This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9
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 05 28.3618 2461188.8618 9.36 02:01:28.10 +58:18:15.0
132.04169 -3.32352 galactic Cas Second-epoch detections are separated by 0.1" and 7.4 pix
The object was found in VSX 1" V0666 Cas
Type: M
# Max. Min./Amp. JD0 Period
10.000 V 13.800 V 2454515.40000 432.100000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:28.10 +58:18:15.0: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:28.10 +58:18:15.0: 10.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.43 +/- 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 05 28.3618* 02 01 28.10 +58 18 15.0 9.4 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
V0666 Cas,2461188.8618,9.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0666 Cas 20260528.3618 9.36CV 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 05 28.3618 2461188.8618 10.15 02:00:57.02 +58:36:59.3
131.89274 -3.04067 galactic Cas Second-epoch detections are separated by 0.5" and 7.5 pix
The object was found in VSX 1" V0924 Cas
Type: SR
# Max. Min./Amp. JD0 Period
11.300 V 13.500 V 2451480.00000 230.000000000000 : M7
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:57.02 +58:36:59.3: 14.61 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:57.02 +58:36:59.3: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 00 57.02 +58 36 59.3 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0924 Cas,2461188.8618,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0924 Cas 20260528.3618 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 10.51 01:16:12.04 +59:15:22.9
126.09782 -3.46309 galactic Cas Second-epoch detections are separated by 0.7" and 7.9 pix
The object was found in VSX 1" HX Cas
Type: LB
# Max. Min./Amp. JD0 Period
14.100 pg 15.000 pg M3
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:12.04 +59:15:22.9: 13.51 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:12.04 +59:15:22.9: 11.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 16 12.04 +59 15 22.9 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
HX Cas,2461188.8618,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HX Cas 20260528.3618 10.51CV 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 05 28.3618 2461188.8618 9.71 02:03:23.58 +57:43:21.9
132.44581 -3.81376 galactic Per Second-epoch detections are separated by 1.1" and 7.4 pix
The object was found in VSX 1" CF Per
Type: ISB
# Max. Min./Amp. JD0 Period
10.500 V 12.500 V M6
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:23.58 +57:43:21.9: 14.71 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:23.58 +57:43:21.9: 10.66 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.66 +/- 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 05 28.3618* 02 03 23.58 +57 43 21.9 9.7 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
CF Per,2461188.8618,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CF Per 20260528.3618 9.71CV 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 05 28.3618 2461188.8618 10.35 01:23:00.77 +64:39:24.1
126.30406 1.99188 galactic Cas Second-epoch detections are separated by 0.1" and 7.7 pix
The object was found in VSX 1" V0900 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
11.100 V 12.300 V 120.000000000000 :
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:00.77 +64:39:24.1: 11.62 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:00.77 +64:39:24.1: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.39 +/- 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 05 28.3618* 01 23 00.77 +64 39 24.1 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0900 Cas,2461188.8618,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0900 Cas 20260528.3618 10.35CV 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 05 28.3618 2461188.8618 8.67 01:56:38.06 +59:15:34.2
131.18807 -2.56316 galactic Cas Second-epoch detections are separated by 0.3" and 7.6 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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.06 +59:15:34.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.06 +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 05 28.3618* 01 56 38.06 +59 15 34.2 8.7 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
X Cas,2461188.8618,8.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3618 8.67CV 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 05 28.3618 2461188.8618 9.09 01:43:36.46 +58:48:08.9
129.65672 -3.38644 galactic Cas Second-epoch detections are separated by 0.4" and 7.7 pix
The object was found in VSX 1" V0917 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
10.500 V 11.200 V M7
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:36.46 +58:48:08.9: 14.68 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:36.46 +58:48:08.9: 10.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.22 +/- 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 05 28.3618* 01 43 36.46 +58 48 08.9 9.1 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
V0917 Cas,2461188.8618,9.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0917 Cas 20260528.3618 9.09CV 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 05 28.3618 2461188.8618 9.70 01:29:35.29 +65:02:04.9
126.94585 2.46069 galactic Cas Second-epoch detections are separated by 0.3" and 7.6 pix
The object was found in VSX 1" V0905 Cas
Type: SR
# Max. Min./Amp. JD0 Period
11.300 V 12.500 V 2458365.80790 177.614155000000 M7
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:35.29 +65:02:04.9: 11.89 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:35.29 +65:02:04.9: 10.79 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.92 +/- 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 05 28.3618* 01 29 35.29 +65 02 04.9 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0905 Cas,2461188.8618,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0905 Cas 20260528.3618 9.70CV 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 05 28.3618 2461188.8618 9.21 02:21:40.62 +60:54:41.8
133.68129 -0.06279 galactic Cas Second-epoch detections are separated by 0.7" and 7.1 pix
The object was found in VSX 2" DE Cas
Type: SRB
# Max. Min./Amp. JD0 Period
13.900 pg 15.100 pg 2428925.00000 151.000000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:40.62 +60:54:41.8: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:40.62 +60:54:41.8: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 21 40.62 +60 54 41.8 9.2 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
DE Cas,2461188.8618,9.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DE Cas 20260528.3618 9.21CV 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 05 28.3618 2461188.8618 9.86 01:43:02.78 +61:34:06.4
129.03491 -0.69026 galactic Cas Second-epoch detections are separated by 1.7" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:43:02.78 +61:34:06.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:02.78 +61:34:06.4: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:02.78 +61:34:06.4: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 43 02.78 +61 34 06.4 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461188.8618,9.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260528.3618 9.86CV 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 05 28.3618 2461188.8618 10.10 00:51:08.53 +64:31:35.6
122.90010 1.65483 galactic Cas Second-epoch detections are separated by 1.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:51:08.53 +64:31:35.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:08.53 +64:31:35.6: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:08.53 +64:31:35.6: 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 05 28.3618* 00 51 08.53 +64 31 35.6 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
target,2461188.8618,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260528.3618 10.10CV 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 05 28.3618 2461188.8618 9.70 02:00:14.31 +65:03:58.2
130.10416 3.15688 galactic Cas Second-epoch detections are separated by 8.2" and 8.3 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 518142144475250304 | 02:00:13.19 +65:04:05.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:14.31 +65:03:58.2: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:14.31 +65:03:58.2: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 05 28.3618* 02 00 14.31 +65 03 58.2 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 518142144475250304,2461188.8618,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518142144475250304 20260528.3618 9.70CV 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 05 28.3618 2461188.8618 9.52 01:02:16.17 +57:08:41.8
124.40790 -5.69576 galactic Cas Second-epoch detections are separated by 2.1" and 8.0 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 J015.5600+57.1456 | 01:02:16.30 +57:08:43.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.376+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:16.17 +57:08:41.8: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:16.17 +57:08:41.8: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 02 16.17 +57 08 41.8 9.5 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 J015.5600+57.1456,2461188.8618,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015.5600+57.1456 20260528.3618 9.52CV 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 05 28.3618 2461188.8618 9.52 01:25:39.69 +59:16:07.4
127.29937 -3.31251 galactic Cas Second-epoch detections are separated by 3.4" and 8.4 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 510043588502369152 | 01:25:40.25 +59:16:13.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:39.69 +59:16:07.4: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:39.69 +59:16:07.4: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 25 39.69 +59 16 07.4 9.5 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 510043588502369152,2461188.8618,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510043588502369152 20260528.3618 9.52CV 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 05 28.3618 2461188.8618 8.86 02:19:45.31 +57:01:15.4
134.76503 -3.80788 galactic Per Second-epoch detections are separated by 4.7" 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 458361216240219648 | 02:19:47.59 +57:00:57.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:45.31 +57:01:15.4: 12.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:45.31 +57:01:15.4: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 19 45.31 +57 01 15.4 8.9 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 458361216240219648,2461188.8618,8.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458361216240219648 20260528.3618 8.86CV 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 05 28.3618 2461188.8618 8.98 01:46:35.86 +59:12:14.3
129.95076 -2.91401 galactic Cas Second-epoch detections are separated by 4.4" 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 | ATO J026.6424+59.1944 | 01:46:35.28 +59:12:16.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1955ApJS....2..123F LF 5 +58 79
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:35.86 +59:12:14.3: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:35.86 +59:12:14.3: 11.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 46 35.86 +59 12 14.3 9.0 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 J026.6424+59.1944,2461188.8618,8.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J026.6424+59.1944 20260528.3618 8.98CV 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 05 28.3618 2461188.8618 9.35 02:03:11.16 +62:07:52.0
131.20927 0.41794 galactic Cas Second-epoch detections are separated by 3.8" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 508769529401745152 | 02:03:12.42 +62:07:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:11.16 +62:07:52.0: 12.64 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:11.16 +62:07:52.0: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 03 11.16 +62 07 52.0 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508769529401745152,2461188.8618,9.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508769529401745152 20260528.3618 9.35CV 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 05 28.3618 2461188.8618 9.56 00:36:55.23 +62:40:46.4
121.26704 -0.14525 galactic Cas Second-epoch detections are separated by 1.4" and 8.3 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 430706329831264640 | 00:36:57.75 +62:40:57.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:36:55.23 +62:40:46.4: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:36:55.23 +62:40:46.4: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 00 36 55.23 +62 40 46.4 9.6 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 430706329831264640,2461188.8618,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430706329831264640 20260528.3618 9.56CV 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 05 28.3618 2461188.8618 8.85 00:51:15.99 +58:39:34.3
122.90957 -4.21221 galactic Cas Second-epoch detections are separated by 1.1" and 8.3 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 424454815954175488 | 00:51:16.26 +58:39:31.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:15.99 +58:39:34.3: 9.19 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:15.99 +58:39:34.3: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 00 51 15.99 +58 39 34.3 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
Gaia DR3 424454815954175488,2461188.8618,8.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424454815954175488 20260528.3618 8.85CV 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 05 28.3618 2461188.8618 6.76 02:25:27.64 +56:46:55.8
135.58023 -3.76280 galactic Per 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 | ATO J036.3787+56.7792 | 02:25:27.69 +56:46:54.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.194+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:27.64 +56:46:55.8: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:27.64 +56:46:55.8: 9.68 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.68 +/- 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 05 28.3618* 02 25 27.64 +56 46 55.8 6.8 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 J036.3787+56.7792,2461188.8618,6.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J036.3787+56.7792 20260528.3618 6.76CV 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 05 28.3618 2461188.8618 6.95 02:29:09.02 +56:37:12.7
