.4059 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 22.4059 2461213.9059 11.10 01:51:26.62 +57:51:36.8
130.86704 -4.08408 galactic Per 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 | 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 01:51:26.62 +57:51:36.8: 12.81 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:26.62 +57:51:36.8: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 51 26.62 +57 51 36.8 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 506162862211871616,2461213.9059,11.10,0.05,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 506162862211871616 20260622.4059 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 22.4059 2461213.9059 11.09 01:09:22.73 +57:26:31.5
125.35444 -5.34525 galactic Cas Second-epoch detections are separated by 2.2" 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 | 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 01:09:22.73 +57:26:31.5: 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 01:09:22.73 +57:26:31.5: 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 22.4059* 01 09 22.73 +57 26 31.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.3204+57.4562,2461213.9059,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.3204+57.4562 20260622.4059 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.23 02:07:53.83 +58:37:40.5
132.75900 -2.77739 galactic Per 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 | Gaia DR3 506785185794584448 | 02:07:53.98 +58:37:02.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:53.83 +58:37:40.5: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:53.83 +58:37:40.5: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 02 07 53.83 +58 37 40.5 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 506785185794584448,2461213.9059,11.23,0.05,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
Gaia DR3 506785185794584448 20260622.4059 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 22.4059 2461213.9059 11.16 02:16:07.65 +58:18:13.6
133.88393 -2.75566 galactic Per Second-epoch detections are separated by 3.2" and 6.7 pix
The object was found in VSX 4" Gaia DR3 458762778499159168
Type: VAR
# Max. Min./Amp. JD0 Period
13.750 G 13.790 G 0.014923200000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:07.65 +58:18:13.6: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:07.65 +58:18:13.6: 13.76 +/- 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 22.4059* 02 16 07.65 +58 18 13.6 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 458762778499159168,2461213.9059,11.16,0.05,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 458762778499159168 20260622.4059 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 22.4059 2461213.9059 11.18 01:27:34.47 +57:48:26.0
127.74714 -4.72628 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 413087553653222272 | 01:27:32.01 +57:48:40.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.887+/-0.037 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:34.47 +57:48:26.0: 12.36 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:34.47 +57:48:26.0: 13.93 +/- 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 22.4059* 01 27 34.47 +57 48 26.0 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
Gaia DR3 413087553653222272,2461213.9059,11.18,0.05,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
Gaia DR3 413087553653222272 20260622.4059 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 22.4059 2461213.9059 11.19 02:15:10.49 +58:07:01.8
133.82473 -2.97262 galactic Per Second-epoch detections are separated by 0.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:15:10.49 +58:07:01.8: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:10.49 +58:07:01.8: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.91 +/- 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 22.4059* 02 15 10.49 +58 07 01.8 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
ATO J033.7918+58.1304,2461213.9059,11.19,0.05,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
ATO J033.7918+58.1304 20260622.4059 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 22.4059 2461213.9059 11.16 02:15:03.79 +58:28:54.1
133.69469 -2.63170 galactic Per Second-epoch detections are separated by 2.0" and 6.8 pix
The object was found in VSX 3" Gaia DR3 506806798067617152
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.780 G 13.810 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:03.79 +58:28:54.1: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:03.79 +58:28:54.1: 13.72 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 22.4059* 02 15 03.79 +58 28 54.1 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 506806798067617152,2461213.9059,11.16,0.05,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 506806798067617152 20260622.4059 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 22.4059 2461213.9059 11.07 01:20:13.79 +65:31:27.3
125.91121 2.81919 galactic Cas Second-epoch detections are separated by 3.3" and 7.7 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 01:20:13.79 +65:31:27.3: 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 01:20:13.79 +65:31:27.3: 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 22.4059* 01 20 13.79 +65 31 27.3 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
V0897 Cas,2461213.9059,11.07,0.05,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
V0897 Cas 20260622.4059 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 22.4059 2461213.9059 11.06 01:08:59.24 +60:47:20.7
125.07278 -2.00970 galactic Cas Second-epoch detections are separated by 1.3" 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 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 01:08:59.24 +60:47:20.7: 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 01:08:59.24 +60:47:20.7: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 22.4059* 01 08 59.24 +60 47 20.7 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 522440066710315904,2461213.9059,11.06,0.05,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 522440066710315904 20260622.4059 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 22.4059 2461213.9059 11.30 02:09:48.66 +59:05:18.0
132.85958 -2.26444 galactic Per Second-epoch detections are separated by 8.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J032.4647+59.0882 | 02:09:48.66 +59:05:18.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:48.66 +59:05:18.0: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:48.66 +59:05:18.0: 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 22.4059* 02 09 48.66 +59 05 18.0 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
ATO J032.4647+59.0882,2461213.9059,11.30,0.05,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
ATO J032.4647+59.0882 20260622.4059 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 22.4059 2461213.9059 11.20 01:50:39.89 +62:00:56.0
129.81921 -0.06162 galactic Cas Second-epoch detections are separated by 0.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 01:50:39.89 +62:00:56.0: 13.31 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:39.89 +62:00:56.0: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 50 39.89 +62 00 56.0 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
Gaia DR3 511356332360621440,2461213.9059,11.20,0.05,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 511356332360621440 20260622.4059 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 22.4059 2461213.9059 11.23 01:34:07.22 +60:12:52.5
128.21341 -2.21875 galactic Cas Second-epoch detections are separated by 1.7" 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 509777472336200448 | 01:34:01.93 +60:13:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0IV/V 1928MeUpp..37....1S BD+59 277 J-Ks=0.892+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:07.22 +60:12:52.5: 11.75 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:07.22 +60:12:52.5: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 22.4059* 01 34 07.22 +60 12 52.5 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 509777472336200448,2461213.9059,11.23,0.05,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
Gaia DR3 509777472336200448 20260622.4059 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 22.4059 2461213.9059 11.26 01:44:29.97 +65:09:24.4
128.47104 2.85725 galactic Cas Second-epoch detections are separated by 1.1" and 7.0 pix
The object was found in VSX 6" Gaia DR3 519045973088246784
Type: ROT
# Max. Min./Amp. JD0 Period
15.090 G 15.140 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:29.97 +65:09:24.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:29.97 +65:09:24.4: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 44 29.97 +65 09 24.4 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
Gaia DR3 519045973088246784,2461213.9059,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 519045973088246784 20260622.4059 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.23 02:13:40.28 +65:08:15.5
131.43945 3.63310 galactic Cas Second-epoch detections are separated by 2.0" 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 | 02:13:40.28 +65:08:15.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:40.28 +65:08:15.5: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:40.28 +65:08:15.5: 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 22.4059* 02 13 40.28 +65 08 15.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.23,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.26 01:59:34.07 +63:37:08.7
130.41379 1.74138 galactic Cas Second-epoch detections are separated by 3.1" 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 | 01:59:34.07 +63:37:08.7 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:34.07 +63:37:08.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:34.07 +63:37:08.7: 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 22.4059* 01 59 34.07 +63 37 08.7 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.36 02:08:50.69 +59:21:19.8
132.66209 -2.04602 galactic Cas Second-epoch detections are separated by 1.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:08:50.69 +59:21:19.8 (user input) | T | P | (position from user input) J-Ks=0.939+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:08:50.69 +59:21:19.8: 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 02:08:50.69 +59:21:19.8: 14.05 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 02 08 50.69 +59 21 19.8 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,2461213.9059,11.36,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.33 01:16:56.61 +59:03:13.9
126.21256 -3.65533 galactic Cas Second-epoch detections are separated by 1.9" and 7.0 pix
The object was found in VSX16" Gaia DR3 414191497686936448
Type: ROT
# Max. Min./Amp. JD0 Period
16.180 G 16.240 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:56.61 +59:03:13.9: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:56.61 +59:03:13.9: 14.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.26 +/- 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 22.4059* 01 16 56.61 +59 03 13.9 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 414191497686936448,2461213.9059,11.33,0.05,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 414191497686936448 20260622.4059 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 22.4059 2461213.9059 11.23 01:56:57.28 +63:00:32.6
130.28624 1.07659 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 | 01:56:57.28 +63:00:32.6 (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 01:56:57.28 +63:00:32.6: 13.26 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:57.28 +63:00:32.6: 13.97 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 56 57.28 +63 00 32.6 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,2461213.9059,11.23,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.24 01:09:58.01 +59:03:02.1
125.31735 -3.73532 galactic Cas Second-epoch detections are separated by 2.5" and 7.7 pix
The object was found in VSX11" ZTF J010958.46+590312.3
Type: EW
# Max. Min./Amp. JD0 Period
17.179 r Y 0.101 r 2458437.80700 0.323170200000
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 01:09:58.01 +59:03:02.1: 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 01:09:58.01 +59:03:02.1: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 09 58.01 +59 03 02.1 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
ZTF J010958.46+590312.3,2461213.9059,11.24,0.05,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
ZTF J010958.46+590312.3 20260622.4059 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 22.4059 2461213.9059 11.34 01:48:19.06 +59:38:19.2
130.07077 -2.44238 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 | 01:48:19.06 +59:38:19.2 (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 01:48:19.06 +59:38:19.2: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:19.06 +59:38:19.2: 13.97 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.97 +/- 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 22.4059* 01 48 19.06 +59 38 19.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.34,0.05,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 20260622.4059 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 22.4059 2461213.9059 11.44 02:02:11.53 +61:55:31.4
131.15314 0.18826 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 | target | 02:02:11.53 +61:55:31.4 (user input) | T | P | (position from user input) J-Ks=0.538+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:11.53 +61:55:31.4: 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 02:02:11.53 +61:55:31.4: 14.04 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.04 +/- 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 22.4059* 02 02 11.53 +61 55 31.4 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.43 01:33:30.54 +58:02:22.0
128.49305 -4.37732 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 J023.3712+58.0394 | 01:33:30.54 +58:02:22.0 (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 01:33:30.54 +58:02:22.0: 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 01:33:30.54 +58:02:22.0: 14.23 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 33 30.54 +58 02 22.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J023.3712+58.0394,2461213.9059,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J023.3712+58.0394 20260622.4059 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.42 01:52:07.07 +59:13:07.6
130.63694 -2.74219 galactic Cas Second-epoch detections are separated by 2.1" and 7.0 pix
The object was found in VSX 2" Gaia DR3 506523983061019904
Type: ROT
# Max. Min./Amp. JD0 Period
14.190 G 14.230 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:07.07 +59:13:07.6: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:07.07 +59:13:07.6: 14.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.22 +/- 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 22.4059* 01 52 07.07 +59 13 07.6 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
Gaia DR3 506523983061019904,2461213.9059,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506523983061019904 20260622.4059 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 22.4059 2461213.9059 11.30 01:51:53.53 +63:26:22.3
129.62884 1.35656 galactic Cas Second-epoch detections are separated by 3.9" and 6.8 pix
The object was found in VSX11" ZTF J015152.31+632614.6
Type: EB:
# Max. Min./Amp. JD0 Period
15.451 r Y 0.389 r 2458367.82620 5.408679200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:53.53 +63:26:22.3: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:53.53 +63:26:22.3: 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 22.4059* 01 51 53.53 +63 26 22.3 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J015152.31+632614.6,2461213.9059,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J015152.31+632614.6 20260622.4059 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 22.4059 2461213.9059 11.26 01:19:29.22 +59:25:22.7
126.49818 -3.25442 galactic Cas Second-epoch detections are separated by 3.2" 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 | Large-amplitude variable Gaia DR2 414042479505165696 | 01:19:30.78 +59:24:54.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G3 1935BSD...C01....0S BSD 8- 264 J-Ks=0.435+/-0.045 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:29.22 +59:25:22.7: 13.16 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:29.22 +59:25:22.7: 14.17 +/- 0.07 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 22.4059* 01 19 29.22 +59 25 22.7 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
Large-amplitude variable Gaia DR2 414042479505165696,2461213.9059,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 414042479505165696 20260622.4059 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.19 01:28:07.34 +59:53:51.6
127.52183 -2.64676 galactic Cas Second-epoch detections are separated by 2.8" 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 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 01:28:07.34 +59:53:51.6: 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 01:28:07.34 +59:53:51.6: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 28 07.34 +59 53 51.6 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 510182298766565376,2461213.9059,11.19,0.05,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 510182298766565376 20260622.4059 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 22.4059 2461213.9059 11.47 01:58:53.87 +61:23:25.6
130.91746 -0.43099 galactic Cas Second-epoch detections are separated by 1.5" 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 508631231454878592 | 01:58:49.24 +61:23:53.7 (Gaia DR3) | ROT (local) | K (local) | Gaia3var=NOT_AVAILABLE SpType: A2V 1928MeUpp..37....1S BD+60 401
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:53.87 +61:23:25.6: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:53.87 +61:23:25.6: 14.28 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.28 +/- 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 22.4059* 01 58 53.87 +61 23 25.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508631231454878592,2461213.9059,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508631231454878592 20260622.4059 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 22.4059 2461213.9059 11.34 02:03:41.72 +58:47:26.1
132.18901 -2.77640 galactic Per Second-epoch detections are separated by 1.4" and 6.9 pix
The object was found in VSX 3" Gaia DR3 507016151955253248
Type: ROT
# Max. Min./Amp. JD0 Period
13.920 G 13.940 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 02:03:41.72 +58:47:26.1: 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 02:03:41.72 +58:47:26.1: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 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 22.4059* 02 03 41.72 +58 47 26.1 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 507016151955253248,2461213.9059,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507016151955253248 20260622.4059 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 22.4059 2461213.9059 11.38 01:33:35.72 +60:32:28.6
128.09580 -1.90710 galactic Cas Second-epoch detections are separated by 3.6" and 7.4 pix
The object was found in VSX19" Gaia DR3 509837735009502592
Type: RS
# Max. Min./Amp. JD0 Period
16.590 G 16.690 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 01:33:35.72 +60:32:28.6: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:35.72 +60:32:28.6: 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 22.4059* 01 33 35.72 +60 32 28.6 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
Gaia DR3 509837735009502592,2461213.9059,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509837735009502592 20260622.4059 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.31 01:29:25.46 +60:01:31.9
127.66473 -2.49669 galactic Cas Second-epoch detections are separated by 2.6" 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 | 01:29:25.46 +60:01:31.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:25.46 +60:01:31.9: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:25.46 +60:01:31.9: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 29 25.46 +60 01 31.9 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.40 01:51:40.02 +60:56:16.7
130.18281 -1.08304 galactic Cas Second-epoch detections are separated by 3.0" 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 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 01:51:40.02 +60:56:16.7: 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 01:51:40.02 +60:56:16.7: 14.13 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.13 +/- 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 22.4059* 01 51 40.02 +60 56 16.7 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508195305151165312,2461213.9059,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508195305151165312 20260622.4059 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.48 02:02:23.72 +64:38:25.5
130.43929 2.80795 galactic Cas Second-epoch detections are separated by 7.8" and 6.8 pix
The object was found in VSX15" 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 02:02:23.72 +64:38:25.5: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:23.72 +64:38:25.5: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 02 02 23.72 +64 38 25.5 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
ASASSN-V J020225.96+643822.9,2461213.9059,11.48,0.05,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
ASASSN-V J020225.96+643822.9 20260622.4059 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 22.4059 2461213.9059 11.51 01:40:21.65 +60:37:45.8
128.89843 -1.67437 galactic Cas Second-epoch detections are separated by 3.5" and 7.4 pix
The object was found in VSX18" Gaia DR3 509712463706282368
Type: RS
# Max. Min./Amp. JD0 Period
17.290 G 17.410 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:21.65 +60:37:45.8: 12.57 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:21.65 +60:37:45.8: 14.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.03 +/- 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 22.4059* 01 40 21.65 +60 37 45.8 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 509712463706282368,2461213.9059,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509712463706282368 20260622.4059 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.40 01:19:11.81 +59:07:32.7
126.49352 -3.55390 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 414009562874273024 | 01:19:13.47 +59:07:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1935BSD...C01....0S BSD 8- 261 J-Ks=0.463+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:11.81 +59:07:32.7: 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 01:19:11.81 +59:07:32.7: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.12 +/- 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 22.4059* 01 19 11.81 +59 07 32.7 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414009562874273024,2461213.9059,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 414009562874273024 20260622.4059 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.56 02:12:20.59 +64:11:16.0
131.59965 2.68608 galactic Cas Second-epoch detections are separated by 4.2" and 7.2 pix
The object was found in VSX 3" Gaia DR3 515007539905053696
Type: ROT
# Max. Min./Amp. JD0 Period
14.490 G 14.520 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:12:20.59 +64:11:16.0: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:12:20.59 +64:11:16.0: 14.11 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.11 +/- 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 22.4059* 02 12 20.59 +64 11 16.0 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 515007539905053696,2461213.9059,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 515007539905053696 20260622.4059 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.43 02:03:33.12 +58:39:09.8
132.20921 -2.91404 galactic Per 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 | Gaia DR3 506962138444777472 | 02:03:27.85 +58:38:49.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1928MeUpp..37....1S BD+57 467 J-Ks=0.472+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:33.12 +58:39:09.8: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:33.12 +58:39:09.8: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.18 +/- 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 22.4059* 02 03 33.12 +58 39 09.8 11.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506962138444777472,2461213.9059,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506962138444777472 20260622.4059 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.51 01:30:50.88 +60:06:03.4
127.82920 -2.39554 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 | IL Cas | 01:30:46.78 +60:06:02.4 (Gaia DR3) | EA/SD (local) | 3.451726000000 (local) | Gaia3var=VARIABLE SpType: B5 1955ApJS....2..123F LF 5 +59 22
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:50.88 +60:06:03.4: 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 01:30:50.88 +60:06:03.4: 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 22.4059* 01 30 50.88 +60 06 03.4 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
IL Cas,2461213.9059,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IL Cas 20260622.4059 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.54 02:01:26.30 +59:44:32.4
131.65217 -1.93899 galactic Cas Second-epoch detections are separated by 2.5" 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 J030.3856+59.7500 | 02:01:28.88 +59:44:50.7 (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 02:01:26.30 +59:44:32.4: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:26.30 +59:44:32.4: 14.45 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.45 +/- 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 22.4059* 02 01 26.30 +59 44 32.4 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
ATO J030.3856+59.7500,2461213.9059,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J030.3856+59.7500 20260622.4059 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.47 01:55:15.25 +58:45:57.8
131.13803 -3.08521 galactic Cas Second-epoch detections are separated by 1.1" and 7.0 pix
The object was found in VSX 2" Gaia DR3 506265151151611264
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.350 G 14.390 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 01:55:15.25 +58:45:57.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:15.25 +58:45:57.8: 14.35 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.35 +/- 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 22.4059* 01 55 15.25 +58 45 57.8 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506265151151611264,2461213.9059,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506265151151611264 20260622.4059 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 22.4059 2461213.9059 11.47 01:24:36.31 +61:08:54.9
126.92363 -1.46585 galactic Cas Second-epoch detections are separated by 2.2" and 7.0 pix
The object was found in VSX 1" Gaia DR3 510685394056841344
Type: ROT
# Max. Min./Amp. JD0 Period
14.210 G 14.240 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 01:24:36.31 +61:08:54.9: 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 01:24:36.31 +61:08:54.9: 14.36 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 24 36.31 +61 08 54.9 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510685394056841344,2461213.9059,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510685394056841344 20260622.4059 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 22.4059 2461213.9059 11.51 01:38:40.39 +64:31:56.4
127.98387 2.12490 galactic Cas Second-epoch detections are separated by 2.6" and 7.3 pix
The object was found in VSX21" Gaia DR3 512964166264921856
Type: YSO
# Max. Min./Amp. JD0 Period
17.250 G 17.380 G M
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:40.39 +64:31:56.4: 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 01:38:40.39 +64:31:56.4: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 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 22.4059* 01 38 40.39 +64 31 56.4 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 512964166264921856,2461213.9059,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512964166264921856 20260622.4059 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.41 01:20:35.08 +64:02:26.5
126.11547 1.34926 galactic Cas Second-epoch detections are separated by 1.9" 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 | 01:20:35.08 +64:02:26.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:35.08 +64:02:26.5: 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 01:20:35.08 +64:02:26.5: 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 22.4059* 01 20 35.08 +64 02 26.5 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
target,2461213.9059,11.41,0.05,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
target 20260622.4059 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 22.4059 2461213.9059 11.54 01:26:06.00 +59:42:39.7
127.29550 -2.86673 galactic Cas Second-epoch detections are separated by 2.1" 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 | ATO J021.5213+59.7108 | 01:26:06.00 +59:42:39.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:06.00 +59:42:39.7: 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 01:26:06.00 +59:42:39.7: 14.51 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.51 +/- 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 22.4059* 01 26 06.00 +59 42 39.7 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 J021.5213+59.7108,2461213.9059,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.5213+59.7108 20260622.4059 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.48 01:22:13.58 +59:52:27.1
126.79090 -2.76667 galactic Cas Second-epoch detections are separated by 0.3" 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 | 01:22:13.58 +59:52:27.1 (user input) | T | P | (position from user input) J-Ks=1.005+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:13.58 +59:52:27.1: 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 01:22:13.58 +59:52:27.1: 14.34 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 22 13.58 +59 52 27.1 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 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 22.4059 2461213.9059 11.56 01:31:27.96 +63:36:57.8
127.36152 1.08909 galactic Cas Second-epoch detections are separated by 1.4" and 7.1 pix
The object was found in VSX15" Gaia DR3 512527174807047680
Type: ROT
# Max. Min./Amp. JD0 Period
17.410 G 17.510 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 01:31:27.96 +63:36:57.8: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:27.96 +63:36:57.8: 14.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.31 +/- 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 22.4059* 01 31 27.96 +63 36 57.8 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512527174807047680,2461213.9059,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512527174807047680 20260622.4059 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.66 01:29:38.33 +63:19:38.0
127.20348 0.77274 galactic Cas Second-epoch detections are separated by 2.7" and 7.4 pix
The object was found in VSX21" Gaia DR3 512422828587465216
Type: S
# Max. Min./Amp. JD0 Period
14.920 G 15.600 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 01:29:38.33 +63:19:38.0: 12.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:38.33 +63:19:38.0: 14.21 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.21 +/- 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 22.4059* 01 29 38.33 +63 19 38.0 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
Gaia DR3 512422828587465216,2461213.9059,11.66,0.05,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 512422828587465216 20260622.4059 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 22.4059 2461213.9059 11.63 01:38:11.93 +62:50:30.9
128.23869 0.45297 galactic Cas Second-epoch detections are separated by 0.5" 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 | Large-amplitude variable Gaia DR2 511677222261497344 | 01:38:16.26 +62:50:42.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F8 1960IzKry..24..160B [B60] +62 261 J-Ks=0.527+/-0.037 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:11.93 +62:50:30.9: 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 01:38:11.93 +62:50:30.9: 14.71 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.71 +/- 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 22.4059* 01 38 11.93 +62 50 30.9 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
Large-amplitude variable Gaia DR2 511677222261497344,2461213.9059,11.63,0.05,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
Large-amplitude variable Gaia DR2 511677222261497344 20260622.4059 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 22.4059 2461213.9059 11.80 01:40:28.70 +60:34:45.2
128.92207 -1.72091 galactic Cas Second-epoch detections are separated by 2.6" 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 | target | 01:40:28.70 +60:34:45.2 (user input) | T | P | (position from user input) J-Ks=0.851+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:28.70 +60:34:45.2: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:28.70 +60:34:45.2: 14.61 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 40 28.70 +60 34 45.2 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,2461213.9059,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 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 22.4059 2461213.9059 11.59 01:48:17.90 +60:40:25.2
129.84192 -1.43297 galactic Cas Second-epoch detections are separated by 2.8" and 7.2 pix
The object was found in VSX 9" Gaia DR3 511167701701981184
Type: ROT
# Max. Min./Amp. JD0 Period
17.690 G 17.800 G 10.278600000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:17.90 +60:40:25.2: 12.84 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:17.90 +60:40:25.2: 14.25 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 48 17.90 +60 40 25.2 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511167701701981184,2461213.9059,11.59,0.05,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 511167701701981184 20260622.4059 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 22.4059 2461213.9059 11.74 01:52:07.71 +59:52:59.5
130.48322 -2.09577 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 | Large-amplitude variable Gaia DR2 506579645838190208 | 01:52:03.18 +59:52:32.6 (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) SpType: B2 1953IzKry..10..120K [K53] 612
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:07.71 +59:52:59.5: 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 01:52:07.71 +59:52:59.5: 14.65 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.65 +/- 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 22.4059* 01 52 07.71 +59 52 59.5 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
Large-amplitude variable Gaia DR2 506579645838190208,2461213.9059,11.74,0.05,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
Large-amplitude variable Gaia DR2 506579645838190208 20260622.4059 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 22.4059 2461213.9059 11.85 01:34:06.34 +59:58:54.2
128.25004 -2.44872 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 | 01:34:06.34 +59:58:54.2 (user input) | T | P | (position from user input) J-Ks=0.739+/-0.037 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:06.34 +59:58:54.2: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:06.34 +59:58:54.2: 14.58 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.58 +/- 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 22.4059* 01 34 06.34 +59 58 54.2 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,2461213.9059,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.76 01:30:40.75 +59:33:48.0
127.89009 -2.93012 galactic Cas Second-epoch detections are separated by 0.7" 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 509406589006933504 | 01:30:37.97 +59:33:59.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.856+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:40.75 +59:33:48.0: 12.87 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:40.75 +59:33:48.0: 14.53 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.38 +/- 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 22.4059* 01 30 40.75 +59 33 48.0 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509406589006933504,2461213.9059,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509406589006933504 20260622.4059 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.79 01:45:17.16 +58:43:30.6
129.88591 -3.41764 galactic Cas Second-epoch detections are separated by 2.4" and 7.3 pix
The object was found in VSX 0" ZTF J014517.20+584330.3
Type: RS
# Max. Min./Amp. JD0 Period
14.603 r Y 0.045 r 2458303.97270 1.759127700000
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 01:45:17.16 +58:43:30.6: 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 01:45:17.16 +58:43:30.6: 14.90 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 45 17.16 +58 43 30.6 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
ZTF J014517.20+584330.3,2461213.9059,11.79,0.05,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
ZTF J014517.20+584330.3 20260622.4059 11.79CV 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 22.4059 2461213.9059 11.64 01:26:31.51 +60:49:34.2
127.19709 -1.75468 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 510666049518654720 | 01:26:28.07 +60:49:49.0 (Gaia DR3) | E (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.669+/-0.042 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:31.51 +60:49:34.2: 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 01:26:31.51 +60:49:34.2: 14.38 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.38 +/- 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 22.4059* 01 26 31.51 +60 49 34.2 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510666049518654720,2461213.9059,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510666049518654720 20260622.4059 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.78 02:16:01.71 +61:10:48.8
132.94730 -0.03583 galactic Cas Second-epoch detections are separated by 2.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:16:01.71 +61:10:48.8 (user input) | T | P | (position from user input) J-Ks=0.469+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:01.71 +61:10:48.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:01.71 +61:10:48.8: 14.65 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.65 +/- 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 22.4059* 02 16 01.71 +61 10 48.8 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.78 01:29:20.64 +60:14:12.4
127.62378 -2.28920 galactic Cas Second-epoch detections are separated by 2.4" and 7.4 pix
The object was found in VSX 2" Gaia DR3 510211470185631104
Type: ROT
# Max. Min./Amp. JD0 Period
14.650 G 14.670 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 01:29:20.64 +60:14:12.4: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:20.64 +60:14:12.4: 14.77 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.77 +/- 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 22.4059* 01 29 20.64 +60 14 12.4 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 510211470185631104,2461213.9059,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510211470185631104 20260622.4059 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.82 01:46:56.51 +61:34:41.2
129.48659 -0.58526 galactic Cas Second-epoch detections are separated by 3.3" 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 | target | 01:46:56.51 +61:34:41.2 (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 01:46:56.51 +61:34:41.2: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:56.51 +61:34:41.2: 14.64 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.64 +/- 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 22.4059* 01 46 56.51 +61 34 41.2 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,2461213.9059,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.73 01:39:55.66 +61:01:23.9
128.77257 -1.29737 galactic Cas Second-epoch detections are separated by 3.5" 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 509930888563480576 | 01:39:53.60 +61:01:54.8 (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 01:39:55.66 +61:01:23.9: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:55.66 +61:01:23.9: 14.69 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 39 55.66 +61 01 23.9 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509930888563480576,2461213.9059,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509930888563480576 20260622.4059 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.84 01:28:14.59 +60:19:20.9
127.47628 -2.22413 galactic Cas Second-epoch detections are separated by 2.3" and 7.5 pix
The object was found in VSX16" Gaia DR3 510216005670888320
Type: ROT
# Max. Min./Amp. JD0 Period
17.120 G 17.200 G 3.707550000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:14.59 +60:19:20.9: 13.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:14.59 +60:19:20.9: 14.70 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.70 +/- 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 22.4059* 01 28 14.59 +60 19 20.9 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 510216005670888320,2461213.9059,11.84,0.05,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
Gaia DR3 510216005670888320 20260622.4059 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 22.4059 2461213.9059 11.97 02:02:05.39 +62:09:27.7
131.07882 0.40869 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 | 02:02:05.39 +62:09:27.7 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.045 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:05.39 +62:09:27.7: 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 02:02:05.39 +62:09:27.7: 14.86 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.86 +/- 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 22.4059* 02 02 05.39 +62 09 27.7 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,2461213.9059,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.97 01:35:45.28 +61:18:34.4
128.22621 -1.10582 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 | 01:35:45.28 +61:18:34.4 (user input) | T | P | (position from user input) J-Ks=0.248+/-0.046 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:45.28 +61:18:34.4: 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 01:35:45.28 +61:18:34.4: 14.76 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.76 +/- 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 22.4059* 01 35 45.28 +61 18 34.4 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.81 01:23:32.35 +60:58:47.9
126.81699 -1.64940 galactic Cas Second-epoch detections are separated by 2.9" 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 | 01:23:32.35 +60:58:47.9 (user input) | T | P | (position from user input) J-Ks=0.262+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:32.35 +60:58:47.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:32.35 +60:58:47.9: 15.03 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.03 +/- 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 22.4059* 01 23 32.35 +60 58 47.9 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.88 01:06:45.13 +60:27:55.0
124.81974 -2.35032 galactic Cas Second-epoch detections are separated by 1.5" 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 | target | 01:06:45.13 +60:27:55.0 (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 01:06:45.13 +60:27:55.0: 12.05 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:45.13 +60:27:55.0: 14.86 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.34 +/- 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 22.4059* 01 06 45.13 +60 27 55.0 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.78 01:36:46.33 +61:14:49.6
128.35744 -1.14617 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 | ASASSN-V J013643.22+611426.0 | 01:36:43.22 +61:14:25.9 (Gaia DR3) | L (local) | (local) | Gaia3var=VARIABLE J-Ks=0.401+/-0.045 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:46.33 +61:14:49.6: 12.65 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:46.33 +61:14:49.6: 14.92 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.25 +/- 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 22.4059* 01 36 46.33 +61 14 49.6 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
ASASSN-V J013643.22+611426.0,2461213.9059,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J013643.22+611426.0 20260622.4059 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.03 01:26:22.35 +61:16:28.9
127.11799 -1.31279 galactic Cas Second-epoch detections are separated by 1.4" and 7.2 pix
The object was found in VSX 2" Gaia DR3 510682198601256192
Type: RS
# Max. Min./Amp. JD0 Period
14.670 G 14.770 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:22.35 +61:16:28.9: 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 01:26:22.35 +61:16:28.9: 14.55 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.55 +/- 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 22.4059* 01 26 22.35 +61 16 28.9 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510682198601256192,2461213.9059,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510682198601256192 20260622.4059 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.13 01:41:15.07 +58:14:31.5
129.46500 -3.99640 galactic Cas Second-epoch detections are separated by 2.9" and 7.4 pix
The object was found in VSX25" Gaia DR3 506046348338018816
Type: ROT