136.11205 -3.73030 galactic Per 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 | Large-amplitude variable Gaia DR2 457593928911905280 | 02:29:09.04 +56:37:12.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A0V 1966POHP....8...25F BD+55 629 J-Ks=0.123+/-0.029 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:09.02 +56:37:12.7: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:09.02 +56:37:12.7: 9.25 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.25 +/- 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 05 28.3618* 02 29 09.02 +56 37 12.7 7.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457593928911905280,2461188.8618,6.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457593928911905280 20260528.3618 6.95CV 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 05 28.3618 2461188.8618 7.00 02:18:53.85 +57:08:41.8
134.61348 -3.72987 galactic Per Second-epoch detections are separated by 2.5" and 7.4 pix
The object was found in VSX20" V0613 Per
Type: BE
# Max. Min./Amp. JD0 Period
9.500 V Y 0.010 V B2V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:53.85 +57:08:41.8: 12.05 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:53.85 +57:08:41.8: 11.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.38 +/- 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 05 28.3618* 02 18 53.85 +57 08 41.8 7.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0613 Per,2461188.8618,7.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0613 Per 20260528.3618 7.00CV 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 05 28.3618 2461188.8618 6.97 02:32:05.67 +56:39:57.3
136.47101 -3.53653 galactic Per Second-epoch detections are separated by 2.5" 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 | ATO J038.0368+56.6612 | 02:32:05.04 +56:39:58.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB 1951ApJ...113..141N HD 15548
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:05.67 +56:39:57.3: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:05.67 +56:39:57.3: 9.30 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.30 +/- 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 05 28.3618* 02 32 05.67 +56 39 57.3 7.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.0368+56.6612,2461188.8618,6.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.0368+56.6612 20260528.3618 6.97CV 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 05 28.3618 2461188.8618 7.05 02:27:58.38 +56:02:38.8
136.17176 -4.32607 galactic Per 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 | ATO J037.0041+56.0452 | 02:27:58.37 +56:02:38.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A8V 1935ApJ....81..187A HD 15091 J-Ks=0.127+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:58.38 +56:02:38.8: 12.05 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:58.38 +56:02:38.8: 9.41 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.41 +/- 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 05 28.3618* 02 27 58.38 +56 02 38.8 7.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.0041+56.0452,2461188.8618,7.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.0041+56.0452 20260528.3618 7.05CV 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 05 28.3618 2461188.8618 7.17 02:31:26.37 +55:59:07.4
136.64470 -4.20086 galactic Per Second-epoch detections are separated by 4.9" and 7.3 pix
The object was found in VSX22" Gaia DR3 457343205908261760
Type: ROT
# Max. Min./Amp. JD0 Period
16.250 G 16.350 G 0.771500000000 M
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:26.37 +55:59:07.4: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:26.37 +55:59:07.4: 9.42 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.42 +/- 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 05 28.3618* 02 31 26.37 +55 59 07.4 7.2 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 457343205908261760,2461188.8618,7.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457343205908261760 20260528.3618 7.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 7.14 02:29:10.08 +56:27:14.1
136.17580 -3.88395 galactic Per 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 | Gaia DR3 457590355506120064 | 02:29:10.50 +56:27:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:10.08 +56:27:14.1: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:10.08 +56:27:14.1: 9.63 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.63 +/- 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 05 28.3618* 02 29 10.08 +56 27 14.1 7.1 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 457590355506120064,2461188.8618,7.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457590355506120064 20260528.3618 7.14CV 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 05 28.3618 2461188.8618 7.20 02:34:11.11 +55:49:59.2
137.05954 -4.19463 galactic Per Second-epoch detections are separated by 6.0" and 7.1 pix
The object was found in VSX 4" Gaia DR3 457311320070532608
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
9.230 G 9.290 G 0.086248700000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:11.11 +55:49:59.2: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:11.11 +55:49:59.2: 9.39 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.39 +/- 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 05 28.3618* 02 34 11.11 +55 49 59.2 7.2 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 457311320070532608,2461188.8618,7.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457311320070532608 20260528.3618 7.20CV 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 05 28.3618 2461188.8618 7.25 02:35:38.10 +57:29:11.6
136.59905 -2.59392 galactic Per Second-epoch detections are separated by 0.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458101181736200448 | 02:35:37.84 +57:29:13.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1928AnHar.100...49C HD 236971
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:38.10 +57:29:11.6: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:38.10 +57:29:11.6: 9.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.58 +/- 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 05 28.3618* 02 35 38.10 +57 29 11.6 7.2 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 458101181736200448,2461188.8618,7.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458101181736200448 20260528.3618 7.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 7.21 02:30:54.10 +56:14:28.3
136.47859 -3.99204 galactic Per Second-epoch detections are separated by 2.8" 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 457384093997742208 | 02:30:54.14 +56:14:26.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.003+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:54.10 +56:14:28.3: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:54.10 +56:14:28.3: 9.94 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.94 +/- 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 05 28.3618* 02 30 54.10 +56 14 28.3 7.2 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 457384093997742208,2461188.8618,7.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457384093997742208 20260528.3618 7.21CV 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 05 28.3618 2461188.8618 7.37 02:27:24.36 +56:23:03.5
135.97403 -4.03788 galactic Per Second-epoch detections are separated by 3.2" and 7.1 pix
The object was found in VSX 1" Gaia DR3 457563554909169536
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
9.480 G 9.530 G 0.595500000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:24.36 +56:23:03.5: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:24.36 +56:23:03.5: 9.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.59 +/- 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 05 28.3618* 02 27 24.36 +56 23 03.5 7.4 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 457563554909169536,2461188.8618,7.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457563554909169536 20260528.3618 7.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 7.40 02:32:05.62 +57:22:03.9
136.20447 -2.88711 galactic Per Second-epoch detections are separated by 0.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.0242+57.3766 | 02:32:05.82 +57:22:02.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.053+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:05.62 +57:22:03.9: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:05.62 +57:22:03.9: 10.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.22 +/- 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 05 28.3618* 02 32 05.62 +57 22 03.9 7.4 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
ATO J038.0242+57.3766,2461188.8618,7.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.0242+57.3766 20260528.3618 7.40CV 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 05 28.3618 2461188.8618 7.30 02:32:46.69 +56:48:22.9
136.50436 -3.37099 galactic Per 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 | ATO J038.2081+56.8041 | 02:32:46.25 +56:48:26.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B3III 1966POHP....8...25F BD+56 651
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:46.69 +56:48:22.9: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:46.69 +56:48:22.9: 9.53 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.53 +/- 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 05 28.3618* 02 32 46.69 +56 48 22.9 7.3 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 J038.2081+56.8041,2461188.8618,7.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.2081+56.8041 20260528.3618 7.30CV 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 05 28.3618 2461188.8618 7.44 02:34:35.28 +56:21:51.3
136.90520 -3.68320 galactic Per 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 | Gaia DR3 457749475453771648 | 02:34:34.64 +56:21:57.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:35.28 +56:21:51.3: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:35.28 +56:21:51.3: 9.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.59 +/- 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 05 28.3618* 02 34 35.28 +56 21 51.3 7.4 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 457749475453771648,2461188.8618,7.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457749475453771648 20260528.3618 7.44CV 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 05 28.3618 2461188.8618 7.49 02:34:44.75 +56:06:07.7
137.02746 -3.91623 galactic Per Second-epoch detections are separated by 6.7" 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 J038.6785+56.0961 | 02:34:44.47 +56:06:09.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:44.75 +56:06:07.7: 11.89 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:44.75 +56:06:07.7: 9.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.64 +/- 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 05 28.3618* 02 34 44.75 +56 06 07.7 7.5 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 J038.6785+56.0961,2461188.8618,7.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.6785+56.0961 20260528.3618 7.49CV 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 05 28.3618 2461188.8618 7.43 02:33:35.26 +55:54:24.6
136.95350 -4.15894 galactic Per Second-epoch detections are separated by 5.3" 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 | ATO J038.3939+55.9184 | 02:33:35.02 +55:54:27.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:35.26 +55:54:24.6: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:35.26 +55:54:24.6: 9.63 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.63 +/- 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 05 28.3618* 02 33 35.26 +55 54 24.6 7.4 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
ATO J038.3939+55.9184,2461188.8618,7.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.3939+55.9184 20260528.3618 7.43CV 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 05 28.3618 2461188.8618 7.37 02:37:08.74 +57:25:19.6
136.81140 -2.57313 galactic Per Second-epoch detections are separated by 1.3" 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 | ATO J039.2772+57.4158 | 02:37:08.61 +57:25:20.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.616+/-0.025 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:08.74 +57:25:19.6: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:08.74 +57:25:19.6: 9.89 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.89 +/- 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 05 28.3618* 02 37 08.74 +57 25 19.6 7.4 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
ATO J039.2772+57.4158,2461188.8618,7.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.2772+57.4158 20260528.3618 7.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 7.45 02:36:33.17 +57:54:38.3
136.54520 -2.15576 galactic Cas Second-epoch detections are separated by 0.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458140386197476352 | 02:36:33.33 +57:54:38.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.899+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:33.17 +57:54:38.3: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:33.17 +57:54:38.3: 10.12 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.12 +/- 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 05 28.3618* 02 36 33.17 +57 54 38.3 7.5 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 458140386197476352,2461188.8618,7.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458140386197476352 20260528.3618 7.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 7.43 02:27:20.52 +56:01:48.8
136.09450 -4.37107 galactic Per 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 | Gaia DR3 457461162889223552 | 02:27:20.64 +56:01:46.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:20.52 +56:01:48.8: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:20.52 +56:01:48.8: 10.19 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.19 +/- 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 05 28.3618* 02 27 20.52 +56 01 48.8 7.4 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 457461162889223552,2461188.8618,7.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457461162889223552 20260528.3618 7.43CV 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 05 28.3618 2461188.8618 7.42 02:31:26.05 +56:07:04.8
136.59387 -4.07832 galactic Per 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 | Gaia DR3 457379661591549312 | 02:31:25.96 +56:07:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:26.05 +56:07:04.8: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:26.05 +56:07:04.8: 10.53 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.53 +/- 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 05 28.3618* 02 31 26.05 +56 07 04.8 7.4 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 457379661591549312,2461188.8618,7.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457379661591549312 20260528.3618 7.42CV 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 05 28.3618 2461188.8618 7.53 02:35:52.05 +57:47:21.5