# Max. Min./Amp. JD0 Period
15.760 G 15.800 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 01:41:15.07 +58:14:31.5: 12.86 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:15.07 +58:14:31.5: 14.83 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.56 +/- 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 22.4059* 01 41 15.07 +58 14 31.5 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506046348338018816,2461213.9059,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506046348338018816 20260622.4059 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.07 01:35:58.99 +57:43:50.5
128.87016 -4.62655 galactic Cas Second-epoch detections are separated by 1.0" and 7.1 pix
The object was found in VSX17" Gaia DR3 508928919924180992
Type: ROT
# Max. Min./Amp. JD0 Period
18.000 G 18.140 G 0.628680000000
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 01:35:58.99 +57:43:50.5: 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 01:35:58.99 +57:43:50.5: 14.82 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.82 +/- 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 22.4059* 01 35 58.99 +57 43 50.5 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508928919924180992,2461213.9059,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508928919924180992 20260622.4059 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.11 01:50:26.85 +59:20:13.4
130.40186 -2.67616 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 | target | 01:50:26.85 +59:20:13.4 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:26.85 +59:20:13.4: 13.08 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:26.85 +59:20:13.4: 15.20 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.74 +/- 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 22.4059* 01 50 26.85 +59 20 13.4 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.05 01:19:47.70 +60:24:29.9
126.42870 -2.27077 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 | 01:19:47.70 +60:24:29.9 (user input) | T | P | (position from user input) J-Ks=0.814+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:47.70 +60:24:29.9: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:47.70 +60:24:29.9: 15.19 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 19 47.70 +60 24 29.9 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.00 01:29:04.61 +62:34:45.2
127.24994 0.02345 galactic Cas Second-epoch detections are separated by 3.5" 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 | target | 01:29:04.61 +62:34:45.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:04.61 +62:34:45.2: 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 01:29:04.61 +62:34:45.2: 15.00 +/- 0.12 detection
Forced photometry reference-image weighted average: 15.00 +/- 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 22.4059* 01 29 04.61 +62 34 45.2 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,2461213.9059,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.01 01:58:37.12 +63:40:15.0
130.29858 1.76408 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 | 01:58:37.12 +63:40:15.0 (user input) | T | P | (position from user input) J-Ks=0.597+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:37.12 +63:40:15.0: 13.17 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:37.12 +63:40:15.0: 15.19 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.66 +/- 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 22.4059* 01 58 37.12 +63 40 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,2461213.9059,12.01,0.05,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 20260622.4059 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
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.98 01:43:25.66 +58:49:24.8
129.62961 -3.37047 galactic Cas Second-epoch detections are separated by 3.1" 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 | target | 01:43:25.66 +58:49:24.8 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.048 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:25.66 +58:49:24.8: 12.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:25.66 +58:49:24.8: 14.86 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.86 +/- 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 22.4059* 01 43 25.66 +58 49 24.8 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,2461213.9059,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.04 01:50:50.64 +59:17:02.3
130.46327 -2.71633 galactic Cas Second-epoch detections are separated by 0.4" 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 | 01:50:50.64 +59:17:02.3 (user input) | T | P | (position from user input) J-Ks=0.433+/- (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:50.64 +59:17:02.3: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:50.64 +59:17:02.3: 14.92 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.92 +/- 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 22.4059* 01 50 50.64 +59 17 02.3 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,2461213.9059,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 12.04CV 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 22.4059 2461213.9059 11.89 01:49:52.71 +58:55:20.4
130.42445 -3.09665 galactic Cas Second-epoch detections are separated by 1.9" 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 | Gaia DR3 506423137227824256 | 01:49:47.89 +58:55:04.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B3 1955ApJS....2..123F LF 5 +58 99 J-Ks=0.379+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:52.71 +58:55:20.4: 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 01:49:52.71 +58:55:20.4: 14.69 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.69 +/- 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 22.4059* 01 49 52.71 +58 55 20.4 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506423137227824256,2461213.9059,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506423137227824256 20260622.4059 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.10 01:53:43.15 +60:08:00.1
130.61741 -1.80575 galactic Cas Second-epoch detections are separated by 2.9" and 7.2 pix
The object was found in VSX21" Gaia DR3 508077696070172544
Type: ROT
# Max. Min./Amp. JD0 Period
17.450 G 17.570 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 01:53:43.15 +60:08:00.1: 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 01:53:43.15 +60:08:00.1: 15.07 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 53 43.15 +60 08 00.1 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508077696070172544,2461213.9059,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508077696070172544 20260622.4059 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.91 01:13:10.72 +58:11:20.8
125.80289 -4.56139 galactic Cas Second-epoch detections are separated by 2.2" 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 | 01:13:10.72 +58:11:20.8 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.042 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:10.72 +58:11:20.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:10.72 +58:11:20.8: 14.66 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.66 +/- 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 22.4059* 01 13 10.72 +58 11 20.8 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.04 01:34:20.25 +61:27:01.2
128.03520 -0.99562 galactic Cas Second-epoch detections are separated by 4.0" and 7.5 pix
The object was found in VSX23" ZTF J013417.04+612659.0
Type: EW
# Max. Min./Amp. JD0 Period
17.851 r Y 0.474 r 2458373.95840 0.321714400000
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 01:34:20.25 +61:27:01.2: 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 01:34:20.25 +61:27:01.2: 15.16 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.16 +/- 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 22.4059* 01 34 20.25 +61 27 01.2 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
ZTF J013417.04+612659.0,2461213.9059,12.04,0.05,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
ZTF J013417.04+612659.0 20260622.4059 12.04CV 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 22.4059 2461213.9059 11.98 01:44:25.02 +65:16:03.2
128.43990 2.96392 galactic Cas Second-epoch detections are separated by 0.3" 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 | 01:44:25.02 +65:16:03.2 (user input) | T | P | (position from user input) J-Ks=0.779+/-0.042 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:25.02 +65:16:03.2: 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 01:44:25.02 +65:16:03.2: 14.88 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.88 +/- 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 22.4059* 01 44 25.02 +65 16 03.2 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,2461213.9059,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.13 01:45:29.06 +58:26:32.6
129.97016 -3.68886 galactic Cas Second-epoch detections are separated by 1.5" and 7.0 pix
The object was found in VSX19" Gaia DR3 506066341403845888
Type: ROT
# Max. Min./Amp. JD0 Period
17.390 G 17.490 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 01:45:29.06 +58:26:32.6: 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 01:45:29.06 +58:26:32.6: 14.92 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.92 +/- 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 22.4059* 01 45 29.06 +58 26 32.6 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506066341403845888,2461213.9059,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506066341403845888 20260622.4059 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.89 01:37:48.39 +58:09:09.1
129.03463 -4.16874 galactic Cas Second-epoch detections are separated by 2.2" 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 | target | 01:37:48.39 +58:09:09.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.814+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:48.39 +58:09:09.1: 12.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:48.39 +58:09:09.1: 14.85 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.85 +/- 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 22.4059* 01 37 48.39 +58 09 09.1 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.02 01:39:27.36 +60:45:14.3
128.76631 -1.57268 galactic Cas Second-epoch detections are separated by 2.4" 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 | 01:39:27.36 +60:45:14.3 (user input) | T | P | (position from user input) J-Ks=0.626+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:27.36 +60:45:14.3: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:27.36 +60:45:14.3: 14.98 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 39 27.36 +60 45 14.3 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,2461213.9059,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 12.02CV 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 22.4059 2461213.9059 12.08 01:46:48.64 +58:27:31.2
130.13667 -3.63637 galactic Cas Second-epoch detections are separated by 1.2" 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 | ATO J026.7072+58.4617 | 01:46:48.64 +58:27:31.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.249+/-0.057 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:48.64 +58:27:31.2: 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 01:46:48.64 +58:27:31.2: 14.86 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.86 +/- 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 22.4059* 01 46 48.64 +58 27 31.2 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.7072+58.4617,2461213.9059,12.08,0.05,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
ATO J026.7072+58.4617 20260622.4059 12.08CV 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 22.4059 2461213.9059 12.01 01:35:59.51 +63:11:54.3
127.92948 0.75980 galactic Cas Second-epoch detections are separated by 2.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:35:59.51 +63:11:54.3 (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 01:35:59.51 +63:11:54.3: 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 01:35:59.51 +63:11:54.3: 14.61 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.61 +/- 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 22.4059* 01 35 59.51 +63 11 54.3 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,2461213.9059,12.01,0.05,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 20260622.4059 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
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.89 01:06:52.62 +62:05:00.8
124.73808 -0.73404 galactic Cas Second-epoch detections are separated by 3.3" 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 | Gaia DR3 522654913849839616 | 01:06:53.41 +62:05:24.4 (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 01:06:52.62 +62:05:00.8: 12.84 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:52.62 +62:05:00.8: 14.93 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.45 +/- 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 22.4059* 01 06 52.62 +62 05 00.8 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522654913849839616,2461213.9059,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522654913849839616 20260622.4059 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.18 02:13:53.24 +65:54:40.5
131.21748 4.37468 galactic Cas Second-epoch detections are separated by 4.6" 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 | 02:13:53.24 +65:54:40.5 (user input) | T | P | (position from user input) J-Ks=0.588+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:53.24 +65:54:40.5: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:53.24 +65:54:40.5: 15.19 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 02 13 53.24 +65 54 40.5 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,12.18,0.05,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 20260622.4059 12.18CV 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 22.4059 2461213.9059 12.01 01:19:21.39 +58:01:15.4
126.63402 -4.64998 galactic Cas Second-epoch detections are separated by 1.4" and 7.3 pix
The object was found in VSX23" Gaia DR3 413800960599944192
Type: E
# Max. Min./Amp. JD0 Period
18.330 G 18.540 G 0.371432000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:21.39 +58:01:15.4: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:21.39 +58:01:15.4: 15.13 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.13 +/- 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 22.4059* 01 19 21.39 +58 01 15.4 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413800960599944192,2461213.9059,12.01,0.05,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
Gaia DR3 413800960599944192 20260622.4059 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
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.07 01:43:56.14 +58:56:40.5
129.66958 -3.23870 galactic Cas Second-epoch detections are separated by 2.0" 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 | 01:43:56.14 +58:56:40.5 (user input) | T | P | (position from user input) J-Ks=0.676+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:56.14 +58:56:40.5: 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 01:43:56.14 +58:56:40.5: 15.00 +/- 0.13 detection
Forced photometry reference-image weighted average: 15.00 +/- 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 22.4059* 01 43 56.14 +58 56 40.5 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.98 01:35:02.55 +59:41:35.0
128.41436 -2.71373 galactic Cas Second-epoch detections are separated by 4.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J023.7880+59.6915 | 01:35:06.83 +59:41:35.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B3 1955ApJS....2..123F LF 5 +59 73 J-Ks=0.543+/-0.041 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:02.55 +59:41:35.0: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:02.55 +59:41:35.0: 14.93 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.93 +/- 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 22.4059* 01 35 02.55 +59 41 35.0 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
ATO J023.7880+59.6915,2461213.9059,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J023.7880+59.6915 20260622.4059 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.12 01:55:15.49 +59:42:12.6
130.90870 -2.17619 galactic Cas Second-epoch detections are separated by 3.9" and 6.9 pix
The object was found in VSX10" Gaia DR3 507875454651402112
Type: RS
# Max. Min./Amp. JD0 Period
15.630 G 15.730 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:15.49 +59:42:12.6: 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 01:55:15.49 +59:42:12.6: 15.33 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 55 15.49 +59 42 12.6 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507875454651402112,2461213.9059,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507875454651402112 20260622.4059 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.07 02:14:12.40 +65:14:53.8
131.45804 3.75577 galactic Cas Second-epoch detections are separated by 2.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:14:12.40 +65:14:53.8 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:12.40 +65:14:53.8: 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 02:14:12.40 +65:14:53.8: 15.29 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.29 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 02 14 12.40 +65 14 53.8 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.12 01:37:59.09 +61:09:38.8
128.51650 -1.20525 galactic Cas Second-epoch detections are separated by 3.3" and 7.3 pix
The object was found in VSX14" ZTF J013800.68+610930.8
Type: BY
# Max. Min./Amp. JD0 Period
16.387 r Y 0.050 r 2458380.95440 3.449227200000
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 01:37:59.09 +61:09:38.8: 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 01:37:59.09 +61:09:38.8: 14.83 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 37 59.09 +61 09 38.8 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J013800.68+610930.8,2461213.9059,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J013800.68+610930.8 20260622.4059 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.10 01:37:09.63 +60:59:35.3
128.44824 -1.38796 galactic Cas Second-epoch detections are separated by 3.9" 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 509923673016595328 | 01:37:09.81 +61:00:08.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1955ApJS....2..123F LF 5 +60 112
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:09.63 +60:59:35.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:09.63 +60:59:35.3: 14.99 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.99 +/- 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 22.4059* 01 37 09.63 +60 59 35.3 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509923673016595328,2461213.9059,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509923673016595328 20260622.4059 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.21 01:45:00.46 +59:26:56.3
129.70087 -2.71691 galactic Cas Second-epoch detections are separated by 0.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:45:00.46 +59:26:56.3 (user input) | T | P | (position from user input) J-Ks=0.729+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:00.46 +59:26:56.3: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:00.46 +59:26:56.3: 15.13 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 45 00.46 +59 26 56.3 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,12.21,0.05,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 20260622.4059 12.21CV 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 22.4059 2461213.9059 12.21 01:45:40.34 +59:47:00.0
129.71369 -2.37238 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 | ATO J026.4197+59.7850 | 01:45:40.34 +59:47:00.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.516+/-0.038 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:40.34 +59:47:00.0: 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 01:45:40.34 +59:47:00.0: 14.91 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.91 +/- 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 22.4059* 01 45 40.34 +59 47 00.0 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.4197+59.7850,2461213.9059,12.21,0.05,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
ATO J026.4197+59.7850 20260622.4059 12.21CV 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 22.4059 2461213.9059 12.18 01:12:27.12 +58:01:05.5
125.72118 -4.73970 galactic Cas Second-epoch detections are separated by 1.0" 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 | 01:12:27.12 +58:01:05.5 (user input) | T | P | (position from user input) J-Ks=0.519+/-0.038 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:27.12 +58:01:05.5: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:27.12 +58:01:05.5: 14.91 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.91 +/- 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 22.4059* 01 12 27.12 +58 01 05.5 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,12.18,0.05,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 20260622.4059 12.18CV 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 22.4059 2461213.9059 12.05 01:31:49.85 +62:50:13.0
127.52316 0.32583 galactic Cas Second-epoch detections are separated by 4.2" 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 512392003595889024 | 01:31:45.91 +62:50:37.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.865+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:49.85 +62:50:13.0: 12.95 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:49.85 +62:50:13.0: 14.81 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.52 +/- 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 22.4059* 01 31 49.85 +62 50 13.0 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512392003595889024,2461213.9059,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512392003595889024 20260622.4059 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 11.86 01:07:40.29 +57:36:50.0
125.11333 -5.18909 galactic Cas Second-epoch detections are separated by 2.6" 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 | 01:07:40.29 +57:36:50.0 (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 01:07:40.29 +57:36:50.0: 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 01:07:40.29 +57:36:50.0: 14.93 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.93 +/- 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 22.4059* 01 07 40.29 +57 36 50.0 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.18 01:37:28.98 +61:17:47.1
128.43284 -1.08258 galactic Cas Second-epoch detections are separated by 2.7" and 7.3 pix
The object was found in VSX24" Gaia DR3 509952810076161152
Type: E
# Max. Min./Amp. JD0 Period
17.170 G 17.690 G 2.913730000000
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 01:37:28.98 +61:17:47.1: 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 01:37:28.98 +61:17:47.1: 15.13 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 22.4059* 01 37 28.98 +61 17 47.1 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509952810076161152,2461213.9059,12.18,0.05,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