136.50904 -2.30317 galactic Cas Second-epoch detections are separated by 0.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458114582034037760 | 02:35:52.03 +57:47:22.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB 1953BOTT....1g...3G BD+57 593 J-Ks=0.224+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:52.05 +57:47:21.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:52.05 +57:47:21.5: 9.94 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.94 +/- 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 05 28.3618* 02 35 52.05 +57 47 21.5 7.5 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 458114582034037760,2461188.8618,7.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458114582034037760 20260528.3618 7.53CV 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 05 28.3618 2461188.8618 7.56 02:26:59.10 +56:01:58.1
136.04694 -4.38672 galactic Per 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 457460991090535808 | 02:26:59.15 +56:01:55.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.789+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:59.10 +56:01:58.1: 12.09 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:59.10 +56:01:58.1: 10.29 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.29 +/- 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 05 28.3618* 02 26 59.10 +56 01 58.1 7.6 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 457460991090535808,2461188.8618,7.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457460991090535808 20260528.3618 7.56CV 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 05 28.3618 2461188.8618 7.53 02:32:16.04 +56:38:48.1
136.50034 -3.54530 galactic Per 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 | Gaia DR3 457772187240678912 | 02:32:15.71 +56:38:50.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:16.04 +56:38:48.1: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:16.04 +56:38:48.1: 10.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.23 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 32 16.04 +56 38 48.1 7.5 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 457772187240678912,2461188.8618,7.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457772187240678912 20260528.3618 7.53CV 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 05 28.3618 2461188.8618 7.57 02:24:11.88 +56:35:43.2
135.48389 -3.99886 galactic Per Second-epoch detections are separated by 1.7" 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 457537269710765824 | 02:24:11.89 +56:35:43.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1966POHP....8...25F BD+55 607 J-Ks=0.116+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:11.88 +56:35:43.2: 8.76 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:11.88 +56:35:43.2: 9.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.73 +/- 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 05 28.3618* 02 24 11.88 +56 35 43.2 7.6 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 457537269710765824,2461188.8618,7.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457537269710765824 20260528.3618 7.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 7.46 02:36:29.15 +57:11:43.0
136.81926 -2.81671 galactic Per Second-epoch detections are separated by 6.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457813144048325248 | 02:36:28.37 +57:11:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1928AnHar.100...49C HD 236972
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:29.15 +57:11:43.0: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:29.15 +57:11:43.0: 9.85 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.85 +/- 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 05 28.3618* 02 36 29.15 +57 11 43.0 7.5 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 457813144048325248,2461188.8618,7.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457813144048325248 20260528.3618 7.46CV 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 05 28.3618 2461188.8618 7.50 02:33:01.83 +57:02:06.6
136.44871 -3.14637 galactic Per Second-epoch detections are separated by 0.6" and 7.2 pix
The object was found in VSX 2" GSC 03695-01369
Type: SR
# Max. Min./Amp. JD0 Period
9.750 R1 10.150 R1 2451481.00000 36.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:01.83 +57:02:06.6: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:01.83 +57:02:06.6: 10.89 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.89 +/- 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 05 28.3618* 02 33 01.83 +57 02 06.6 7.5 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
GSC 03695-01369,2461188.8618,7.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 03695-01369 20260528.3618 7.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 7.56 02:21:16.42 +57:08:40.1
134.91776 -3.62189 galactic Per Second-epoch detections are separated by 2.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458454296770820992 | 02:21:17.02 +57:08:42.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1949UppAn...3b....W NGC 884 1924
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:16.42 +57:08:40.1: 11.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:16.42 +57:08:40.1: 10.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.09 +/- 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 05 28.3618* 02 21 16.42 +57 08 40.1 7.6 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 458454296770820992,2461188.8618,7.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458454296770820992 20260528.3618 7.56CV 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 05 28.3618 2461188.8618 7.63 02:34:06.21 +56:25:27.6
136.81996 -3.65375 galactic Per Second-epoch detections are separated by 0.8" 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 | Gaia DR3 457750815483540992 | 02:34:05.68 +56:25:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:06.21 +56:25:27.6: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:06.21 +56:25:27.6: 10.12 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.12 +/- 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 05 28.3618* 02 34 06.21 +56 25 27.6 7.6 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 457750815483540992,2461188.8618,7.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457750815483540992 20260528.3618 7.63CV 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 05 28.3618 2461188.8618 7.67 02:36:36.23 +57:46:58.2
136.60189 -2.27053 galactic Cas Second-epoch detections are separated by 1.1" 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 458112864047109120 | 02:36:36.18 +57:46:59.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1928AnHar.100...49C HD 236973 J-Ks=0.098+/-0.028 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:36.23 +57:46:58.2: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:36.23 +57:46:58.2: 9.93 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.93 +/- 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 05 28.3618* 02 36 36.23 +57 46 58.2 7.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458112864047109120,2461188.8618,7.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458112864047109120 20260528.3618 7.67CV 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 05 28.3618 2461188.8618 7.62 02:20:54.00 +56:16:37.9
135.16518 -4.45489 galactic Per Second-epoch detections are separated by 0.9" and 7.5 pix
The object was found in VSX 4" ASASSN-V J022054.22+561634.7
Type: SRS
# Max. Min./Amp. JD0 Period
10.990 V 11.120 V 2457360.93000 22.473000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:54.00 +56:16:37.9: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:54.00 +56:16:37.9: 10.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.73 +/- 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 05 28.3618* 02 20 54.00 +56 16 37.9 7.6 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 J022054.22+561634.7,2461188.8618,7.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022054.22+561634.7 20260528.3618 7.62CV 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 05 28.3618 2461188.8618 7.54 02:29:12.20 +56:18:00.7
136.23722 -4.02501 galactic Per Second-epoch detections are separated by 3.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.2903+56.3099 | 02:29:12.29 +56:17:57.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:12.20 +56:18:00.7: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:12.20 +56:18:00.7: 10.25 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.25 +/- 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 05 28.3618* 02 29 12.20 +56 18 00.7 7.5 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 J037.2903+56.3099,2461188.8618,7.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.2903+56.3099 20260528.3618 7.54CV 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 05 28.3618 2461188.8618 7.74 02:22:35.24 +56:18:15.4
135.37645 -4.34922 galactic Per Second-epoch detections are separated by 1.3" 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 458276622563145984 | 02:22:35.42 +56:18:12.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:35.24 +56:18:15.4: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:35.24 +56:18:15.4: 10.42 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.42 +/- 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 05 28.3618* 02 22 35.24 +56 18 15.4 7.7 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 458276622563145984,2461188.8618,7.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458276622563145984 20260528.3618 7.74CV 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 05 28.3618 2461188.8618 7.70 02:32:55.76 +56:39:38.1
136.57931 -3.49781 galactic Per Second-epoch detections are separated by 0.9" 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 | ATO J038.2188+56.6593 | 02:32:55.49 +56:39:40.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:55.76 +56:39:38.1: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:55.76 +56:39:38.1: 10.28 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.28 +/- 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 05 28.3618* 02 32 55.76 +56 39 38.1 7.7 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 J038.2188+56.6593,2461188.8618,7.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.2188+56.6593 20260528.3618 7.70CV 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 05 28.3618 2461188.8618 7.71 02:30:44.92 +56:56:13.4
136.19772 -3.35478 galactic Per Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.6828+56.9432 | 02:30:44.89 +56:56:12.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.356+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:44.92 +56:56:13.4: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:44.92 +56:56:13.4: 10.14 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.14 +/- 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 05 28.3618* 02 30 44.92 +56 56 13.4 7.7 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 J037.6828+56.9432,2461188.8618,7.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.6828+56.9432 20260528.3618 7.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 7.91 02:37:36.90 +57:51:16.6
136.69713 -2.15128 galactic Cas Second-epoch detections are separated by 2.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.3909+57.8574 | 02:37:36.95 +57:51:15.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.719+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:36.90 +57:51:16.6: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:36.90 +57:51:16.6: 10.42 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.42 +/- 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 05 28.3618* 02 37 36.90 +57 51 16.6 7.9 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 J039.3909+57.8574,2461188.8618,7.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.3909+57.8574 20260528.3618 7.91CV 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 05 28.3618 2461188.8618 7.75 02:21:55.26 +56:25:09.3
135.24986 -4.27307 galactic Per Second-epoch detections are separated by 1.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.4640+56.4218 | 02:21:55.21 +56:25:08.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.079+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:55.26 +56:25:09.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:55.26 +56:25:09.3: 10.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 21 55.26 +56 25 09.3 7.8 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 J035.4640+56.4218,2461188.8618,7.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J035.4640+56.4218 20260528.3618 7.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 7.80 02:28:50.68 +56:20:50.4
136.17347 -3.99952 galactic Per Second-epoch detections are separated by 2.8" 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 | Gaia DR3 457554415218933120 | 02:28:50.80 +56:20:47.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:50.68 +56:20:50.4: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:50.68 +56:20:50.4: 10.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.69 +/- 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 05 28.3618* 02 28 50.68 +56 20 50.4 7.8 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 457554415218933120,2461188.8618,7.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457554415218933120 20260528.3618 7.80CV 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 05 28.3618 2461188.8618 7.79 02:31:06.61 +56:30:44.0
136.40341 -3.73000 galactic Per 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 | Gaia DR3 457581971731866368 | 02:31:06.88 +56:30:40.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:06.61 +56:30:44.0: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:06.61 +56:30:44.0: 10.51 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.51 +/- 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 05 28.3618* 02 31 06.61 +56 30 44.0 7.8 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 457581971731866368,2461188.8618,7.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457581971731866368 20260528.3618 7.79CV 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 05 28.3618 2461188.8618 7.86 02:30:12.73 +56:11:27.6
136.40829 -4.07443 galactic Per Second-epoch detections are separated by 3.1" and 7.3 pix
The object was found in VSX20" ZTF J023014.84+561117.4
Type: EW
# Max. Min./Amp. JD0 Period
18.223 r Y 0.543 r 2458387.94220 0.264294400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:12.73 +56:11:27.6: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:12.73 +56:11:27.6: 10.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.59 +/- 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 05 28.3618* 02 30 12.73 +56 11 27.6 7.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J023014.84+561117.4,2461188.8618,7.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J023014.84+561117.4 20260528.3618 7.86CV 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 05 28.3618 2461188.8618 7.91 02:24:41.97 +56:55:48.3
135.43021 -3.66135 galactic Per Second-epoch detections are separated by 2.8" 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 J036.1620+56.9296 | 02:24:42.04 +56:55:46.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.133+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:41.97 +56:55:48.3: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:41.97 +56:55:48.3: 10.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.76 +/- 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 05 28.3618* 02 24 41.97 +56 55 48.3 7.9 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 J036.1620+56.9296,2461188.8618,7.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J036.1620+56.9296 20260528.3618 7.91CV 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 05 28.3618 2461188.8618 7.95 02:31:11.88 +57:09:48.4
136.16940 -3.12200 galactic Per Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.7864+57.1721 | 02:31:12.13 +57:09:46.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.198+/-0.073 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:11.88 +57:09:48.4: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:11.88 +57:09:48.4: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.81 +/- 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 05 28.3618* 02 31 11.88 +57 09 48.4 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.7864+57.1721,2461188.8618,7.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.7864+57.1721 20260528.3618 7.95CV 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 05 28.3618 2461188.8618 7.92 02:35:34.11 +57:09:17.2
136.72071 -2.90278 galactic Per 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 | Gaia DR3 457812216335433344 | 02:35:34.20 +57:09:17.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.105+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:34.11 +57:09:17.2: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:34.11 +57:09:17.2: 10.86 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.86 +/- 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 05 28.3618* 02 35 34.11 +57 09 17.2 7.9 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 457812216335433344,2461188.8618,7.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457812216335433344 20260528.3618 7.92CV 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 05 28.3618 2461188.8618 7.89 02:37:55.13 +57:39:02.3
136.81569 -2.32219 galactic Cas Second-epoch detections are separated by 1.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.4658+57.6504 | 02:37:55.25 +57:39:01.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.884+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:55.13 +57:39:02.3: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:55.13 +57:39:02.3: 10.45 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.45 +/- 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 05 28.3618* 02 37 55.13 +57 39 02.3 7.9 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 J039.4658+57.6504,2461188.8618,7.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.4658+57.6504 20260528.3618 7.89CV 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 05 28.3618 2461188.8618 7.98 02:27:07.81 +56:33:54.6
135.87277 -3.88310 galactic Per Second-epoch detections are separated by 1.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457618423109114880 | 02:27:07.78 +56:33:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.740+/-0.025 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:07.81 +56:33:54.6: 12.96 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:07.81 +56:33:54.6: 10.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.73 +/- 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 05 28.3618* 02 27 07.81 +56 33 54.6 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457618423109114880,2461188.8618,7.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457618423109114880 20260528.3618 7.98CV 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 05 28.3618 2461188.8618 8.01 02:38:46.94 +57:49:57.0
136.84843 -2.10941 galactic Cas Second-epoch detections are separated by 1.9" 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 | Gaia DR3 457946459832991616 | 02:38:46.61 +57:49:58.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1978A&AS...32...25R BD+57 603
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:46.94 +57:49:57.0: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:46.94 +57:49:57.0: 10.34 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.34 +/- 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 05 28.3618* 02 38 46.94 +57 49 57.0 8.0 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 457946459832991616,2461188.8618,8.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457946459832991616 20260528.3618 8.01CV 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 05 28.3618 2461188.8618 8.14 02:25:28.20 +56:11:20.2
135.79307 -4.31673 galactic Per Second-epoch detections are separated by 3.2" 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 | ATO J036.3836+56.1834 | 02:25:28.14 +56:11:20.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +55 6 J-Ks=-0.048+/-0.031 (B)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:28.20 +56:11:20.2: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:28.20 +56:11:20.2: 10.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.40 +/- 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 05 28.3618* 02 25 28.20 +56 11 20.2 8.1 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
ATO J036.3836+56.1834,2461188.8618,8.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J036.3836+56.1834 20260528.3618 8.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 7.96 02:34:04.70 +56:30:40.2
136.78314 -3.57500 galactic Per 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 | Gaia DR3 457755763285796480 | 02:34:03.88 +56:30:45.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:04.70 +56:30:40.2: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:04.70 +56:30:40.2: 10.32 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.32 +/- 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 05 28.3618* 02 34 04.70 +56 30 40.2 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457755763285796480,2461188.8618,7.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457755763285796480 20260528.3618 7.96CV 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 05 28.3618 2461188.8618 8.17 02:25:34.10 +56:34:22.3
135.66875 -3.95313 galactic Per 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 | ATO J036.4026+56.5763 | 02:25:33.82 +56:34:22.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.196+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:34.10 +56:34:22.3: 12.03 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:34.10 +56:34:22.3: 10.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.59 +/- 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 05 28.3618* 02 25 34.10 +56 34 22.3 8.2 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 J036.4026+56.5763,2461188.8618,8.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J036.4026+56.5763 20260528.3618 8.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.04 02:32:45.29 +57:08:07.3
136.37574 -3.06807 galactic Per Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.1901+57.1255 | 02:32:45.21 +57:08:08.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.302+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:45.29 +57:08:07.3: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:45.29 +57:08:07.3: 10.51 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.51 +/- 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 05 28.3618* 02 32 45.29 +57 08 07.3 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.1901+57.1255,2461188.8618,8.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.1901+57.1255 20260528.3618 8.04CV 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 05 28.3618 2461188.8618 8.07 02:31:38.17 +56:33:35.0
136.45279 -3.65869 galactic Per Second-epoch detections are separated by 1.0" and 7.3 pix
The object was found in VSX14" Gaia DR3 457583792795921664
Type: ROT
# Max. Min./Amp. JD0 Period
15.730 G 15.790 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:38.17 +56:33:35.0: 12.70 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:38.17 +56:33:35.0: 10.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.70 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 31 38.17 +56 33 35.0 8.1 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 457583792795921664,2461188.8618,8.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457583792795921664 20260528.3618 8.07CV 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 05 28.3618 2461188.8618 8.04 02:32:05.15 +56:49:22.4
136.41029 -3.39173 galactic Per Second-epoch detections are separated by 3.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457963193027127424 | 02:32:04.79 +56:49:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:05.15 +56:49:22.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:05.15 +56:49:22.4: 10.34 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.34 +/- 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 05 28.3618* 02 32 05.15 +56 49 22.4 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457963193027127424,2461188.8618,8.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457963193027127424 20260528.3618 8.04CV 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 05 28.3618 2461188.8618 8.07 02:22:10.11 +56:24:22.8
135.28655 -4.27344 galactic Per Second-epoch detections are separated by 2.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458278477988992384 | 02:22:10.19 +56:24:23.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.108+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:10.11 +56:24:22.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:10.11 +56:24:22.8: 10.46 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.46 +/- 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 05 28.3618* 02 22 10.11 +56 24 22.8 8.1 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 458278477988992384,2461188.8618,8.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458278477988992384 20260528.3618 8.07CV 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 05 28.3618 2461188.8618 8.10 02:30:51.88 +57:04:10.0
136.16272 -3.22611 galactic Per Second-epoch detections are separated by 0.6" 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 | ATO J037.7008+57.0647 | 02:30:51.84 +57:04:10.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.142+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:51.88 +57:04:10.0: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:51.88 +57:04:10.0: 10.55 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.55 +/- 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 05 28.3618* 02 30 51.88 +57 04 10.0 8.1 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
ATO J037.7008+57.0647,2461188.8618,8.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.7008+57.0647 20260528.3618 8.10CV 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 05 28.3618 2461188.8618 8.14 02:25:20.49 +56:12:13.5
135.77104 -4.30925 galactic Per Second-epoch detections are separated by 2.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457513149174786176 | 02:25:20.28 +56:12:13.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +55 5 J-Ks=-0.059+/-0.034 (B)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:20.49 +56:12:13.5: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:20.49 +56:12:13.5: 10.45 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.45 +/- 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 05 28.3618* 02 25 20.49 +56 12 13.5 8.1 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 457513149174786176,2461188.8618,8.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457513149174786176 20260528.3618 8.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.12 02:19:52.90 +56:15:39.2
135.03724 -4.51800 galactic Per Second-epoch detections are separated by 1.8" 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 | Gaia DR3 458262328911050880 | 02:19:52.94 +56:15:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.175+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:52.90 +56:15:39.2: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:52.90 +56:15:39.2: 10.44 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.44 +/- 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 05 28.3618* 02 19 52.90 +56 15 39.2 8.1 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 458262328911050880,2461188.8618,8.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458262328911050880 20260528.3618 8.12CV 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 05 28.3618 2461188.8618 8.11 02:33:49.42 +57:35:11.7
136.33595 -2.59606 galactic Per Second-epoch detections are separated by 1.3" and 7.2 pix
The object was found in VSX19" ZTF J023348.90+573530.8
Type: BY
# Max. Min./Amp. JD0 Period
19.921 r Y 0.213 r 2458379.92900 0.792993600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:49.42 +57:35:11.7: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:49.42 +57:35:11.7: 10.53 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.53 +/- 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 05 28.3618* 02 33 49.42 +57 35 11.7 8.1 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
ZTF J023348.90+573530.8,2461188.8618,8.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J023348.90+573530.8 20260528.3618 8.11CV 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 05 28.3618 2461188.8618 8.11 02:33:29.99 +57:42:17.0
136.25047 -2.50364 galactic Per Second-epoch detections are separated by 0.6" and 7.1 pix
The object was found in VSX 2" Gaia DR3 458028957566623360
Type: ROT
# Max. Min./Amp. JD0 Period
10.440 G 10.470 G 10.914500000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:29.99 +57:42:17.0: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:29.99 +57:42:17.0: 10.67 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.67 +/- 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 05 28.3618* 02 33 29.99 +57 42 17.0 8.1 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 458028957566623360,2461188.8618,8.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458028957566623360 20260528.3618 8.11CV 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 05 28.3618 2461188.8618 8.16 02:31:38.51 +57:13:48.2
136.20004 -3.03765 galactic Per Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457989856183731328 | 02:31:38.47 +57:13:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.311+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:38.51 +57:13:48.2: 9.37 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:38.51 +57:13:48.2: 10.66 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.55 +/- 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 05 28.3618* 02 31 38.51 +57 13 48.2 8.2 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 457989856183731328,2461188.8618,8.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457989856183731328 20260528.3618 8.16CV 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 05 28.3618 2461188.8618 8.00 02:33:48.99 +57:01:45.0