Gaia DR3 509952810076161152 20260622.4059 12.18CV 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 22.4059 2461213.9059 12.06 01:45:06.92 +57:56:34.9
130.02647 -4.18743 galactic Cas Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 505979690443920000 | 01:45:01.30 +57:56:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9IV/V 1928MeUpp..37....1S BD+57 380 J-Ks=0.403+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:06.92 +57:56:34.9: 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 01:45:06.92 +57:56:34.9: 14.53 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.53 +/- 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 22.4059* 01 45 06.92 +57 56 34.9 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505979690443920000,2461213.9059,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505979690443920000 20260622.4059 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.05 01:07:57.66 +60:18:17.7
124.97885 -2.50115 galactic Cas Second-epoch detections are separated by 2.3" 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 | 01:07:57.66 +60:18:17.7 (user input) | T | P | (position from user input) J-Ks=0.469+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:57.66 +60:18:17.7: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:57.66 +60:18:17.7: 14.91 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.91 +/- 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 22.4059* 01 07 57.66 +60 18 17.7 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.13 01:22:24.79 +62:39:02.2
126.48099 -0.00750 galactic Cas Second-epoch detections are separated by 3.7" 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 | 01:22:24.79 +62:39:02.2 (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 01:22:24.79 +62:39:02.2: 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 01:22:24.79 +62:39:02.2: 15.25 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.25 +/- 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 22.4059* 01 22 24.79 +62 39 02.2 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 22.4059 2461213.9059 12.21 01:17:35.37 +59:21:38.7
126.26415 -3.34169 galactic Cas Second-epoch detections are separated by 5.1" and 8.1 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 | 01:17:35.37 +59:21:38.7 (user input) | T | P | (position from user input) J-Ks=0.968+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:35.37 +59:21:38.7: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:35.37 +59:21:38.7: 14.91 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.91 +/- 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 22.4059* 01 17 35.37 +59 21 38.7 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461213.9059,12.21,0.05,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 20260622.4059 12.21CV 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 22.4059 2461213.9059 12.38 01:22:54.68 +58:55:22.5
126.99259 -3.70046 galactic Cas Second-epoch detections are separated by 6.8" and 8.1 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 | 01:22:54.68 +58:55:22.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:54.68 +58:55:22.5: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:54.68 +58:55:22.5: 15.15 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.15 +/- 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 22.4059* 01 22 54.68 +58 55 22.5 12.4 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,2461213.9059,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260622.4059 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461213.90621714 22.06.2026 09:44:47.161 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 12
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: 14 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): 26891
Objects passed selection criteria: 26778
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 20758.8
Average stars matched: 18953.5 (91.3037 %)
Memory usage VmPeak: 128420 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 Mon Jun 22 05:51:40 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: 2461213.90621714 22.06.2026 09:44:47.161 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 404
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: 273 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): 197994
Objects passed selection criteria: 197451
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 158224
Average stars matched: 144471 (91.3079 %)
Memory usage VmPeak: 1956400 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 Mon Jun 22 06:00:25 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_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.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_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.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: 2461213.90560589
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_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits'
wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.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_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:43:38.994 +61:58:33.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:43:38.994 +61:58:33.14
Angular distance between the image centers 0.1379 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:43:38.466 +61:59:15.40 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:43:38.466 +61:59:15.40
Angular distance between the image centers 0.1366 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:43:38.994 +61:58:33.14
Second-epoch second image center 01:43:38.466 +61:59:15.40
Angular distance between the image centers 0.01178 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.Y0zZDARhlM
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.xcZJXG10Nz
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_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits &> /tmp/tmp.mdjihemyMP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits &> /tmp/tmp.9Pxrxl86Z3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.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 9 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_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.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
14.9 mag. fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
14.9 mag. fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Y0zZDARhlM (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_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/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.xcZJXG10Nz (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_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/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.mdjihemyMP (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_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.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_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.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_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.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=2174, bad_region=5211, passed=23578
Got 23578 stars (including 16614 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits.wcscat
util/solve_plate_with_UCAC5 got 23578 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 to 67.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 18924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 55.8 to 67.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 18925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 18925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits N_match=972 sigma_overall_arcsec=0.494 sigma_q1_arcsec=0.481 sigma_q2_arcsec=0.415 sigma_q3_arcsec=0.566 sigma_q4_arcsec=0.446 n_q1=321 n_q2=281 n_q3=250 n_q4=120 worst_quadrant_to_overall_ratio=1.145
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.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.9Pxrxl86Z3 (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_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.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_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.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_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.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=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2239, bad_region=5202, passed=23420
Got 23420 stars (including 16416 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits.wcscat
util/solve_plate_with_UCAC5 got 23420 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 18726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 18727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 18727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits N_match=972 sigma_overall_arcsec=0.520 sigma_q1_arcsec=0.502 sigma_q2_arcsec=0.446 sigma_q3_arcsec=0.647 sigma_q4_arcsec=0.472 n_q1=321 n_q2=283 n_q3=253 n_q4=115 worst_quadrant_to_overall_ratio=1.244
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.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_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits sigma_overall=0.494 worst_q_ratio=1.145
new2=fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits sigma_overall=0.520 worst_q_ratio=1.244
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_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444_astrometric_residuals.png (972 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445_astrometric_residuals.png (972 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-43-54_20.00sec_5.00C_LIGHT_0444.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Cas-03-Q2b1x1_045022_TTUQ2b1x1_4103664_v2Le4Qm4/wcs_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445.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 02:09:11.31 +58:01:03.0: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:55.22 +62:38:07.5: 13.72 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:06.22 +59:12:12.1: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:41.87 +62:13:41.4: 14.96 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.06 +59:12:14.2: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.03 +59:15:34.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:55.22 +62:38:07.5: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:41.87 +62:13:41.4: 12.29 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 01:48:55.22 +62:38:07.5: ref_mag=12.42 +/- 0.01 new_mean_mag=12.2692 delta=0.15 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:38.06 +59:12:14.2: 11.99 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:06.22 +59:12:12.1: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter REJECTED candidate at 01:57:41.87 +62:13:41.4: ref_mag=12.31 +/- 0.01 new_mean_mag=12.2110 delta=0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:11.31 +58:01:03.0: 10.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry filter REJECTED candidate at 02:13:06.22 +59:12:12.1: ref_mag=12.28 +/- 0.01 new_mean_mag=12.2533 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry reference-image weighted average: 10.60 +/- 0.00
Forced photometry filter REJECTED candidate at 01:46:38.06 +59:12:14.2: ref_mag=11.99 +/- 0.01 new_mean_mag=12.0920 delta=-0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:09:11.31 +58:01:03.0: ref_mag=10.60 +/- 0.00 new_mean_mag=10.8340 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.03 +59:15:34.2: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter KEPT candidate at 01:56:38.03 +59:15:34.2: ref_mag=9.75 +/- 0.00 new_mean_mag=8.7752 delta=0.98 (need > 0.90)
Adding exclusion_list_local.txt__out20109.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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 51604_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 51604_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
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Considering the candidate 51606_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 51606_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
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Considering the candidate 54660_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 54660_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:46:08.65 +61:12:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55940_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 55940_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
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Considering the candidate 56062_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 56062_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
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Considering the candidate 56304_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 56304_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
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Considering the candidate 56423_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 56423_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:47:55.73 +64:32:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 08339_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
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Considering the candidate 247679_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247679_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247680_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247680_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247694_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247694_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247714_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247714_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247723_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247723_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247725_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247725_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247728_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247728_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247737_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247737_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247742_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 247742_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 247750_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247750_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247752_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247752_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247754_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247754_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247758_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247758_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247764_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247764_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247767_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247767_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247770_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247770_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247771_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247771_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247780_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247780_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247785_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247785_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247787_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247787_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247804_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247804_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247806_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247806_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247807_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247807_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247808_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247808_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247809_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247809_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247811_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 247811_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
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Considering the candidate 247813_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247813_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247814_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247814_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247816_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247816_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247822_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247822_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247823_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247823_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247828_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247828_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247829_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247829_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247833_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247833_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247834_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247834_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 247840_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247840_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247841_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247841_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247847_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247847_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247848_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 247848_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:09:23.28 +61:36:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247849_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247849_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247850_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247850_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247858_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 247858_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247859_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247859_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247866_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247866_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247868_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247868_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247869_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247869_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247870_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247870_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247881_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247881_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247887_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247887_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247890_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247890_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247891_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247891_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247895_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247895_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247897_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247897_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247900_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 247900_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:46:32.06 +57:52:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247901_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247901_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247902_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247902_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247909_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 247909_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:10:09.81 +59:33:19.