136.54991 -3.11089 galactic Per Second-epoch detections are separated by 2.1" 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 | ATO J038.4387+57.0274 | 02:33:48.47 +57:01:46.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:48.99 +57:01:45.0: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:48.99 +57:01:45.0: 10.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.43 +/- 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 05 28.3618* 02 33 48.99 +57 01 45.0 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4387+57.0274,2461188.8618,8.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.4387+57.0274 20260528.3618 8.00CV 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 05 28.3618 2461188.8618 8.24 02:24:06.55 +56:30:01.1
135.50586 -4.09213 galactic Per Second-epoch detections are separated by 2.0" 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 J036.0447+56.4918 | 02:24:06.53 +56:29:59.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.852+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:06.55 +56:30:01.1: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:06.55 +56:30:01.1: 10.93 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.93 +/- 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 05 28.3618* 02 24 06.55 +56 30 01.1 8.2 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 J036.0447+56.4918,2461188.8618,8.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J036.0447+56.4918 20260528.3618 8.24CV 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 05 28.3618 2461188.8618 8.16 02:36:56.79 +57:06:43.6
136.90961 -2.86843 galactic Per 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 | ATO J039.2495+57.1096 | 02:36:56.78 +57:06:43.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.727+/-0.042 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:56.79 +57:06:43.6: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:56.79 +57:06:43.6: 10.80 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.80 +/- 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 05 28.3618* 02 36 56.79 +57 06 43.6 8.2 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 J039.2495+57.1096,2461188.8618,8.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.2495+57.1096 20260528.3618 8.16CV 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 05 28.3618 2461188.8618 8.21 02:31:18.98 +55:53:51.0
136.66190 -4.28876 galactic Per Second-epoch detections are separated by 6.8" 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 J037.8193+55.8908 | 02:31:18.96 +55:53:50.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.878+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:18.98 +55:53:51.0: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:18.98 +55:53:51.0: 10.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.76 +/- 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 05 28.3618* 02 31 18.98 +55 53 51.0 8.2 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 J037.8193+55.8908,2461188.8618,8.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.8193+55.8908 20260528.3618 8.21CV 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 05 28.3618 2461188.8618 8.21 02:24:09.75 +56:34:02.5
135.48916 -4.02676 galactic Per Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457537063552340736 | 02:24:09.65 +56:34:02.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.079+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:09.75 +56:34:02.5: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:09.75 +56:34:02.5: 10.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.59 +/- 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 05 28.3618* 02 24 09.75 +56 34 02.5 8.2 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 457537063552340736,2461188.8618,8.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457537063552340736 20260528.3618 8.21CV 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 05 28.3618 2461188.8618 8.21 02:37:31.97 +57:28:17.7
136.83958 -2.50705 galactic Per Second-epoch detections are separated by 2.8" 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 | Large-amplitude variable Gaia DR2 457916253319743616 | 02:37:31.82 +57:28:17.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.147+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:31.97 +57:28:17.7: 10.56 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:31.97 +57:28:17.7: 10.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.64 +/- 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 05 28.3618* 02 37 31.97 +57 28 17.7 8.2 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
Large-amplitude variable Gaia DR2 457916253319743616,2461188.8618,8.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457916253319743616 20260528.3618 8.21CV 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 05 28.3618 2461188.8618 9.08 00:52:30.58 +59:43:27.9
123.06720 -3.14705 galactic Cas Second-epoch detections are separated by 2.9" and 8.8 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 426857012646129536 | 00:52:31.09 +59:43:23.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A8: 1935BSD...C01....0S BSD 8- 287
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:30.58 +59:43:27.9: 9.50 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:30.58 +59:43:27.9: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 00 52 30.58 +59 43 27.9 9.1 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 426857012646129536,2461188.8618,9.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426857012646129536 20260528.3618 9.08CV 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 05 28.3618 2461188.8618 8.24 02:30:37.35 +56:23:01.5
136.38908 -3.87437 galactic Per Second-epoch detections are separated by 1.2" and 7.3 pix
The object was found in VSX22" Gaia DR3 457575031062827776
Type: ROT
# Max. Min./Amp. JD0 Period
15.200 G 15.240 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:37.35 +56:23:01.5: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:37.35 +56:23:01.5: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 30 37.35 +56 23 01.5 8.2 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 457575031062827776,2461188.8618,8.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457575031062827776 20260528.3618 8.24CV 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 05 28.3618 2461188.8618 8.22 02:36:19.99 +57:15:26.8
136.77573 -2.76771 galactic Per 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 | Gaia DR3 457907358450596352 | 02:36:19.89 +57:15:28.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1978A&AS...32...25R BD+56 661 J-Ks=0.222+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:19.99 +57:15:26.8: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:19.99 +57:15:26.8: 10.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.54 +/- 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 05 28.3618* 02 36 19.99 +57 15 26.8 8.2 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 457907358450596352,2461188.8618,8.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457907358450596352 20260528.3618 8.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.25 02:35:18.58 +57:31:37.0
136.54300 -2.57381 galactic Per 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 458102246888080768 | 02:35:18.44 +57:31:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:18.58 +57:31:37.0: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:18.58 +57:31:37.0: 10.63 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.63 +/- 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 05 28.3618* 02 35 18.58 +57 31 37.0 8.2 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 458102246888080768,2461188.8618,8.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458102246888080768 20260528.3618 8.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.22 02:32:18.76 +56:21:25.6
136.61638 -3.81080 galactic Per Second-epoch detections are separated by 2.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457388938720751616 | 02:32:18.57 +56:21:26.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.694+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:18.76 +56:21:25.6: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:18.76 +56:21:25.6: 10.82 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.82 +/- 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 05 28.3618* 02 32 18.76 +56 21 25.6 8.2 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 457388938720751616,2461188.8618,8.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457388938720751616 20260528.3618 8.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.31 02:21:59.04 +56:30:02.2
135.23004 -4.19367 galactic Per Second-epoch detections are separated by 0.4" and 7.4 pix
The object was found in VSX 3" TYC 3694-1258-1
Type: SRS
# Max. Min./Amp. JD0 Period
11.810 V 12.020 V 2455719.00000 24.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:59.04 +56:30:02.2: 11.33 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:59.04 +56:30:02.2: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 21 59.04 +56 30 02.2 8.3 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
TYC 3694-1258-1,2461188.8618,8.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TYC 3694-1258-1 20260528.3618 8.31CV 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 05 28.3618 2461188.8618 8.45 02:22:31.60 +56:14:10.7
135.39209 -4.41591 galactic Per Second-epoch detections are separated by 0.9" and 7.5 pix
The object was found in VSX15" Gaia DR3 457502291496530304
Type: ROT
# Max. Min./Amp. JD0 Period
16.090 G 16.130 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:31.60 +56:14:10.7: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:31.60 +56:14:10.7: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.87 +/- 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 05 28.3618* 02 22 31.60 +56 14 10.7 8.4 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 457502291496530304,2461188.8618,8.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457502291496530304 20260528.3618 8.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.33 02:30:30.72 +57:30:28.2
135.95428 -2.83736 galactic Per Second-epoch detections are separated by 1.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458046515393935744 | 02:30:30.94 +57:30:26.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:30.72 +57:30:28.2: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:30.72 +57:30:28.2: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 30 30.72 +57 30 28.2 8.3 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 458046515393935744,2461188.8618,8.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458046515393935744 20260528.3618 8.33CV 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 05 28.3618 2461188.8618 8.44 02:36:08.67 +57:39:33.5
136.59415 -2.40822 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 | ATO J039.0481+57.6598 | 02:36:08.50 +57:39:34.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.314+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:08.67 +57:39:33.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:08.67 +57:39:33.5: 10.90 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.90 +/- 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 05 28.3618* 02 36 08.67 +57 39 33.5 8.4 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 J039.0481+57.6598,2461188.8618,8.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.0481+57.6598 20260528.3618 8.44CV 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 05 28.3618 2461188.8618 8.30 02:22:04.64 +57:10:39.2
135.00900 -3.55353 galactic Per Second-epoch detections are separated by 0.8" and 7.2 pix
The object was found in VSX 1" NSV 800
Type: GCAS:
# Max. Min./Amp. JD0 Period
10.380 V Y 0.040 V B2Vn(e)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:04.64 +57:10:39.2: 11.39 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:04.64 +57:10:39.2: 10.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 22 04.64 +57 10 39.2 8.3 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
NSV 800,2461188.8618,8.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 800 20260528.3618 8.30CV 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 05 28.3618 2461188.8618 8.29 02:33:05.67 +56:13:01.3
136.77044 -3.89891 galactic Per Second-epoch detections are separated by 7.5" 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 | Gaia DR3 457372446046599424 | 02:33:05.74 +56:12:59.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=1.319+/-0.039 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:05.67 +56:13:01.3: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:05.67 +56:13:01.3: 11.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 33 05.67 +56 13 01.3 8.3 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 457372446046599424,2461188.8618,8.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457372446046599424 20260528.3618 8.29CV 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 05 28.3618 2461188.8618 8.48 02:27:33.00 +56:13:09.5
136.05275 -4.18437 galactic Per Second-epoch detections are separated by 2.5" 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 | Gaia DR3 457557060918681856 | 02:27:33.13 +56:13:10.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.062+/-0.026 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:33.00 +56:13:09.5: 11.21 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:33.00 +56:13:09.5: 10.65 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.65 +/- 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 05 28.3618* 02 27 33.00 +56 13 09.5 8.5 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 457557060918681856,2461188.8618,8.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457557060918681856 20260528.3618 8.48CV 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 05 28.3618 2461188.8618 8.35 02:31:59.20 +56:42:22.0
136.44203 -3.50494 galactic Per 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 | ATO J038.0032+56.7143 | 02:31:58.77 +56:42:23.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:59.20 +56:42:22.0: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:59.20 +56:42:22.0: 10.63 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.63 +/- 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 05 28.3618* 02 31 59.20 +56 42 22.0 8.3 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 J038.0032+56.7143,2461188.8618,8.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.0032+56.7143 20260528.3618 8.35CV 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 05 28.3618 2461188.8618 8.40 02:26:07.28 +56:25:11.5