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247910_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247910_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247915_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247915_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247917_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247917_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247919_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247919_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247921_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247921_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247925_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247925_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247928_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247928_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247931_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247931_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247932_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247932_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247933_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247933_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247935_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247935_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247937_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247937_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247940_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247940_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247951_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247951_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247956_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247956_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247959_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247959_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247964_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247964_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247966_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 247966_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:39:59.22 +60:24:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247967_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247967_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247968_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247968_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247970_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 247970_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247971_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247971_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247972_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247972_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247973_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247973_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247975_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247975_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247977_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247977_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247982_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247982_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247983_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 247983_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:33:01.68 +59:16:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247984_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247984_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247989_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247989_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247990_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 247990_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:07:35.03 +57:33:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247991_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 247991_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:14:01.31 +57:40:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247994_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 247994_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247996_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 247996_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:00:46.21 +57:54:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248002_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 248002_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248006_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 248006_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248010_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248010_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:33:35.34 +59:56:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248012_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248012_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:51:39.94 +58:29:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248013_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248013_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:58:54.89 +58:10:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248016_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248016_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:27:01.40 +61:22:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248018_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248018_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:54:45.35 +57:45:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248027_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248027_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 248028_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 248028_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248029_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248029_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:37:09.94 +58:51:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248030_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248030_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:05:57.27 +63:03:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248031_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248031_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:07:34.05 +60:52:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248034_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248034_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
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Considering the candidate 248037_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248037_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:19:24.10 +58:26:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248042_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248042_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:10:37.54 +57:22:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248045_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248045_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:03:21.68 +57:48:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248047_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248047_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:14:45.16 +60:30:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248048_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248048_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:07:08.07 +57:44:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248051_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248051_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:12:41.00 +61:20:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248053_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 248053_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 248054_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248054_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:25:26.59 +60:57:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248059_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248059_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:15:16.82 +57:28:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248060_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248060_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:55:14.55 +59:32:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248061_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248061_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:43:59.19 +61:55:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248062_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248062_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:20:24.31 +59:10:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248063_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248063_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:15:30.59 +63:53:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248064_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248064_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:19:48.73 +61:38:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248068_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248068_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:51:35.74 +57:52:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248071_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 248071_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:47:13.11 +57:44:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251269_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 251269_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:44:02.06 +61:53:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251498_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 251498_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:28:00.44 +61:19:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251799_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 251799_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:46:30.15 +61:12:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252005_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 252005_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:38:00.47 +57:56:46.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252268_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 252268_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:19:11.13 +58:20:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253987_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 253987_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:26:41.04 +60:46:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254437_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 254437_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:28:15.43 +58:44:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255693_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 255693_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:18:14.17 +61:44:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255972_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 255972_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:43:53.04 +61:53:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256192_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 256192_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 256273_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 256273_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:44:17.71 +61:53:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256323_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 256323_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:16:08.63 +58:49:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256438_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 256438_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:20:10.93 +58:12:09.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256891_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 256891_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:15:58.91 +63:12:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257107_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 257107_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:44:32.39 +58:45:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257219_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 257219_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:11:23.11 +61:21:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257503_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 257503_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:23:23.53 +63:36:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258108_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 258108_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:00:36.71 +58:30:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258514_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 258514_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:13:30.24 +58:34:25.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259048_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 259048_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:19:03.83 +63:57:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259803_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 259803_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
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Considering the candidate 260005_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 260005_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:10:23.83 +60:01:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260042_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 260042_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:43:07.01 +58:57:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260322_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 260322_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:13:36.00 +57:52:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260398_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 260398_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:35:50.59 +61:27:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260608_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 260608_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:16:05.15 +58:49:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260718_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 260718_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:58:04.13 +57:58:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260726_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 260726_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:26:35.97 +57:57:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260902_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 260902_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:29:32.89 +63:19:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260956_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 260956_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:08:30.50 +58:24:17.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 261203_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 261203_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:01:15.10 +59:23:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261789_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 261789_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:02:53.99 +60:15:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261842_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 261842_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:14:29.80 +63:16:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261881_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 261881_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:11:35.93 +57:37:13.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262556_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 262556_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:38:12.06 +61:01:26.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262573_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 262573_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:54:30.32 +59:06:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263065_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 263065_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:38:33.81 +60:47:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263248_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 263248_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:14:00.31 +61:42:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263530_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 263530_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263802_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 263802_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:19:12.09 +65:36:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264047_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 264047_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264156_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 264156_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:43:12.79 +64:00:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264159_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 264159_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264165_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 264165_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:18:04.11 +65:36:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264170_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 264170_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:59:06.06 +59:55:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264258_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 264258_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264273_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 264273_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264282_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 264282_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:42:54.84 +64:01:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264318_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 264318_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:43:03.30 +58:57:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264608_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 264608_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264850_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 264850_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:46:18.43 +60:59:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264998_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 264998_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:56:15.90 +60:00:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265387_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 265387_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:17:01.71 +63:21:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265403_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 265403_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265605_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 265605_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265670_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 265670_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:42:26.65 +59:34:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265716_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 265716_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:10:10.07 +59:08:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265747_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 265747_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265973_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 265973_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:11:34.60 +57:37:41.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 266059_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 266059_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266143_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 266143_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:56:25.43 +62:05:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266242_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 266242_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:31:48.50 +64:22:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266315_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 266315_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:11:49.99 +59:02:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266373_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 266373_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 266562_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 266562_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:00:35.50 +58:32:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266715_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 266715_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:49:06.15 +65:23:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266733_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 266733_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266751_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 266751_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266795_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 266795_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:15:05.56 +64:08:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266841_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 266841_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:41:13.38 +62:53:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266982_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 266982_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267057_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 267057_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267067_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 267067_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:37:55.40 +58:09:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267088_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 267088_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:55:05.16 +59:57:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267091_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 267091_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:54:06.19 +61:05:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267216_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 267216_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267395_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 267395_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267408_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 267408_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:23:42.46 +63:43:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267649_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 267649_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267680_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 267680_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268128_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 268128_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268320_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 268320_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268358_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 268358_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:38:57.06 +63:28:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268449_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 268449_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268596_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 268596_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:47:18.65 +58:31:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268656_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 268656_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269004_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 269004_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269513_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 269513_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269589_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 269589_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269824_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 269824_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270146_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 270146_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:53:02.95 +60:26:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270171_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 270171_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270257_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 270257_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:42:49.51 +61:24:06.