135.79499 -4.06878 galactic Per Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457610077996536576 | 02:26:07.34 +56:25:12.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.169+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:07.28 +56:25:11.5: 11.91 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:07.28 +56:25:11.5: 10.82 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.82 +/- 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 05 28.3618* 02 26 07.28 +56 25 11.5 8.4 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 457610077996536576,2461188.8618,8.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457610077996536576 20260528.3618 8.40CV 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 05 28.3618 2461188.8618 8.39 02:36:35.17 +57:36:34.3
136.66815 -2.43071 galactic Cas Second-epoch detections are separated by 4.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457921720823408384 | 02:36:35.02 +57:36:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9pSi? 1971AN....293..163Z BD+56 664
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:35.17 +57:36:34.3: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:35.17 +57:36:34.3: 10.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.69 +/- 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 05 28.3618* 02 36 35.17 +57 36 34.3 8.4 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 457921720823408384,2461188.8618,8.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457921720823408384 20260528.3618 8.39CV 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 05 28.3618 2461188.8618 8.42 02:35:20.47 +57:29:29.4
136.56074 -2.60480 galactic Per Second-epoch detections are separated by 2.3" 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 | ATO J038.8552+57.4916 | 02:35:20.17 +57:29:30.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:20.47 +57:29:29.4: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:20.47 +57:29:29.4: 10.85 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.85 +/- 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 05 28.3618* 02 35 20.47 +57 29 29.4 8.4 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
ATO J038.8552+57.4916,2461188.8618,8.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.8552+57.4916 20260528.3618 8.42CV 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 05 28.3618 2461188.8618 8.46 02:37:41.05 +57:33:20.1
136.82477 -2.42190 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 | ATO J039.4083+57.5560 | 02:37:41.21 +57:33:21.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.780+/-0.045 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:41.05 +57:33:20.1: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:41.05 +57:33:20.1: 11.05 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.05 +/- 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 05 28.3618* 02 37 41.05 +57 33 20.1 8.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.4083+57.5560,2461188.8618,8.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.4083+57.5560 20260528.3618 8.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.46 02:30:49.77 +56:11:02.6
136.49075 -4.04877 galactic Per 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 457383716040658304 | 02:30:49.82 +56:11:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.698+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:49.77 +56:11:02.6: 13.02 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:49.77 +56:11:02.6: 11.00 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.00 +/- 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 05 28.3618* 02 30 49.77 +56 11 02.6 8.5 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 457383716040658304,2461188.8618,8.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457383716040658304 20260528.3618 8.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.13 00:57:05.28 +57:30:11.8
123.69407 -5.36011 galactic Cas Second-epoch detections are separated by 0.8" and 8.5 pix
The object was found in VSX 0" Gaia DR3 424324390688629760
Type: L
# Max. Min./Amp. JD0 Period
11.460 G 11.720 G M
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:57:05.28 +57:30:11.8: 10.86 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:57:05.28 +57:30:11.8: 12.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 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 05 28.3618* 00 57 05.28 +57 30 11.8 9.1 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 424324390688629760,2461188.8618,9.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424324390688629760 20260528.3618 9.13CV 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 05 28.3618 2461188.8618 8.45 02:30:33.01 +56:53:08.7
136.19177 -3.41249 galactic Per 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 457978483110691456 | 02:30:32.95 +56:53:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.097+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:33.01 +56:53:08.7: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:33.01 +56:53:08.7: 10.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.78 +/- 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 05 28.3618* 02 30 33.01 +56 53 08.7 8.4 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 457978483110691456,2461188.8618,8.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457978483110691456 20260528.3618 8.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.49 02:19:44.52 +56:42:25.7
134.86880 -4.10412 galactic Per Second-epoch detections are separated by 4.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458348022100955904 | 02:19:41.27 +56:42:58.5 (Gaia DR3) | BCEP (local) | B (local) | Gaia3var=VARIABLE SpType: OB- 1965LS....C05....0H LS V +56 25
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:44.52 +56:42:25.7: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:44.52 +56:42:25.7: 10.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.97 +/- 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 05 28.3618* 02 19 44.52 +56 42 25.7 8.5 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 458348022100955904,2461188.8618,8.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458348022100955904 20260528.3618 8.49CV 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 05 28.3618 2461188.8618 8.46 02:21:04.81 +56:15:32.5
135.19497 -4.46347 galactic Per Second-epoch detections are separated by 2.4" and 7.2 pix
The object was found in VSX13" Gaia DR3 458255319524584576
Type: ROT
# Max. Min./Amp. JD0 Period
15.290 G 15.310 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:04.81 +56:15:32.5: 12.43 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:04.81 +56:15:32.5: 11.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.06 +/- 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 05 28.3618* 02 21 04.81 +56 15 32.5 8.5 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 458255319524584576,2461188.8618,8.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458255319524584576 20260528.3618 8.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.46 02:26:13.37 +56:36:45.1
135.73888 -3.88389 galactic Per Second-epoch detections are separated by 2.5" 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 | Gaia DR3 457622310064448128 | 02:26:13.35 +56:36:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:13.37 +56:36:45.1: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:13.37 +56:36:45.1: 10.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.78 +/- 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 05 28.3618* 02 26 13.37 +56 36 45.1 8.5 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 457622310064448128,2461188.8618,8.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457622310064448128 20260528.3618 8.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.55 02:29:33.40 +55:57:20.3
136.41086 -4.32693 galactic Per 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 | Gaia DR3 457351177367649536 | 02:29:33.62 +55:57:17.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:33.40 +55:57:20.3: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:33.40 +55:57:20.3: 11.05 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.05 +/- 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 05 28.3618* 02 29 33.40 +55 57 20.3 8.6 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 457351177367649536,2461188.8618,8.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457351177367649536 20260528.3618 8.55CV 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 05 28.3618 2461188.8618 8.56 02:36:22.57 +57:40:03.4
136.61938 -2.38840 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 | Gaia DR3 458109771665185536 | 02:36:22.54 +57:40:06.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:22.57 +57:40:03.4: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:22.57 +57:40:03.4: 11.05 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.05 +/- 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 05 28.3618* 02 36 22.57 +57 40 03.4 8.6 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 458109771665185536,2461188.8618,8.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458109771665185536 20260528.3618 8.56CV 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 05 28.3618 2461188.8618 8.57 02:33:09.48 +57:00:39.2
136.47407 -3.16217 galactic Per 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 | ATO J038.2979+57.0026 | 02:33:09.28 +57:00:39.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.196+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:09.48 +57:00:39.2: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:09.48 +57:00:39.2: 10.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.97 +/- 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 05 28.3618* 02 33 09.48 +57 00 39.2 8.6 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 J038.2979+57.0026,2461188.8618,8.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.2979+57.0026 20260528.3618 8.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.48 02:29:50.72 +56:19:10.9
136.31288 -3.97393 galactic Per Second-epoch detections are separated by 7.2" and 8.0 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 J037.4614+56.3323 | 02:29:50.90 +56:19:10.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.096+/-0.036 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:50.72 +56:19:10.9: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:50.72 +56:19:10.9: 11.00 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.00 +/- 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 05 28.3618* 02 29 50.72 +56 19 10.9 8.5 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 J037.4614+56.3323,2461188.8618,8.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.4614+56.3323 20260528.3618 8.48CV 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 05 28.3618 2461188.8618 8.42 02:29:41.24 +56:20:06.8
136.28672 -3.96764 galactic Per Second-epoch detections are separated by 3.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457550704367181056 | 02:29:41.31 +56:20:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:41.24 +56:20:06.8: 10.43 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:41.24 +56:20:06.8: 11.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 29 41.24 +56 20 06.8 8.4 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 457550704367181056,2461188.8618,8.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457550704367181056 20260528.3618 8.42CV 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 05 28.3618 2461188.8618 8.54 02:28:09.92 +56:10:50.3
136.14678 -4.18919 galactic Per Second-epoch detections are separated by 3.0" 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 457545687845511808 | 02:28:09.79 +56:10:50.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.085+/-0.029 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:09.92 +56:10:50.3: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:09.92 +56:10:50.3: 10.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.95 +/- 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 05 28.3618* 02 28 09.92 +56 10 50.3 8.5 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 457545687845511808,2461188.8618,8.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457545687845511808 20260528.3618 8.54CV 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 05 28.3618 2461188.8618 8.51 02:34:26.97 +56:29:12.2
136.83994 -3.57773 galactic Per Second-epoch detections are separated by 1.6" 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 | Gaia DR3 457752877067783040 | 02:34:26.47 +56:29:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:26.97 +56:29:12.2: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:26.97 +56:29:12.2: 11.14 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.14 +/- 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 05 28.3618* 02 34 26.97 +56 29 12.2 8.5 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 457752877067783040,2461188.8618,8.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457752877067783040 20260528.3618 8.51CV 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 05 28.3618 2461188.8618 8.53 02:31:06.05 +56:37:19.1
136.36090 -3.62878 galactic Per Second-epoch detections are separated by 3.4" 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 457585132825664640 | 02:31:06.16 +56:37:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.101+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:06.05 +56:37:19.1: 12.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:06.05 +56:37:19.1: 10.89 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.89 +/- 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 05 28.3618* 02 31 06.05 +56 37 19.1 8.5 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 457585132825664640,2461188.8618,8.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457585132825664640 20260528.3618 8.53CV 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 05 28.3618 2461188.8618 8.74 02:40:07.39 +58:29:00.9
136.74691 -1.44241 galactic Cas Second-epoch detections are separated by 1.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 464162102144148736 | 02:40:07.63 +58:28:57.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:40:07.39 +58:29:00.9: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:40:07.39 +58:29:00.9: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 40 07.39 +58 29 00.9 8.7 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 464162102144148736,2461188.8618,8.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 464162102144148736 20260528.3618 8.74CV 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 05 28.3618 2461188.8618 8.65 02:35:08.80 +57:36:14.7