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 270363_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 270363_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:16:55.49 +62:27:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270397_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 270397_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:27:03.99 +64:43:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270426_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 270426_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270516_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 270516_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:13:35.36 +58:31:49.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 270737_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 270737_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270986_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 270986_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270999_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 270999_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 271061_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 271061_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271157_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 271157_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271178_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 271178_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271265_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 271265_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271285_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 271285_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:15:16.90 +59:21:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271373_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 271373_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:10:18.00 +60:08:15.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271526_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 271526_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271999_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 271999_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272039_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 272039_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272231_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 272231_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:41:41.06 +57:56:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272232_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 272232_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272278_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 272278_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272366_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 272366_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272627_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 272627_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272652_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 272652_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272674_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 272674_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272678_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 272678_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272724_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 272724_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272771_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 272771_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272807_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 272807_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 273194_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 273194_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:54:56.74 +63:41:23.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 273233_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 273233_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 273640_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 273640_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 273814_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 273814_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 273842_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 273842_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 275468_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 275468_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 275498_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 275498_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 275526_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 275526_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 275712_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 275712_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 275774_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 275774_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 275776_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 275776_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 275843_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 275843_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 275901_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 275901_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:48:21.39 +62:53:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 275955_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 275955_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 276422_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 276422_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 276501_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 276501_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277011_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 277011_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277100_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 277100_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277527_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 277527_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277791_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 277791_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277815_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 277815_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277910_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 277910_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278203_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 278203_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278372_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 278372_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 278509_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 278509_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278785_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 278785_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278994_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 278994_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279028_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 279028_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279174_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 279174_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279368_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 279368_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279481_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 279481_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279745_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 279745_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279750_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 279750_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279796_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 279796_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279830_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 279830_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279883_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 279883_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279988_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 279988_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280123_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280123_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280136_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280136_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280215_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 280215_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280271_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 280271_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280298_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 280298_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
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Considering the candidate 280319_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280319_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280336_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280336_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280354_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280354_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280379_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280379_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280389_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280389_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280424_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280424_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280473_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280473_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280479_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280479_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280764_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280764_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280767_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280767_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280862_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 280862_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
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Considering the candidate 280959_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280959_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280964_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280964_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 280997_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 280997_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281047_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281047_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281057_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281057_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281084_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281084_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281205_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281205_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281287_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281287_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281295_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281295_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281335_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281335_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281391_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281391_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281404_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 281404_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281491_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281491_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281516_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281516_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281527_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281527_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281556_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281556_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281581_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281581_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281623_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281623_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281712_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 281712_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281791_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281791_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281808_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 281808_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281883_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 281883_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 281977_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 281977_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 282000_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 282000_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 282001_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 282001_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 282145_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
Preparing report for the candidate 282145_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 70271_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:20:32.46 +62:32:01.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 72532_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:45:35.77 +63:07:03.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 112593_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:21:55.12 +61:20:58.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234396_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 234396_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:29:32.67 +63:18:27.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 233956_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 233956_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 02:18:51.74 +62:48:15.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156692_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 156692_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:56:38.05 +59:15:34.1 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 39378_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
**** FOUND 01:47:55.61 +64:32:55.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164131_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445
The candidate 164131_fd_Cas-03-Q2b1x1_2026-06-22_04-44-47_20.00sec_5.00C_LIGHT_0445 did not pass the final checks
Rejecting candidate due to large distance (38.7") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 12s
make_report_in_HTML.sh TOTAL: 464s
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 ####
01:56:38.03 +59:15:34.2
02:13:57.98 +64:54:41.5
01:22:37.56 +58:29:18.7
01:15:31.02 +60:11:14.3
01:06:49.17 +60:52:38.6
01:33:22.79 +61:41:09.1
01:13:56.67 +59:30:04.6
01:19:29.37 +60:17:35.0
01:43:44.10 +58:30:28.3
01:28:02.88 +62:04:06.1
01:14:36.05 +59:51:11.4
01:39:44.00 +57:57:02.6
01:59:39.67 +58:16:32.4
01:16:16.54 +59:38:19.7
01:26:01.63 +59:58:53.0
01:11:16.45 +58:55:56.1
01:59:07.36 +58:48:33.4
01:36:52.29 +58:28:35.9
01:19:08.74 +60:17:20.1
01:23:56.64 +62:15:29.2
01:41:12.20 +60:00:52.4
01:16:20.25 +58:49:31.5
01:32:34.60 +60:01:12.0
02:15:20.97 +63:07:35.0
01:08:06.01 +61:33:37.1
01:43:24.05 +61:12:07.1
01:06:16.00 +57:53:25.1
01:47:11.11 +58:16:20.0
01:49:03.19 +60:18:50.1
01:12:41.15 +61:18:07.7
01:41:20.99 +58:11:50.9
02:00:30.18 +62:28:28.3
02:12:28.25 +62:23:03.9
01:30:58.15 +59:29:29.4
01:24:44.68 +63:34:17.1
01:32:09.12 +61:32:10.9
01:48:26.29 +60:22:28.9
01:13:34.72 +58:01:48.7
01:05:53.86 +59:06:25.2
01:45:17.42 +62:09:43.0
01:53:37.98 +64:44:10.2
01:33:12.85 +61:16:55.2
01:57:29.35 +60:09:19.2
01:52:02.35 +59:36:20.4
01:42:02.51 +59:46:32.9
01:08:25.45 +59:48:03.8
01:36:47.04 +59:24:04.7
01:20:38.69 +59:28:19.0
01:17:26.20 +61:54:16.6
01:32:10.96 +59:36:02.6
01:22:33.22 +60:44:43.0
01:18:32.34 +57:50:16.0
02:11:00.59 +60:08:50.5
01:47:04.41 +59:18:56.1
01:32:41.63 +60:27:01.5
01:12:09.67 +58:47:54.3
01:21:45.28 +58:34:14.7
01:08:39.03 +60:32:42.2
01:10:05.00 +57:48:02.6
01:30:39.42 +59:02:43.7
01:10:43.79 +60:59:19.0
01:12:59.89 +57:33:53.5
01:06:59.51 +61:28:40.4
01:07:36.77 +58:09:25.4
01:59:41.75 +63:32:25.4
01:13:19.97 +61:29:38.9
01:36:49.02 +62:46:52.5
01:06:13.06 +59:33:47.0
01:30:00.97 +60:10:50.2
01:43:27.45 +58:38:06.5
01:51:47.42 +58:37:58.5
01:56:13.05 +59:33:49.7
02:03:04.99 +57:50:13.7
01:24:54.86 +59:41:45.2
01:25:27.57 +59:27:15.1
01:18:31.18 +60:17:31.5
01:12:00.91 +64:42:20.0
01:07:01.45 +59:43:01.3
01:07:39.20 +59:59:18.4
02:00:21.98 +58:20:18.3
01:34:16.42 +60:57:34.8
02:00:23.29 +64:54:51.9
01:07:31.78 +61:28:29.6
01:31:23.12 +59:33:43.4
01:23:22.18 +60:18:16.6
01:57:04.38 +58:53:27.3
01:18:28.11 +58:11:23.7
01:32:05.63 +61:59:26.8
01:44:02.95 +61:54:45.6
01:08:36.65 +60:44:55.0
01:22:23.83 +61:13:51.2
01:18:48.45 +64:12:21.9
01:13:38.99 +58:10:51.5
01:51:26.62 +57:51:36.8
01:09:22.73 +57:26:31.5
02:07:53.83 +58:37:40.5
02:16:07.65 +58:18:13.6
01:27:34.47 +57:48:26.0
02:15:10.49 +58:07:01.8
02:15:03.79 +58:28:54.1
01:20:13.79 +65:31:27.3
01:08:59.24 +60:47:20.7
02:09:48.66 +59:05:18.0
01:50:39.89 +62:00:56.0
01:34:07.22 +60:12:52.5
01:44:29.97 +65:09:24.4
02:13:40.28 +65:08:15.5
01:59:34.07 +63:37:08.7
02:08:50.69 +59:21:19.8
01:16:56.61 +59:03:13.9
01:56:57.28 +63:00:32.6
01:09:58.01 +59:03:02.1
01:48:19.06 +59:38:19.2
02:02:11.53 +61:55:31.4
01:33:30.54 +58:02:22.0
01:52:07.07 +59:13:07.6
01:51:53.53 +63:26:22.3
01:19:29.22 +59:25:22.7
01:28:07.34 +59:53:51.6
01:58:53.87 +61:23:25.6
02:03:41.72 +58:47:26.1
01:33:35.72 +60:32:28.6
01:29:25.46 +60:01:31.9
01:51:40.02 +60:56:16.7
02:02:23.72 +64:38:25.5
01:40:21.65 +60:37:45.8
01:19:11.81 +59:07:32.7
02:12:20.59 +64:11:16.0
02:03:33.12 +58:39:09.8
01:30:50.88 +60:06:03.4
02:01:26.30 +59:44:32.4
01:55:15.25 +58:45:57.8
01:24:36.31 +61:08:54.9
01:38:40.39 +64:31:56.4
01:20:35.08 +64:02:26.5
01:26:06.00 +59:42:39.7
01:22:13.58 +59:52:27.1
01:31:27.96 +63:36:57.8
01:29:38.33 +63:19:38.0
01:38:11.93 +62:50:30.9
01:40:28.70 +60:34:45.2
01:48:17.90 +60:40:25.2
01:52:07.71 +59:52:59.5
01:34:06.34 +59:58:54.2
01:30:40.75 +59:33:48.0
01:45:17.16 +58:43:30.6
01:26:31.51 +60:49:34.2
02:16:01.71 +61:10:48.8
01:29:20.64 +60:14:12.4
01:46:56.51 +61:34:41.2
01:39:55.66 +61:01:23.9
01:28:14.59 +60:19:20.9
02:02:05.39 +62:09:27.7
01:35:45.28 +61:18:34.4
01:23:32.35 +60:58:47.9
01:06:45.13 +60:27:55.0
01:36:46.33 +61:14:49.6
01:26:22.35 +61:16:28.9
01:41:15.07 +58:14:31.5
01:35:58.99 +57:43:50.5
01:50:26.85 +59:20:13.4
01:19:47.70 +60:24:29.9
01:29:04.61 +62:34:45.2
01:58:37.12 +63:40:15.0
01:43:25.66 +58:49:24.8
01:50:50.64 +59:17:02.3
01:49:52.71 +58:55:20.4
01:53:43.15 +60:08:00.1
01:13:10.72 +58:11:20.8
01:34:20.25 +61:27:01.2
01:44:25.02 +65:16:03.2
01:45:29.06 +58:26:32.6
01:37:48.39 +58:09:09.1
01:39:27.36 +60:45:14.3
01:46:48.64 +58:27:31.2
01:35:59.51 +63:11:54.3
01:06:52.62 +62:05:00.8
02:13:53.24 +65:54:40.5
01:19:21.39 +58:01:15.4
01:43:56.14 +58:56:40.5
01:35:02.55 +59:41:35.0
01:55:15.49 +59:42:12.6
02:14:12.40 +65:14:53.8
01:37:59.09 +61:09:38.8
01:37:09.63 +60:59:35.3
01:45:00.46 +59:26:56.3
01:45:40.34 +59:47:00.0
01:12:27.12 +58:01:05.5
01:31:49.85 +62:50:13.0
01:07:40.29 +57:36:50.0
01:37:28.98 +61:17:47.1
01:45:06.92 +57:56:34.9
01:07:57.66 +60:18:17.7
01:22:24.79 +62:39:02.2
01:17:35.37 +59:21:38.7
01:22:54.68 +58:55:22.5
########### 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 ####
01:56:38.03 +59:15:34.2
02:13:57.98 +64:54:41.5
01:22:37.56 +58:29:18.7
01:15:31.02 +60:11:14.3
01:06:49.17 +60:52:38.6
01:33:22.79 +61:41:09.1
01:13:56.67 +59:30:04.6
01:19:29.37 +60:17:35.0
01:43:44.10 +58:30:28.3
01:28:02.88 +62:04:06.1
01:14:36.05 +59:51:11.4
01:39:44.00 +57:57:02.6
01:59:39.67 +58:16:32.4
01:16:16.54 +59:38:19.7
01:26:01.63 +59:58:53.0
01:11:16.45 +58:55:56.1
01:59:07.36 +58:48:33.4
01:36:52.29 +58:28:35.9
01:19:08.74 +60:17:20.1
01:23:56.64 +62:15:29.2
01:41:12.20 +60:00:52.4
01:16:20.25 +58:49:31.5
01:32:34.60 +60:01:12.0
02:15:20.97 +63:07:35.0
01:08:06.01 +61:33:37.1
01:43:24.05 +61:12:07.1
01:06:16.00 +57:53:25.1
01:47:11.11 +58:16:20.0
01:49:03.19 +60:18:50.1
01:12:41.15 +61:18:07.7
01:41:20.99 +58:11:50.9
02:00:30.18 +62:28:28.3
02:12:28.25 +62:23:03.9
01:30:58.15 +59:29:29.4
01:24:44.68 +63:34:17.1
01:32:09.12 +61:32:10.9
01:48:26.29 +60:22:28.9
01:13:34.72 +58:01:48.7
01:05:53.86 +59:06:25.2
01:45:17.42 +62:09:43.0
01:53:37.98 +64:44:10.2
01:33:12.85 +61:16:55.2
01:57:29.35 +60:09:19.2
01:52:02.35 +59:36:20.4
01:42:02.51 +59:46:32.9
01:08:25.45 +59:48:03.8
01:36:47.04 +59:24:04.7
01:20:38.69 +59:28:19.0
01:17:26.20 +61:54:16.6
01:32:10.96 +59:36:02.6
01:22:33.22 +60:44:43.0
01:18:32.34 +57:50:16.0
02:11:00.59 +60:08:50.5
01:47:04.41 +59:18:56.1
01:32:41.63 +60:27:01.5
01:12:09.67 +58:47:54.3
01:21:45.28 +58:34:14.7
01:08:39.03 +60:32:42.2
01:10:05.00 +57:48:02.6
01:30:39.42 +59:02:43.7
01:10:43.79 +60:59:19.0
01:12:59.89 +57:33:53.5
01:06:59.51 +61:28:40.4
01:07:36.77 +58:09:25.4
01:59:41.75 +63:32:25.4
01:13:19.97 +61:29:38.9
01:36:49.02 +62:46:52.5
01:06:13.06 +59:33:47.0
01:30:00.97 +60:10:50.2
01:43:27.45 +58:38:06.5
01:51:47.42 +58:37:58.5
01:56:13.05 +59:33:49.7
02:03:04.99 +57:50:13.7
01:24:54.86 +59:41:45.2
01:25:27.57 +59:27:15.1
01:18:31.18 +60:17:31.5
01:12:00.91 +64:42:20.0
01:07:01.45 +59:43:01.3
01:07:39.20 +59:59:18.4
02:00:21.98 +58:20:18.3
01:34:16.42 +60:57:34.8
02:00:23.29 +64:54:51.9
01:07:31.78 +61:28:29.6
01:31:23.12 +59:33:43.4
01:23:22.18 +60:18:16.6
01:57:04.38 +58:53:27.3
01:18:28.11 +58:11:23.7
01:32:05.63 +61:59:26.8
01:44:02.95 +61:54:45.6
01:08:36.65 +60:44:55.0
01:22:23.83 +61:13:51.2
01:18:48.45 +64:12:21.9
01:13:38.99 +58:10:51.5
01:51:26.62 +57:51:36.8
01:09:22.73 +57:26:31.5
02:07:53.83 +58:37:40.5
02:16:07.65 +58:18:13.6
01:27:34.47 +57:48:26.0
02:15:10.49 +58:07:01.8
02:15:03.79 +58:28:54.1
01:20:13.79 +65:31:27.3
01:08:59.24 +60:47:20.7
02:09:48.66 +59:05:18.0
01:50:39.89 +62:00:56.0
01:34:07.22 +60:12:52.5
01:44:29.97 +65:09:24.4
02:13:40.28 +65:08:15.5
01:59:34.07 +63:37:08.7
02:08:50.69 +59:21:19.8
01:16:56.61 +59:03:13.9
01:56:57.28 +63:00:32.6
01:09:58.01 +59:03:02.1
01:48:19.06 +59:38:19.2
02:02:11.53 +61:55:31.4
01:33:30.54 +58:02:22.0
01:52:07.07 +59:13:07.6
01:51:53.53 +63:26:22.3
01:19:29.22 +59:25:22.7
01:28:07.34 +59:53:51.6
01:58:53.87 +61:23:25.6