136.49275 -2.51129 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 458105717221633536 | 02:35:08.75 +57:36:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.847+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:08.80 +57:36:14.7: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:08.80 +57:36:14.7: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 35 08.80 +57 36 14.7 8.7 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 458105717221633536,2461188.8618,8.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458105717221633536 20260528.3618 8.65CV 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 05 28.3618 2461188.8618 8.45 02:34:05.16 +56:42:26.1
136.70827 -3.39372 galactic Per Second-epoch detections are separated by 2.1" and 6.8 pix
The object was found in VSX16" Gaia DR3 457775687633336704
Type: RS
# Max. Min./Amp. JD0 Period
17.400 G 17.580 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:05.16 +56:42:26.1: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:05.16 +56:42:26.1: 11.20 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.20 +/- 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 05 28.3618* 02 34 05.16 +56 42 26.1 8.4 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 457775687633336704,2461188.8618,8.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457775687633336704 20260528.3618 8.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.57 02:32:26.23 +56:47:10.1
136.46884 -3.40747 galactic Per Second-epoch detections are separated by 2.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.1078+56.7931 | 02:32:26.17 +56:47:10.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.926+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:26.23 +56:47:10.1: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:26.23 +56:47:10.1: 11.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 32 26.23 +56 47 10.1 8.6 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 J038.1078+56.7931,2461188.8618,8.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.1078+56.7931 20260528.3618 8.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.63 02:33:13.67 +57:44:32.4
136.20247 -2.48282 galactic Per Second-epoch detections are separated by 4.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458029850919815680 | 02:33:13.70 +57:44:32.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.278+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:13.67 +57:44:32.4: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:13.67 +57:44:32.4: 11.01 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.01 +/- 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 05 28.3618* 02 33 13.67 +57 44 32.4 8.6 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 458029850919815680,2461188.8618,8.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458029850919815680 20260528.3618 8.63CV 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 05 28.3618 2461188.8618 8.64 02:30:52.97 +56:54:21.1
136.22643 -3.37684 galactic Per Second-epoch detections are separated by 4.5" and 7.9 pix
The object was found in VSX 1" Gaia DR3 457978208232758784
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.940 G 10.990 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:52.97 +56:54:21.1: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:52.97 +56:54:21.1: 11.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 30 52.97 +56 54 21.1 8.6 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 457978208232758784,2461188.8618,8.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457978208232758784 20260528.3618 8.64CV 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 05 28.3618 2461188.8618 8.59 02:29:40.98 +56:18:42.4
136.29488 -3.98964 galactic Per Second-epoch detections are separated by 4.9" and 8.0 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 457550601287980160 | 02:29:40.90 +56:18:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: em 1950ApJ...112...72M BD+55 633 J-Ks=0.176+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:40.98 +56:18:42.4: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:40.98 +56:18:42.4: 10.88 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.88 +/- 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 05 28.3618* 02 29 40.98 +56 18 42.4 8.6 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 457550601287980160,2461188.8618,8.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457550601287980160 20260528.3618 8.59CV 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 05 28.3618 2461188.8618 8.62 02:35:43.04 +56:44:19.4
136.90251 -3.27769 galactic Per Second-epoch detections are separated by 1.8" and 6.8 pix
The object was found in VSX 2" Gaia DR3 457785175221622144
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.720 G 10.770 G 5.916700000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:43.04 +56:44:19.4: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:43.04 +56:44:19.4: 10.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.97 +/- 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 05 28.3618* 02 35 43.04 +56 44 19.4 8.6 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 457785175221622144,2461188.8618,8.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457785175221622144 20260528.3618 8.62CV 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 05 28.3618 2461188.8618 8.70 02:32:59.22 +57:28:35.8
136.27435 -2.74068 galactic Per 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 | Gaia DR3 458022738454361216 | 02:32:59.16 +57:28:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1965LS....C05....0H LS V +57 45 J-Ks=0.121+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:59.22 +57:28:35.8: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:59.22 +57:28:35.8: 11.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 32 59.22 +57 28 35.8 8.7 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 458022738454361216,2461188.8618,8.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458022738454361216 20260528.3618 8.70CV 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 05 28.3618 2461188.8618 8.79 02:28:41.20 +56:12:06.5
136.20666 -4.14291 galactic Per Second-epoch detections are separated by 2.1" and 7.5 pix
The object was found in VSX 7" ASASSN-V J022841.63+561200.9
Type: L
# Max. Min./Amp. JD0 Period
12.590 V 12.860 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:41.20 +56:12:06.5: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:41.20 +56:12:06.5: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 28 41.20 +56 12 06.5 8.8 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 J022841.63+561200.9,2461188.8618,8.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022841.63+561200.9 20260528.3618 8.79CV 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 05 28.3618 2461188.8618 8.70 02:18:24.04 +56:23:24.4
134.79988 -4.46460 galactic Per Second-epoch detections are separated by 4.1" 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 458313421843558528 | 02:18:24.08 +56:23:24.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.115+/-0.035 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:24.04 +56:23:24.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:24.04 +56:23:24.4: 11.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 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 05 28.3618* 02 18 24.04 +56 23 24.4 8.7 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 458313421843558528,2461188.8618,8.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458313421843558528 20260528.3618 8.70CV 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 05 28.3618 2461188.8618 8.82 02:29:57.20 +56:36:49.0
136.21732 -3.69552 galactic Per Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457581490693447040 | 02:29:57.38 +56:36:48.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.969+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:57.20 +56:36:49.0: 10.81 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:57.20 +56:36:49.0: 11.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 29 57.20 +56 36 49.0 8.8 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 457581490693447040,2461188.8618,8.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457581490693447040 20260528.3618 8.82CV 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 05 28.3618 2461188.8618 8.69 02:29:58.23 +56:08:53.2
136.39300 -4.12676 galactic Per Second-epoch detections are separated by 2.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457359423705242368 | 02:29:58.63 +56:08:48.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:58.23 +56:08:53.2: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:58.23 +56:08:53.2: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 29 58.23 +56 08 53.2 8.7 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 457359423705242368,2461188.8618,8.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457359423705242368 20260528.3618 8.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.70 02:35:04.79 +57:26:52.8
136.54532 -2.65855 galactic Per Second-epoch detections are separated by 1.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458007791968161280 | 02:35:04.80 +57:26:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.761+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:04.79 +57:26:52.8: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:04.79 +57:26:52.8: 11.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 35 04.79 +57 26 52.8 8.7 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 458007791968161280,2461188.8618,8.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458007791968161280 20260528.3618 8.70CV 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 05 28.3618 2461188.8618 8.78 02:19:36.25 +56:23:22.4
134.95759 -4.40970 galactic Per Second-epoch detections are separated by 3.4" and 7.1 pix
The object was found in VSX 4" Gaia DR3 458272396314337536
Type: S
# Max. Min./Amp. JD0 Period
15.810 G 16.200 G M
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:36.25 +56:23:22.4: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:36.25 +56:23:22.4: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 19 36.25 +56 23 22.4 8.8 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 458272396314337536,2461188.8618,8.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458272396314337536 20260528.3618 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 05 28.3618 2461188.8618 8.66 02:31:28.99 +57:11:53.7
136.19213 -3.07521 galactic Per Second-epoch detections are separated by 4.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457988344355269888 | 02:31:29.21 +57:11:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:28.99 +57:11:53.7: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:28.99 +57:11:53.7: 11.19 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.19 +/- 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 05 28.3618* 02 31 28.99 +57 11 53.7 8.7 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 457988344355269888,2461188.8618,8.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457988344355269888 20260528.3618 8.66CV 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 05 28.3618 2461188.8618 8.79 02:37:50.62 +57:45:48.2
136.76146 -2.22281 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 | ATO J039.4571+57.7717 | 02:37:50.58 +57:45:50.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +57 75 J-Ks=0.138+/-0.026 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:50.62 +57:45:48.2: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:50.62 +57:45:48.2: 11.10 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.10 +/- 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 05 28.3618* 02 37 50.62 +57 45 48.2 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
ATO J039.4571+57.7717,2461188.8618,8.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.4571+57.7717 20260528.3618 8.79CV 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 05 28.3618 2461188.8618 8.70 02:29:28.85 +56:33:09.5
136.17943 -3.77626 galactic Per Second-epoch detections are separated by 2.0" and 7.0 pix
The object was found in VSX 3" Gaia DR3 457591145780012800
Type: BCEP
# Max. Min./Amp. JD0 Period
10.740 G 10.780 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:28.85 +56:33:09.5: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:28.85 +56:33:09.5: 10.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.99 +/- 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 05 28.3618* 02 29 28.85 +56 33 09.5 8.7 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 457591145780012800,2461188.8618,8.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457591145780012800 20260528.3618 8.70CV 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 05 28.3618 2461188.8618 8.71 02:29:39.44 +56:11:35.3
136.33566 -4.10114 galactic Per Second-epoch detections are separated by 1.2" and 7.5 pix
The object was found in VSX 6" NSV 15519
Type: SR
# Max. Min./Amp. JD0 Period
12.400 V 13.100 V 2458443.36190 299.178129200000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:39.44 +56:11:35.3: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:39.44 +56:11:35.3: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 29 39.44 +56 11 35.3 8.7 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
NSV 15519,2461188.8618,8.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 15519 20260528.3618 8.71CV 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 05 28.3618 2461188.8618 8.86 02:26:43.32 +56:24:14.7
135.87840 -4.05366 galactic Per Second-epoch detections are separated by 5.6" 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 | ATO J036.6811+56.4136 | 02:26:43.21 +56:24:13.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.233+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:43.32 +56:24:14.7: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:43.32 +56:24:14.7: 11.14 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.14 +/- 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 05 28.3618* 02 26 43.32 +56 24 14.7 8.9 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 J036.6811+56.4136,2461188.8618,8.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J036.6811+56.4136 20260528.3618 8.86CV 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 05 28.3618 2461188.8618 8.63 02:29:59.81 +56:13:02.8
136.37056 -4.06104 galactic Per Second-epoch detections are separated by 3.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457548814581644416 | 02:30:00.12 +56:12:59.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:59.81 +56:13:02.8: 11.73 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:59.81 +56:13:02.8: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 29 59.81 +56 13 02.8 8.6 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 457548814581644416,2461188.8618,8.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457548814581644416 20260528.3618 8.63CV 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 05 28.3618 2461188.8618 8.84 02:21:34.70 +56:26:46.5