02:03:41.72 +58:47:26.1
01:33:35.72 +60:32:28.6
01:29:25.46 +60:01:31.9
01:51:40.02 +60:56:16.7
02:02:23.72 +64:38:25.5
01:40:21.65 +60:37:45.8
01:19:11.81 +59:07:32.7
02:12:20.59 +64:11:16.0
02:03:33.12 +58:39:09.8
01:30:50.88 +60:06:03.4
02:01:26.30 +59:44:32.4
01:55:15.25 +58:45:57.8
01:24:36.31 +61:08:54.9
01:38:40.39 +64:31:56.4
01:20:35.08 +64:02:26.5
01:26:06.00 +59:42:39.7
01:22:13.58 +59:52:27.1
01:31:27.96 +63:36:57.8
01:29:38.33 +63:19:38.0
01:38:11.93 +62:50:30.9
01:40:28.70 +60:34:45.2
01:48:17.90 +60:40:25.2
01:52:07.71 +59:52:59.5
01:34:06.34 +59:58:54.2
01:30:40.75 +59:33:48.0
01:45:17.16 +58:43:30.6
01:26:31.51 +60:49:34.2
02:16:01.71 +61:10:48.8
01:29:20.64 +60:14:12.4
01:46:56.51 +61:34:41.2
01:39:55.66 +61:01:23.9
01:28:14.59 +60:19:20.9
02:02:05.39 +62:09:27.7
01:35:45.28 +61:18:34.4
01:23:32.35 +60:58:47.9
01:06:45.13 +60:27:55.0
01:36:46.33 +61:14:49.6
01:26:22.35 +61:16:28.9
01:41:15.07 +58:14:31.5
01:35:58.99 +57:43:50.5
01:50:26.85 +59:20:13.4
01:19:47.70 +60:24:29.9
01:29:04.61 +62:34:45.2
01:58:37.12 +63:40:15.0
01:43:25.66 +58:49:24.8
01:50:50.64 +59:17:02.3
01:49:52.71 +58:55:20.4
01:53:43.15 +60:08:00.1
01:13:10.72 +58:11:20.8
01:34:20.25 +61:27:01.2
01:44:25.02 +65:16:03.2
01:45:29.06 +58:26:32.6
01:37:48.39 +58:09:09.1
01:39:27.36 +60:45:14.3
01:46:48.64 +58:27:31.2
01:35:59.51 +63:11:54.3
01:06:52.62 +62:05:00.8
02:13:53.24 +65:54:40.5
01:19:21.39 +58:01:15.4
01:43:56.14 +58:56:40.5
01:35:02.55 +59:41:35.0
01:55:15.49 +59:42:12.6
02:14:12.40 +65:14:53.8
01:37:59.09 +61:09:38.8
01:37:09.63 +60:59:35.3
01:45:00.46 +59:26:56.3
01:45:40.34 +59:47:00.0
01:12:27.12 +58:01:05.5
01:31:49.85 +62:50:13.0
01:07:40.29 +57:36:50.0
01:37:28.98 +61:17:47.1
01:45:06.92 +57:56:34.9
01:07:57.66 +60:18:17.7
01:22:24.79 +62:39:02.2
01:17:35.37 +59:21:38.7
01:22:54.68 +58:55:22.5
###################################################################################
01:56:38.03 +59:15:34.2 -- not an asteroid (will add it to exclusion list)
02:13:57.98 +64:54:41.5 -- not an asteroid (will add it to exclusion list)
01:22:37.56 +58:29:18.7 -- not an asteroid (will add it to exclusion list)
01:15:31.02 +60:11:14.3 -- not an asteroid (will add it to exclusion list)
01:06:49.17 +60:52:38.6 -- not an asteroid (will add it to exclusion list)
01:33:22.79 +61:41:09.1 -- not an asteroid (will add it to exclusion list)
01:13:56.67 +59:30:04.6 -- not an asteroid (will add it to exclusion list)
01:19:29.37 +60:17:35.0 -- not an asteroid (will add it to exclusion list)
01:43:44.10 +58:30:28.3 -- not an asteroid (will add it to exclusion list)
01:28:02.88 +62:04:06.1 -- not an asteroid (will add it to exclusion list)
01:14:36.05 +59:51:11.4 -- not an asteroid (will add it to exclusion list)
01:39:44.00 +57:57:02.6 -- not an asteroid (will add it to exclusion list)
01:59:39.67 +58:16:32.4 -- not an asteroid (will add it to exclusion list)
01:16:16.54 +59:38:19.7 -- not an asteroid (will add it to exclusion list)
01:26:01.63 +59:58:53.0 -- not an asteroid (will add it to exclusion list)
01:11:16.45 +58:55:56.1 -- not an asteroid (will add it to exclusion list)
01:59:07.36 +58:48:33.4 -- not an asteroid (will add it to exclusion list)
01:36:52.29 +58:28:35.9 -- not an asteroid (will add it to exclusion list)
01:19:08.74 +60:17:20.1 -- not an asteroid (will add it to exclusion list)
01:23:56.64 +62:15:29.2 -- not an asteroid (will add it to exclusion list)
01:41:12.20 +60:00:52.4 -- not an asteroid (will add it to exclusion list)
01:16:20.25 +58:49:31.5 -- not an asteroid (will add it to exclusion list)
01:32:34.60 +60:01:12.0 -- not an asteroid (will add it to exclusion list)
02:15:20.97 +63:07:35.0 -- not an asteroid (will add it to exclusion list)
01:08:06.01 +61:33:37.1 -- not an asteroid (will add it to exclusion list)
01:43:24.05 +61:12:07.1 -- not an asteroid (will add it to exclusion list)
01:06:16.00 +57:53:25.1 -- not an asteroid (will add it to exclusion list)
01:47:11.11 +58:16:20.0 -- not an asteroid (will add it to exclusion list)
01:49:03.19 +60:18:50.1 -- not an asteroid (will add it to exclusion list)
01:12:41.15 +61:18:07.7 -- not an asteroid (will add it to exclusion list)
01:41:20.99 +58:11:50.9 -- not an asteroid (will add it to exclusion list)
02:00:30.18 +62:28:28.3 -- not an asteroid (will add it to exclusion list)
02:12:28.25 +62:23:03.9 -- not an asteroid (will add it to exclusion list)
01:30:58.15 +59:29:29.4 -- not an asteroid (will add it to exclusion list)
01:24:44.68 +63:34:17.1 -- not an asteroid (will add it to exclusion list)
01:32:09.12 +61:32:10.9 -- not an asteroid (will add it to exclusion list)
01:48:26.29 +60:22:28.9 -- not an asteroid (will add it to exclusion list)
01:13:34.72 +58:01:48.7 -- not an asteroid (will add it to exclusion list)
01:05:53.86 +59:06:25.2 -- not an asteroid (will add it to exclusion list)
01:45:17.42 +62:09:43.0 -- not an asteroid (will add it to exclusion list)
01:53:37.98 +64:44:10.2 -- not an asteroid (will add it to exclusion list)
01:33:12.85 +61:16:55.2 -- not an asteroid (will add it to exclusion list)
01:57:29.35 +60:09:19.2 -- not an asteroid (will add it to exclusion list)
01:52:02.35 +59:36:20.4 -- not an asteroid (will add it to exclusion list)
01:42:02.51 +59:46:32.9 -- not an asteroid (will add it to exclusion list)
01:08:25.45 +59:48:03.8 -- not an asteroid (will add it to exclusion list)
01:36:47.04 +59:24:04.7 -- not an asteroid (will add it to exclusion list)
01:20:38.69 +59:28:19.0 -- not an asteroid (will add it to exclusion list)
01:17:26.20 +61:54:16.6 -- not an asteroid (will add it to exclusion list)
01:32:10.96 +59:36:02.6 -- not an asteroid (will add it to exclusion list)
01:22:33.22 +60:44:43.0 -- not an asteroid (will add it to exclusion list)
01:18:32.34 +57:50:16.0 -- not an asteroid (will add it to exclusion list)
02:11:00.59 +60:08:50.5 -- not an asteroid (will add it to exclusion list)
01:47:04.41 +59:18:56.1 -- not an asteroid (will add it to exclusion list)
01:32:41.63 +60:27:01.5 -- not an asteroid (will add it to exclusion list)
01:12:09.67 +58:47:54.3 -- not an asteroid (will add it to exclusion list)
01:21:45.28 +58:34:14.7 -- not an asteroid (will add it to exclusion list)
01:08:39.03 +60:32:42.2 -- not an asteroid (will add it to exclusion list)
01:10:05.00 +57:48:02.6 -- not an asteroid (will add it to exclusion list)
01:30:39.42 +59:02:43.7 -- not an asteroid (will add it to exclusion list)
01:10:43.79 +60:59:19.0 -- not an asteroid (will add it to exclusion list)
01:12:59.89 +57:33:53.5 -- not an asteroid (will add it to exclusion list)
01:06:59.51 +61:28:40.4 -- not an asteroid (will add it to exclusion list)
01:07:36.77 +58:09:25.4 -- not an asteroid (will add it to exclusion list)
01:59:41.75 +63:32:25.4 -- not an asteroid (will add it to exclusion list)
01:13:19.97 +61:29:38.9 -- not an asteroid (will add it to exclusion list)
01:36:49.02 +62:46:52.5 -- not an asteroid (will add it to exclusion list)
01:06:13.06 +59:33:47.0 -- not an asteroid (will add it to exclusion list)
01:30:00.97 +60:10:50.2 -- not an asteroid (will add it to exclusion list)
01:43:27.45 +58:38:06.5 -- not an asteroid (will add it to exclusion list)
01:51:47.42 +58:37:58.5 -- not an asteroid (will add it to exclusion list)
01:56:13.05 +59:33:49.7 -- not an asteroid (will add it to exclusion list)
02:03:04.99 +57:50:13.7 -- not an asteroid (will add it to exclusion list)
01:24:54.86 +59:41:45.2 -- not an asteroid (will add it to exclusion list)
01:25:27.57 +59:27:15.1 -- not an asteroid (will add it to exclusion list)
01:18:31.18 +60:17:31.5 -- not an asteroid (will add it to exclusion list)
01:12:00.91 +64:42:20.0 -- not an asteroid (will add it to exclusion list)
01:07:01.45 +59:43:01.3 -- not an asteroid (will add it to exclusion list)
01:07:39.20 +59:59:18.4 -- not an asteroid (will add it to exclusion list)
02:00:21.98 +58:20:18.3 -- not an asteroid (will add it to exclusion list)
01:34:16.42 +60:57:34.8 -- not an asteroid (will add it to exclusion list)
02:00:23.29 +64:54:51.9 -- not an asteroid (will add it to exclusion list)
01:07:31.78 +61:28:29.6 -- not an asteroid (will add it to exclusion list)
01:31:23.12 +59:33:43.4 -- not an asteroid (will add it to exclusion list)
01:23:22.18 +60:18:16.6 -- not an asteroid (will add it to exclusion list)
01:57:04.38 +58:53:27.3 -- not an asteroid (will add it to exclusion list)
01:18:28.11 +58:11:23.7 -- not an asteroid (will add it to exclusion list)
01:32:05.63 +61:59:26.8 -- not an asteroid (will add it to exclusion list)
01:44:02.95 +61:54:45.6 -- not an asteroid (will add it to exclusion list)
01:08:36.65 +60:44:55.0 -- not an asteroid (will add it to exclusion list)
01:22:23.83 +61:13:51.2 -- not an asteroid (will add it to exclusion list)
01:18:48.45 +64:12:21.9 -- not an asteroid (will add it to exclusion list)
01:13:38.99 +58:10:51.5 -- not an asteroid (will add it to exclusion list)
01:51:26.62 +57:51:36.8 -- not an asteroid (will add it to exclusion list)
01:09:22.73 +57:26:31.5 -- not an asteroid (will add it to exclusion list)
02:07:53.83 +58:37:40.5 -- not an asteroid (will add it to exclusion list)
02:16:07.65 +58:18:13.6 -- not an asteroid (will add it to exclusion list)
01:27:34.47 +57:48:26.0 -- not an asteroid (will add it to exclusion list)
02:15:10.49 +58:07:01.8 -- not an asteroid (will add it to exclusion list)
02:15:03.79 +58:28:54.1 -- not an asteroid (will add it to exclusion list)
01:20:13.79 +65:31:27.3 -- not an asteroid (will add it to exclusion list)
01:08:59.24 +60:47:20.7 -- not an asteroid (will add it to exclusion list)
02:09:48.66 +59:05:18.0 -- not an asteroid (will add it to exclusion list)
01:50:39.89 +62:00:56.0 -- not an asteroid (will add it to exclusion list)
01:34:07.22 +60:12:52.5 -- not an asteroid (will add it to exclusion list)
01:44:29.97 +65:09:24.4 -- not an asteroid (will add it to exclusion list)
02:13:40.28 +65:08:15.5 -- not an asteroid (will add it to exclusion list)
01:59:34.07 +63:37:08.7 -- not an asteroid (will add it to exclusion list)
02:08:50.69 +59:21:19.8 -- not an asteroid (will add it to exclusion list)
01:16:56.61 +59:03:13.9 -- not an asteroid (will add it to exclusion list)
01:56:57.28 +63:00:32.6 -- not an asteroid (will add it to exclusion list)
01:09:58.01 +59:03:02.1 -- not an asteroid (will add it to exclusion list)
01:48:19.06 +59:38:19.2 -- not an asteroid (will add it to exclusion list)
02:02:11.53 +61:55:31.4 -- not an asteroid (will add it to exclusion list)
01:33:30.54 +58:02:22.0 -- not an asteroid (will add it to exclusion list)
01:52:07.07 +59:13:07.6 -- not an asteroid (will add it to exclusion list)
01:51:53.53 +63:26:22.3 -- not an asteroid (will add it to exclusion list)
01:19:29.22 +59:25:22.7 -- not an asteroid (will add it to exclusion list)
01:28:07.34 +59:53:51.6 -- not an asteroid (will add it to exclusion list)
01:58:53.87 +61:23:25.6 -- not an asteroid (will add it to exclusion list)
02:03:41.72 +58:47:26.1 -- not an asteroid (will add it to exclusion list)
01:33:35.72 +60:32:28.6 -- not an asteroid (will add it to exclusion list)
01:29:25.46 +60:01:31.9 -- not an asteroid (will add it to exclusion list)
01:51:40.02 +60:56:16.7 -- not an asteroid (will add it to exclusion list)
02:02:23.72 +64:38:25.5 -- not an asteroid (will add it to exclusion list)
01:40:21.65 +60:37:45.8 -- not an asteroid (will add it to exclusion list)
01:19:11.81 +59:07:32.7 -- not an asteroid (will add it to exclusion list)
02:12:20.59 +64:11:16.0 -- not an asteroid (will add it to exclusion list)
02:03:33.12 +58:39:09.8 -- not an asteroid (will add it to exclusion list)
01:30:50.88 +60:06:03.4 -- not an asteroid (will add it to exclusion list)
02:01:26.30 +59:44:32.4 -- not an asteroid (will add it to exclusion list)
01:55:15.25 +58:45:57.8 -- not an asteroid (will add it to exclusion list)
01:24:36.31 +61:08:54.9 -- not an asteroid (will add it to exclusion list)
01:38:40.39 +64:31:56.4 -- not an asteroid (will add it to exclusion list)
01:20:35.08 +64:02:26.5 -- not an asteroid (will add it to exclusion list)
01:26:06.00 +59:42:39.7 -- not an asteroid (will add it to exclusion list)
01:22:13.58 +59:52:27.1 -- not an asteroid (will add it to exclusion list)
01:31:27.96 +63:36:57.8 -- not an asteroid (will add it to exclusion list)
01:29:38.33 +63:19:38.0 -- not an asteroid (will add it to exclusion list)
01:38:11.93 +62:50:30.9 -- not an asteroid (will add it to exclusion list)
01:40:28.70 +60:34:45.2 -- not an asteroid (will add it to exclusion list)
01:48:17.90 +60:40:25.2 -- not an asteroid (will add it to exclusion list)
01:52:07.71 +59:52:59.5 -- not an asteroid (will add it to exclusion list)
01:34:06.34 +59:58:54.2 -- not an asteroid (will add it to exclusion list)
01:30:40.75 +59:33:48.0 -- not an asteroid (will add it to exclusion list)
01:45:17.16 +58:43:30.6 -- not an asteroid (will add it to exclusion list)
01:26:31.51 +60:49:34.2 -- not an asteroid (will add it to exclusion list)
02:16:01.71 +61:10:48.8 -- not an asteroid (will add it to exclusion list)
01:29:20.64 +60:14:12.4 -- not an asteroid (will add it to exclusion list)
01:46:56.51 +61:34:41.2 -- not an asteroid (will add it to exclusion list)
01:39:55.66 +61:01:23.9 -- not an asteroid (will add it to exclusion list)
01:28:14.59 +60:19:20.9 -- not an asteroid (will add it to exclusion list)
02:02:05.39 +62:09:27.7 -- not an asteroid (will add it to exclusion list)
01:35:45.28 +61:18:34.4 -- not an asteroid (will add it to exclusion list)
01:23:32.35 +60:58:47.9 -- not an asteroid (will add it to exclusion list)
01:06:45.13 +60:27:55.0 -- not an asteroid (will add it to exclusion list)
01:36:46.33 +61:14:49.6 -- not an asteroid (will add it to exclusion list)
01:26:22.35 +61:16:28.9 -- not an asteroid (will add it to exclusion list)
01:41:15.07 +58:14:31.5 -- not an asteroid (will add it to exclusion list)
01:35:58.99 +57:43:50.5 -- not an asteroid (will add it to exclusion list)
01:50:26.85 +59:20:13.4 -- not an asteroid (will add it to exclusion list)
01:19:47.70 +60:24:29.9 -- not an asteroid (will add it to exclusion list)
01:29:04.61 +62:34:45.2 -- not an asteroid (will add it to exclusion list)
01:58:37.12 +63:40:15.0 -- not an asteroid (will add it to exclusion list)
01:43:25.66 +58:49:24.8 -- not an asteroid (will add it to exclusion list)
01:50:50.64 +59:17:02.3 -- not an asteroid (will add it to exclusion list)
01:49:52.71 +58:55:20.4 -- not an asteroid (will add it to exclusion list)
01:53:43.15 +60:08:00.1 -- not an asteroid (will add it to exclusion list)
01:13:10.72 +58:11:20.8 -- not an asteroid (will add it to exclusion list)
01:34:20.25 +61:27:01.2 -- not an asteroid (will add it to exclusion list)
01:44:25.02 +65:16:03.2 -- not an asteroid (will add it to exclusion list)
01:45:29.06 +58:26:32.6 -- not an asteroid (will add it to exclusion list)
01:37:48.39 +58:09:09.1 -- not an asteroid (will add it to exclusion list)
01:39:27.36 +60:45:14.3 -- not an asteroid (will add it to exclusion list)
01:46:48.64 +58:27:31.2 -- not an asteroid (will add it to exclusion list)
01:35:59.51 +63:11:54.3 -- not an asteroid (will add it to exclusion list)
01:06:52.62 +62:05:00.8 -- not an asteroid (will add it to exclusion list)
02:13:53.24 +65:54:40.5 -- not an asteroid (will add it to exclusion list)
01:19:21.39 +58:01:15.4 -- not an asteroid (will add it to exclusion list)
01:43:56.14 +58:56:40.5 -- not an asteroid (will add it to exclusion list)
01:35:02.55 +59:41:35.0 -- not an asteroid (will add it to exclusion list)
01:55:15.49 +59:42:12.6 -- not an asteroid (will add it to exclusion list)
02:14:12.40 +65:14:53.8 -- not an asteroid (will add it to exclusion list)
01:37:59.09 +61:09:38.8 -- not an asteroid (will add it to exclusion list)
01:37:09.63 +60:59:35.3 -- not an asteroid (will add it to exclusion list)
01:45:00.46 +59:26:56.3 -- not an asteroid (will add it to exclusion list)
01:45:40.34 +59:47:00.0 -- not an asteroid (will add it to exclusion list)
01:12:27.12 +58:01:05.5 -- not an asteroid (will add it to exclusion list)
01:31:49.85 +62:50:13.0 -- not an asteroid (will add it to exclusion list)
01:07:40.29 +57:36:50.0 -- not an asteroid (will add it to exclusion list)
01:37:28.98 +61:17:47.1 -- not an asteroid (will add it to exclusion list)
01:45:06.92 +57:56:34.9 -- not an asteroid (will add it to exclusion list)
01:07:57.66 +60:18:17.7 -- not an asteroid (will add it to exclusion list)
01:22:24.79 +62:39:02.2 -- not an asteroid (will add it to exclusion list)
01:17:35.37 +59:21:38.7 -- not an asteroid (will add it to exclusion list)
01:22:54.68 +58:55:22.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:05:53.86 +59:06:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:13.06 +59:33:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:16.00 +57:53:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:45.13 +60:27:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:49.17 +60:52:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:52.62 +62:05:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:59.51 +61:28:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:01.45 +59:43:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:31.78 +61:28:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:36.77 +58:09:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.20 +59:59:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:40.29 +57:36:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:57.66 +60:18:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:06.01 +61:33:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:25.45 +59:48:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:36.65 +60:44:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:39.03 +60:32:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:59.24 +60:47:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:22.73 +57:26:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:58.01 +59:03:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:05.00 +57:48:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:43.79 +60:59:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:16.45 +58:55:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:00.91 +64:42:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:09.67 +58:47:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:27.12 +58:01:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:41.15 +61:18:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:59.89 +57:33:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:10.72 +58:11:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:19.97 +61:29:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:34.72 +58:01:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:38.99 +58:10:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:56.67 +59:30:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:36.05 +59:51:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:31.02 +60:11:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:16.54 +59:38:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:20.25 +58:49:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:56.61 +59:03:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:26.20 +61:54:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:35.37 +59:21:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:28.11 +58:11:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:31.18 +60:17:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:32.34 +57:50:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:48.45 +64:12:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:08.74 +60:17:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:11.81 +59:07:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:21.39 +58:01:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:29.22 +59:25:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:29.37 +60:17:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:47.70 +60:24:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:13.79 +65:31:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:35.08 +64:02:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:38.69 +59:28:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:45.28 +58:34:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:13.58 +59:52:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:23.83 +61:13:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:24.79 +62:39:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:33.22 +60:44:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:37.56 +58:29:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:54.68 +58:55:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:22.18 +60:18:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:32.35 +60:58:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:56.64 +62:15:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:36.31 +61:08:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:44.68 +63:34:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:54.86 +59:41:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:27.57 +59:27:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:01.63 +59:58:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:06.00 +59:42:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:22.35 +61:16:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:31.51 +60:49:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:34.47 +57:48:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:02.88 +62:04:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:07.34 +59:53:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:14.59 +60:19:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:04.61 +62:34:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:20.64 +60:14:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:25.46 +60:01:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:38.33 +63:19:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:00.97 +60:10:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:39.42 +59:02:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:40.75 +59:33:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:50.88 +60:06:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:58.15 +59:29:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:23.12 +59:33:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:27.96 +63:36:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:49.85 +62:50:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:05.63 +61:59:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:09.12 +61:32:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:10.96 +59:36:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:34.60 +60:01:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:41.63 +60:27:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:12.85 +61:16:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:22.79 +61:41:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:30.54 +58:02:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:35.72 +60:32:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:06.34 +59:58:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:07.22 +60:12:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:16.42 +60:57:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:20.25 +61:27:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:02.55 +59:41:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:45.28 +61:18:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:58.99 +57:43:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:59.51 +63:11:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:46.33 +61:14:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:47.04 +59:24:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:49.02 +62:46:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:52.29 +58:28:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:09.63 +60:59:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:28.98 +61:17:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:48.39 +58:09:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:59.09 +61:09:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:11.93 +62:50:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:40.39 +64:31:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:27.36 +60:45:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:44.00 +57:57:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:55.66 +61:01:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:21.65 +60:37:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:28.70 +60:34:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:12.20 +60:00:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:15.07 +58:14:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:20.99 +58:11:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:02.51 +59:46:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:24.05 +61:12:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:25.66 +58:49:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:27.45 +58:38:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:44.10 +58:30:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:56.14 +58:56:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:02.95 +61:54:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:25.02 +65:16:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:29.97 +65:09:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:00.46 +59:26:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:06.92 +57:56:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:17.16 +58:43:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:17.42 +62:09:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:29.06 +58:26:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:40.34 +59:47:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:48.64 +58:27:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:56.51 +61:34:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:04.41 +59:18:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:11.11 +58:16:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:17.90 +60:40:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:19.06 +59:38:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:26.29 +60:22:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:03.19 +60:18:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:52.71 +58:55:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:26.85 +59:20:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:39.89 +62:00:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:50.64 +59:17:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:26.62 +57:51:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:40.02 +60:56:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:47.42 +58:37:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:53.53 +63:26:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:02.35 +59:36:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:07.07 +59:13:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:07.71 +59:52:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:37.98 +64:44:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:43.15 +60:08:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:15.25 +58:45:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:15.49 +59:42:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:13.05 +59:33:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:38.03 +59:15:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:57.28 +63:00:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:04.38 +58:53:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:29.35 +60:09:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:37.12 +63:40:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:53.87 +61:23:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:07.36 +58:48:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:34.07 +63:37:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:39.67 +58:16:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:41.75 +63:32:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:21.98 +58:20:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:23.29 +64:54:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:30.18 +62:28:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:26.30 +59:44:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:05.39 +62:09:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:11.53 +61:55:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:23.72 +64:38:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:04.99 +57:50:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:33.12 +58:39:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:41.72 +58:47:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:53.83 +58:37:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:50.69 +59:21:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:48.66 +59:05:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:00.59 +60:08:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:20.59 +64:11:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:28.25 +62:23:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:40.28 +65:08:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:53.24 +65:54:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:57.98 +64:54:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:12.40 +65:14:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:03.79 +58:28:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:10.49 +58:07:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:20.97 +63:07:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:01.71 +61:10:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:07.65 +58:18:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:05:53.86 +59:06:25.2 -- not a known variable star
01:06:13.06 +59:33:47.0 -- not a known variable star
01:06:16.00 +57:53:25.1 -- not a known variable star
01:06:45.13 +60:27:55.0 -- not a known variable star
01:06:49.17 +60:52:38.6 -- not a known variable star
01:06:52.62 +62:05:00.8 -- not a known variable star
01:06:59.51 +61:28:40.4 -- a known variable star
01:07:01.45 +59:43:01.3 -- not a known variable star
01:07:31.78 +61:28:29.6 -- not a known variable star
01:07:36.77 +58:09:25.4 -- not a known variable star
01:07:39.20 +59:59:18.4 -- not a known variable star
01:07:40.29 +57:36:50.0 -- not a known variable star
01:07:57.66 +60:18:17.7 -- not a known variable star
01:08:06.01 +61:33:37.1 -- a known variable star
01:08:25.45 +59:48:03.8 -- not a known variable star
01:08:36.65 +60:44:55.0 -- not a known variable star
01:08:39.03 +60:32:42.2 -- not a known variable star
01:08:59.24 +60:47:20.7 -- not a known variable star
01:09:22.73 +57:26:31.5 -- not a known variable star
01:09:58.01 +59:03:02.1 -- a known variable star
01:10:05.00 +57:48:02.6 -- not a known variable star
01:10:43.79 +60:59:19.0 -- not a known variable star
01:11:16.45 +58:55:56.1 -- not a known variable star
01:12:00.91 +64:42:20.0 -- a known variable star
01:12:09.67 +58:47:54.3 -- not a known variable star
01:12:27.12 +58:01:05.5 -- not a known variable star
01:12:41.15 +61:18:07.7 -- not a known variable star
01:12:59.89 +57:33:53.5 -- not a known variable star
01:13:10.72 +58:11:20.8 -- not a known variable star
01:13:19.97 +61:29:38.9 -- a known variable star
01:13:34.72 +58:01:48.7 -- not a known variable star
01:13:38.99 +58:10:51.5 -- not a known variable star
01:13:56.67 +59:30:04.6 -- not a known variable star
01:14:36.05 +59:51:11.4 -- a known variable star
01:15:31.02 +60:11:14.3 -- not a known variable star
01:16:16.54 +59:38:19.7 -- a known variable star
01:16:20.25 +58:49:31.5 -- not a known variable star
01:16:56.61 +59:03:13.9 -- a known variable star
01:17:26.20 +61:54:16.6 -- not a known variable star
01:17:35.37 +59:21:38.7 -- not a known variable star
01:18:28.11 +58:11:23.7 -- not a known variable star
01:18:31.18 +60:17:31.5 -- not a known variable star
01:18:32.34 +57:50:16.0 -- a known variable star
01:18:48.45 +64:12:21.9 -- not a known variable star
01:19:08.74 +60:17:20.1 -- not a known variable star
01:19:11.81 +59:07:32.7 -- not a known variable star
01:19:21.39 +58:01:15.4 -- a known variable star
01:19:29.22 +59:25:22.7 -- not a known variable star
01:19:29.37 +60:17:35.0 -- not a known variable star
01:19:47.70 +60:24:29.9 -- not a known variable star
01:20:13.79 +65:31:27.3 -- a known variable star
01:20:35.08 +64:02:26.5 -- not a known variable star
01:20:38.69 +59:28:19.0 -- a known variable star
01:21:45.28 +58:34:14.7 -- a known variable star
01:22:13.58 +59:52:27.1 -- not a known variable star
01:22:23.83 +61:13:51.2 -- a known variable star
01:22:24.79 +62:39:02.2 -- not a known variable star
01:22:33.22 +60:44:43.0 -- not a known variable star
01:22:37.56 +58:29:18.7 -- not a known variable star
01:22:54.68 +58:55:22.5 -- not a known variable star
01:23:22.18 +60:18:16.6 -- a known variable star
01:23:32.35 +60:58:47.9 -- not a known variable star
01:23:56.64 +62:15:29.2 -- not a known variable star
01:24:36.31 +61:08:54.9 -- a known variable star
01:24:44.68 +63:34:17.1 -- not a known variable star
01:24:54.86 +59:41:45.2 -- not a known variable star
01:25:27.57 +59:27:15.1 -- a known variable star
01:26:01.63 +59:58:53.0 -- not a known variable star
01:26:06.00 +59:42:39.7 -- not a known variable star
01:26:22.35 +61:16:28.9 -- a known variable star
01:26:31.51 +60:49:34.2 -- not a known variable star
01:27:34.47 +57:48:26.0 -- not a known variable star
01:28:02.88 +62:04:06.1 -- not a known variable star
01:28:07.34 +59:53:51.6 -- not a known variable star
01:28:14.59 +60:19:20.9 -- a known variable star
01:29:04.61 +62:34:45.2 -- not a known variable star
01:29:20.64 +60:14:12.4 -- a known variable star
01:29:25.46 +60:01:31.9 -- not a known variable star
01:29:38.33 +63:19:38.0 -- a known variable star
01:30:00.97 +60:10:50.2 -- a known variable star
01:30:39.42 +59:02:43.7 -- a known variable star
01:30:40.75 +59:33:48.0 -- not a known variable star
01:30:50.88 +60:06:03.4 -- not a known variable star
01:30:58.15 +59:29:29.4 -- not a known variable star
01:31:23.12 +59:33:43.4 -- not a known variable star
01:31:27.96 +63:36:57.8 -- a known variable star
01:31:49.85 +62:50:13.0 -- not a known variable star
01:32:05.63 +61:59:26.8 -- not a known variable star
01:32:09.12 +61:32:10.9 -- not a known variable star
01:32:10.96 +59:36:02.6 -- not a known variable star
01:32:34.60 +60:01:12.0 -- not a known variable star
01:32:41.63 +60:27:01.5 -- a known variable star
01:33:12.85 +61:16:55.2 -- not a known variable star
01:33:22.79 +61:41:09.1 -- not a known variable star
01:33:30.54 +58:02:22.0 -- not a known variable star
01:33:35.72 +60:32:28.6 -- a known variable star
01:34:06.34 +59:58:54.2 -- not a known variable star
01:34:07.22 +60:12:52.5 -- not a known variable star
01:34:16.42 +60:57:34.8 -- not a known variable star
01:34:20.25 +61:27:01.2 -- a known variable star
01:35:02.55 +59:41:35.0 -- not a known variable star
01:35:45.28 +61:18:34.4 -- not a known variable star
01:35:58.99 +57:43:50.5 -- a known variable star
01:35:59.51 +63:11:54.3 -- not a known variable star
01:36:46.33 +61:14:49.6 -- not a known variable star
01:36:47.04 +59:24:04.7 -- not a known variable star
01:36:49.02 +62:46:52.5 -- a known variable star
01:36:52.29 +58:28:35.9 -- not a known variable star
01:37:09.63 +60:59:35.3 -- not a known variable star
01:37:28.98 +61:17:47.1 -- a known variable star
01:37:48.39 +58:09:09.1 -- not a known variable star
01:37:59.09 +61:09:38.8 -- a known variable star
01:38:11.93 +62:50:30.9 -- not a known variable star
01:38:40.39 +64:31:56.4 -- a known variable star
01:39:27.36 +60:45:14.3 -- not a known variable star
01:39:44.00 +57:57:02.6 -- not a known variable star
01:39:55.66 +61:01:23.9 -- not a known variable star
01:40:21.65 +60:37:45.8 -- a known variable star
01:40:28.70 +60:34:45.2 -- not a known variable star
01:41:12.20 +60:00:52.4 -- not a known variable star
01:41:15.07 +58:14:31.5 -- a known variable star
01:41:20.99 +58:11:50.9 -- not a known variable star
01:42:02.51 +59:46:32.9 -- not a known variable star
01:43:24.05 +61:12:07.1 -- a known variable star
01:43:25.66 +58:49:24.8 -- not a known variable star
01:43:27.45 +58:38:06.5 -- a known variable star
01:43:44.10 +58:30:28.3 -- not a known variable star
01:43:56.14 +58:56:40.5 -- not a known variable star
01:44:02.95 +61:54:45.6 -- not a known variable star
01:44:25.02 +65:16:03.2 -- not a known variable star
01:44:29.97 +65:09:24.4 -- a known variable star
01:45:00.46 +59:26:56.3 -- not a known variable star
01:45:06.92 +57:56:34.9 -- not a known variable star
01:45:17.16 +58:43:30.6 -- a known variable star
01:45:17.42 +62:09:43.0 -- not a known variable star
01:45:29.06 +58:26:32.6 -- a known variable star
01:45:40.34 +59:47:00.0 -- not a known variable star
01:46:48.64 +58:27:31.2 -- not a known variable star
01:46:56.51 +61:34:41.2 -- not a known variable star
01:47:04.41 +59:18:56.1 -- not a known variable star
01:47:11.11 +58:16:20.0 -- not a known variable star
01:48:17.90 +60:40:25.2 -- a known variable star
01:48:19.06 +59:38:19.2 -- not a known variable star
01:48:26.29 +60:22:28.9 -- not a known variable star
01:49:03.19 +60:18:50.1 -- a known variable star
01:49:52.71 +58:55:20.4 -- not a known variable star
01:50:26.85 +59:20:13.4 -- not a known variable star
01:50:39.89 +62:00:56.0 -- not a known variable star
01:50:50.64 +59:17:02.3 -- not a known variable star
01:51:26.62 +57:51:36.8 -- not a known variable star
01:51:40.02 +60:56:16.7 -- not a known variable star
01:51:47.42 +58:37:58.5 -- not a known variable star
01:51:53.53 +63:26:22.3 -- a known variable star
01:52:02.35 +59:36:20.4 -- not a known variable star
01:52:07.07 +59:13:07.6 -- a known variable star
01:52:07.71 +59:52:59.5 -- not a known variable star
01:53:37.98 +64:44:10.2 -- a known variable star
01:53:43.15 +60:08:00.1 -- a known variable star
01:55:15.25 +58:45:57.8 -- a known variable star
01:55:15.49 +59:42:12.6 -- a known variable star
01:56:13.05 +59:33:49.7 -- not a known variable star
01:56:38.03 +59:15:34.2 -- a known variable star
01:56:57.28 +63:00:32.6 -- not a known variable star
01:57:04.38 +58:53:27.3 -- not a known variable star
01:57:29.35 +60:09:19.2 -- not a known variable star
01:58:37.12 +63:40:15.0 -- not a known variable star
01:58:53.87 +61:23:25.6 -- not a known variable star
01:59:07.36 +58:48:33.4 -- not a known variable star
01:59:34.07 +63:37:08.7 -- not a known variable star
01:59:39.67 +58:16:32.4 -- not a known variable star
01:59:41.75 +63:32:25.4 -- not a known variable star
02:00:21.98 +58:20:18.3 -- not a known variable star
02:00:23.29 +64:54:51.9 -- not a known variable star
02:00:30.18 +62:28:28.3 -- not a known variable star
02:01:26.30 +59:44:32.4 -- not a known variable star
02:02:05.39 +62:09:27.7 -- not a known variable star
02:02:11.53 +61:55:31.4 -- not a known variable star
02:02:23.72 +64:38:25.5 -- a known variable star
02:03:04.99 +57:50:13.7 -- a known variable star
02:03:33.12 +58:39:09.8 -- not a known variable star
02:03:41.72 +58:47:26.1 -- a known variable star
02:07:53.83 +58:37:40.5 -- not a known variable star
02:08:50.69 +59:21:19.8 -- not a known variable star
02:09:48.66 +59:05:18.0 -- not a known variable star
02:11:00.59 +60:08:50.5 -- not a known variable star
02:12:20.59 +64:11:16.0 -- a known variable star
02:12:28.25 +62:23:03.9 -- not a known variable star
02:13:40.28 +65:08:15.5 -- not a known variable star
02:13:53.24 +65:54:40.5 -- not a known variable star
02:13:57.98 +64:54:41.5 -- not a known variable star
02:14:12.40 +65:14:53.8 -- not a known variable star
02:15:03.79 +58:28:54.1 -- a known variable star
02:15:10.49 +58:07:01.8 -- not a known variable star
02:15:20.97 +63:07:35.0 -- not a known variable star
02:16:01.71 +61:10:48.8 -- not a known variable star
02:16:07.65 +58:18:13.6 -- a known variable star
Found 142 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
196 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 196 (excluding asteroids and hot pixels, 142 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461213.90560589 -observatory V36
07:42:41.01 +21:01:17.8 Mercury (1.0mag)
08:52:01.68 +19:37:60.0 Venus (-4.0mag)
03:31:09.62 +18:38:01.2 Mars (1.3mag)
08:00:36.93 +20:59:10.4 Jupiter (-1.8mag)
00:52:55.66 +03:07:20.8 Saturn (0.8mag)
04:03:29.64 +20:34:46.8 Uranus (5.8mag)
00:16:47.03 +00:20:09.7 Neptune (7.8mag)
20:32:25.49 -23:10:13.5 Pluto (14.5mag)
12:16:27.00 -05:40:28.3 Moon (-10.5mag)
-rw-r--r-- 1 apache apache 362 Jun 22 05:51 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461213.90560589:
08:00:39.23 +20:59:05.0 Io (6.2mag)
08:00:37.03 +20:59:12.2 Europa (6.3mag)
08:00:22.00 +20:59:59.2 Ganymede (5.6mag)
08:01:07.72 +20:57:30.8 Callisto (6.9mag)
08:00:04.31 +20:37:34.0 Himalia (15.6mag)
08:00:41.46 +20:58:55.1 Thebe (16.6mag)
07:59:41.10 +20:47:16.4 Elara (17.6mag)
08:03:28.45 +21:03:05.8 Pasiphae (17.8mag)
08:06:32.14 +21:02:06.6 Carme (18.9mag)
00:52:44.75 +03:07:36.3 Titan (8.6mag)
00:52:51.01 +03:07:23.9 Rhea (9.9mag)
00:53:04.76 +03:09:33.8 Iapetus (11.3mag)
00:52:50.34 +03:07:50.5 Hyperion (14.6mag)
00:53:20.01 +03:07:13.0 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jun 22 05:51 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461213.90560589:
17:29:15.14 -35:24:08.1 JWST
17:30:08.65 +37:57:18.6 Chandra
03:45:20.95 +58:16:20.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 22 05:51 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461213.90560589 -observatory V36
18:32:37.83 -33:35:15.9 13.6mag P/2010 H2 (Vales)
06:07:37.66 -67:59:42.1 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:54:19.32 +32:09:52.1 17.6mag C/2017 K2 (PANSTARRS)
17:09:08.77 +15:52:55.6 17.9mag C/2021 G2 (ATLAS)
23:33:07.85 -32:05:03.6 15.7mag P/2021 N1 (ZTF)
23:08:20.17 +32:02:59.4 17.2mag C/2022 E2 (ATLAS)
05:51:19.03 +27:00:41.9 16.6mag C/2022 N2 (PANSTARRS)
09:40:31.48 +30:32:46.4 16.7mag C/2022 QE78 (ATLAS)
08:58:35.59 +04:31:00.6 17.8mag C/2022 R6 (PANSTARRS)
18:18:47.94 +21:41:35.6 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:14:55.09 -11:05:31.9 17.6mag P/2023 B1 (PANSTARRS)
22:06:49.49 +67:16:03.0 17.8mag C/2023 H5 (Lemmon)
17:11:07.37 -08:09:27.9 13.7mag C/2023 R1 (PANSTARRS)
13:18:22.75 +79:38:25.3 18.0mag C/2023 X2 (Lemmon)
07:31:16.81 +64:50:56.4 17.8mag C/2024 A1 (ATLAS)
07:08:12.79 +28:56:49.9 14.1mag C/2024 E1 (Wierzchos)
15:26:50.80 +14:33:56.9 17.4mag C/2024 G6 (ATLAS)
20:01:29.95 +35:10:29.5 13.9mag C/2024 J3 (ATLAS)
04:32:12.87 -14:49:59.6 15.9mag C/2024 T5 (ATLAS)
06:18:58.65 +32:03:53.8 17.9mag C/2025 J1 (Borisov)
11:32:07.54 +51:52:34.0 17.9mag C/2025 L1 (ATLAS)
06:59:54.22 -11:35:25.4 15.3mag C/2025 R3 (PANSTARRS)
09:36:56.27 +23:03:24.2 17.8mag C/2025 V2 (Rankin)
12:40:27.91 +04:30:47.3 17.1mag C/2025 Y1 (ATLAS)
17:43:12.37 +77:40:39.5 17.7mag C/2026 A2 (Bok)
02:23:26.66 +44:19:52.3 16.4mag C/2026 B2 (Sun-Gao)
11:15:53.15 +00:37:04.2 16.7mag A/2026 E1
20:48:58.96 -10:18:42.0 8.0mag 10P/Tempel
11:06:08.46 -01:15:44.5 16.1mag 29P/Schwassmann-Wachmann
03:33:31.78 +27:28:16.2 17.7mag 47P/Ashbrook-Jackson
09:30:15.14 +19:35:18.8 16.9mag 63P/Wild
00:38:01.91 -05:35:59.5 15.6mag 65P/Gunn
07:29:37.71 +34:22:10.4 17.3mag 76P/West-Kohoutek-Ikemura
03:43:42.67 +18:49:12.9 13.8mag 78P/Gehrels
01:50:05.96 +07:42:18.4 15.9mag 88P/Howell
05:40:08.48 +30:56:09.2 15.4mag 93P/Lovas
03:24:36.24 +29:37:29.9 17.3mag 114P/Wiseman-Skiff
07:24:49.99 +32:17:57.0 15.4mag 123P/West-Hartley
10:15:18.82 +08:36:38.5 16.6mag 124P/Mrkos
04:22:28.52 +20:05:22.3 16.3mag 128P/Shoemaker-Holt
05:01:39.29 +19:34:20.2 17.8mag 131P/Mueller
06:55:04.92 +16:35:51.8 16.4mag 141P/Machholz
06:58:53.26 +17:49:38.3 16.4mag 141P-A/Machholz
06:02:21.78 +17:22:18.2 13.2mag 141P-D/Machholz
03:07:11.10 -22:53:48.3 16.3mag 161P/Hartley-IRAS
04:29:31.08 +29:00:47.7 15.1mag 162P/SidingSpring
19:31:06.16 +06:29:34.9 16.0mag 169P/NEAT
00:56:00.58 +05:03:16.4 17.8mag 220P/McNaught
16:42:31.26 -08:04:52.8 16.6mag 235P/LINEAR
08:06:27.72 +34:43:20.8 17.7mag 240P/NEAT
01:10:05.65 +03:46:53.1 16.0mag 260P/McNaught
04:44:02.37 +34:48:04.7 17.5mag 295P/LINEAR
01:03:44.28 +05:00:46.6 18.0mag 320P/McNaught
15:09:51.95 +07:24:51.9 17.5mag 391P/Kowalski
08:18:52.27 +20:19:55.8 17.9mag 450P/LONEOS
07:23:05.48 +40:38:51.9 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 22 05:51 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 22 05:51 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 22 05:51 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:14:06.106 -11:08:18.15 AT 2026pee 2026-06-11.44 20.4029
21:31:13.883 +04:04:18.31 AT 2026ped 2026-06-14.41 14.1027
20:54:11.027 -17:40:35.49 SN 2026pec 2026-06-10.43 20.2794
22:58:51.251 +07:13:59.21 AT 2026peb 2026-06-10.41 19.9741
00:52:47.343 -02:41:38.57 AT 2026pea 2026-06-13.47 20.2545
11:04:44.817 +45:14:11.22 AT 2026pdz 2026-06-11.28 19.51
17:09:03.949 +56:34:07.30 AT 2026pdy 2026-06-12.37 20.61
10:19:45.260 +42:02:36.17 AT 2026pdx 2026-06-14.27 19.92
10:28:08.632 +39:13:49.12 AT 2026pdw 2026-06-14.27 20.76
14:13:16.283 +48:39:44.66 AT 2026pdv 2026-06-14.28 20.99
17:23:28.371 +30:40:11.58 AT 2026pdu 2026-06-14.39 21.05
01:33:49.397 +35:17:20.49 AT 2026pdt 2026-06-14.47 19.9212
21:13:42.065 -02:21:55.88 AT 2026pds 2026-06-14.43 19.2907
16:22:58.748 -03:23:44.29 AT 2026pdr 2026-06-14.30 19.949
23:21:42.174 -06:08:29.93 SN 2026pdq 2026-06-14.21 19.2
23:13:31.599 +74:22:22.00 AT 2026pdp 2026-05-11.44 19.8851
20:13:16.456 -24:45:05.98 AT 2026pdo 2026-06-08.44 19.9371
20:00:27.602 -27:22:34.43 AT 2026pdn 2026-06-12.42 20.0708
00:56:08.209 +05:40:25.40 AT 2026pdm 2026-06-13.47 20.1547
22:23:01.922 -16:35:38.00 AT 2026pdl 2026-06-10.41 19.9219
-rw-r--r-- 1 apache apache 30K Jun 22 05:51 tns_transients_list.txt