135.19596 -4.26394 galactic Per Second-epoch detections are separated by 7.9" 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 | ATO J035.4115+56.4466 | 02:21:34.45 +56:26:43.9 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:34.70 +56:26:46.5: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:34.70 +56:26:46.5: 11.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 21 34.70 +56 26 46.5 8.8 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 J035.4115+56.4466,2461188.8618,8.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J035.4115+56.4466 20260528.3618 8.84CV 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 05 28.3618 2461188.8618 8.70 02:31:09.60 +57:16:15.9
136.12412 -3.02418 galactic Per Second-epoch detections are separated by 3.6" 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 457993944995787520 | 02:31:09.65 +57:16:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +57 41 J-Ks=0.133+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:09.60 +57:16:15.9: 12.50 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:09.60 +57:16:15.9: 11.15 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.15 +/- 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 05 28.3618* 02 31 09.60 +57 16 15.9 8.7 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 457993944995787520,2461188.8618,8.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457993944995787520 20260528.3618 8.70CV 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 05 28.3618 2461188.8618 8.79 02:26:55.68 +56:30:21.4
135.86818 -3.94839 galactic Per 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 | Gaia DR3 457617843297470592 | 02:26:55.70 +56:30:20.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.099+/-0.028 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:55.68 +56:30:21.4: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:55.68 +56:30:21.4: 11.08 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.08 +/- 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 05 28.3618* 02 26 55.68 +56 30 21.4 8.8 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 457617843297470592,2461188.8618,8.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457617843297470592 20260528.3618 8.79CV 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 05 28.3618 2461188.8618 8.65 02:35:30.33 +57:03:27.8
136.75083 -2.99545 galactic Per Second-epoch detections are separated by 0.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.8893+57.0658 | 02:35:30.27 +57:03:32.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.411+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:30.33 +57:03:27.8: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:30.33 +57:03:27.8: 11.05 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.05 +/- 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 05 28.3618* 02 35 30.33 +57 03 27.8 8.7 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 J038.8893+57.0658,2461188.8618,8.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.8893+57.0658 20260528.3618 8.65CV 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 05 28.3618 2461188.8618 8.73 02:28:49.65 +56:07:39.2
136.25231 -4.20476 galactic Per Second-epoch detections are separated by 4.8" and 6.9 pix
The object was found in VSX 3" Gaia DR3 457541805195095296
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.960 G 11.030 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:49.65 +56:07:39.2: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:49.65 +56:07:39.2: 11.12 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.12 +/- 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 05 28.3618* 02 28 49.65 +56 07 39.2 8.7 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 457541805195095296,2461188.8618,8.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457541805195095296 20260528.3618 8.73CV 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 05 28.3618 2461188.8618 8.73 02:26:10.82 +56:48:29.2
135.66318 -3.70339 galactic Per Second-epoch detections are separated by 1.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.5437+56.8208 | 02:26:10.73 +56:48:29.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.384+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:10.82 +56:48:29.2: 10.66 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:10.82 +56:48:29.2: 11.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.08 +/- 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 05 28.3618* 02 26 10.82 +56 48 29.2 8.7 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 J036.5437+56.8208,2461188.8618,8.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J036.5437+56.8208 20260528.3618 8.73CV 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 05 28.3618 2461188.8618 8.72 02:32:17.90 +57:17:10.0
136.26107 -2.95217 galactic Per Second-epoch detections are separated by 1.7" and 7.3 pix
The object was found in VSX 1" Gaia DR3 458013701843090176
Type: E
# Max. Min./Amp. JD0 Period
10.980 G 11.070 G 3.240760000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:17.90 +57:17:10.0: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:17.90 +57:17:10.0: 11.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.24 +/- 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 05 28.3618* 02 32 17.90 +57 17 10.0 8.7 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 458013701843090176,2461188.8618,8.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458013701843090176 20260528.3618 8.72CV 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 05 28.3618 2461188.8618 8.87 02:34:24.43 +57:28:27.5
136.45165 -2.66942 galactic Per Second-epoch detections are separated by 4.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5831+57.4740 | 02:34:24.42 +57:28:26.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.152+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:24.43 +57:28:27.5: 9.91 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:24.43 +57:28:27.5: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 34 24.43 +57 28 27.5 8.9 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 J038.5831+57.4740,2461188.8618,8.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.5831+57.4740 20260528.3618 8.87CV 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 05 28.3618 2461188.8618 8.89 02:31:51.85 +56:45:48.0
136.40475 -3.45834 galactic Per Second-epoch detections are separated by 1.0" and 6.9 pix
The object was found in VSX 1" NSV 15534
Type: LB:
# Max. Min./Amp. JD0 Period
12.900 V 13.200 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:51.85 +56:45:48.0: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:51.85 +56:45:48.0: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 31 51.85 +56 45 48.0 8.9 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
NSV 15534,2461188.8618,8.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 15534 20260528.3618 8.89CV 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 05 28.3618 2461188.8618 8.99 02:25:42.03 +56:37:15.5
135.66860 -3.90170 galactic Per Second-epoch detections are separated by 2.4" and 7.8 pix
The object was found in VSX 5" ASASSN-V J022542.34+563711.6
Type: SR
# Max. Min./Amp. JD0 Period
12.400 V 12.550 V 2458546.70420 284.180457300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:42.03 +56:37:15.5: 13.08 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:42.03 +56:37:15.5: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 25 42.03 +56 37 15.5 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022542.34+563711.6,2461188.8618,8.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022542.34+563711.6 20260528.3618 8.99CV 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 05 28.3618 2461188.8618 8.88 02:36:59.24 +57:56:30.4
136.58592 -2.10437 galactic Cas Second-epoch detections are separated by 3.0" and 6.6 pix
The object was found in VSX19" Gaia DR3 458140695435098880
Type: ROT
# Max. Min./Amp. JD0 Period
15.900 G 15.940 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:59.24 +57:56:30.4: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:59.24 +57:56:30.4: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 36 59.24 +57 56 30.4 8.9 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 458140695435098880,2461188.8618,8.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458140695435098880 20260528.3618 8.88CV 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 05 28.3618 2461188.8618 8.85 02:33:03.14 +57:03:26.9
136.44292 -3.12463 galactic Per Second-epoch detections are separated by 2.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2584+57.0472 | 02:33:03.33 +57:03:28.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.027+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:03.14 +57:03:26.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:03.14 +57:03:26.9: 11.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 33 03.14 +57 03 26.9 8.8 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 J038.2584+57.0472,2461188.8618,8.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.2584+57.0472 20260528.3618 8.85CV 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 05 28.3618 2461188.8618 8.94 02:36:07.89 +57:21:40.2
136.70982 -2.68306 galactic Per Second-epoch detections are separated by 3.8" 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 457911653417858560 | 02:36:07.78 +57:21:40.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.113+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:07.89 +57:21:40.2: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:07.89 +57:21:40.2: 11.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.24 +/- 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 05 28.3618* 02 36 07.89 +57 21 40.2 8.9 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 457911653417858560,2461188.8618,8.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457911653417858560 20260528.3618 8.94CV 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 05 28.3618 2461188.8618 8.96 02:20:24.36 +56:41:46.0
134.95856 -4.08383 galactic Per Second-epoch detections are separated by 2.6" and 7.2 pix
The object was found in VSX 3" ASASSN-V J022024.69+564144.6
Type: L
# Max. Min./Amp. JD0 Period
12.350 V 12.450 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:24.36 +56:41:46.0: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:24.36 +56:41:46.0: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 20 24.36 +56 41 46.0 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022024.69+564144.6,2461188.8618,8.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022024.69+564144.6 20260528.3618 8.96CV 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 05 28.3618 2461188.8618 8.94 02:20:07.34 +56:27:53.6
134.99989 -4.31468 galactic Per 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 | Gaia DR3 458274320459648000 | 02:20:07.35 +56:27:51.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.713+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:07.34 +56:27:53.6: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:07.34 +56:27:53.6: 11.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 20 07.34 +56 27 53.6 8.9 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 458274320459648000,2461188.8618,8.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458274320459648000 20260528.3618 8.94CV 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 05 28.3618 2461188.8618 9.06 02:26:02.45 +56:20:59.5
135.80969 -4.13813 galactic Per Second-epoch detections are separated by 0.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.5102+56.3494 | 02:26:02.46 +56:20:57.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.146+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:02.45 +56:20:59.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:02.45 +56:20:59.5: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 26 02.45 +56 20 59.5 9.1 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
ATO J036.5102+56.3494,2461188.8618,9.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J036.5102+56.3494 20260528.3618 9.06CV 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 05 28.3618 2461188.8618 9.18 02:26:00.91 +56:46:18.9
135.65500 -3.74528 galactic Per Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457636122678005120 | 02:26:00.79 +56:46:18.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.239+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:00.91 +56:46:18.9: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:00.91 +56:46:18.9: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 26 00.91 +56 46 18.9 9.2 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 457636122678005120,2461188.8618,9.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457636122678005120 20260528.3618 9.18CV 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 05 28.3618 2461188.8618 9.04 02:33:37.63 +57:40:23.9
136.27827 -2.52612 galactic Per Second-epoch detections are separated by 4.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4074+57.6734 | 02:33:40.23 +57:40:02.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.496+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:37.63 +57:40:23.9: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:37.63 +57:40:23.9: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 33 37.63 +57 40 23.9 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4074+57.6734,2461188.8618,9.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.4074+57.6734 20260528.3618 9.04CV 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 05 28.3618 2461188.8618 9.10 02:24:52.65 +56:43:13.3
135.52730 -3.84894 galactic Per Second-epoch detections are separated by 2.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457632652344319616 | 02:24:52.42 +56:43:10.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:52.65 +56:43:13.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:52.65 +56:43:13.3: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 24 52.65 +56 43 13.3 9.1 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 457632652344319616,2461188.8618,9.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457632652344319616 20260528.3618 9.10CV 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 05 28.3618 2461188.8618 9.07 02:40:00.93 +58:49:46.1
136.59353 -1.13205 galactic Cas Second-epoch detections are separated by 5.2" and 6.1 pix
The object was found in VSX20" Gaia DR3 464205979529555200
Type: E
# Max. Min./Amp. JD0 Period
17.000 G 17.080 G 0.278418000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:40:00.93 +58:49:46.1: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:40:00.93 +58:49:46.1: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 40 00.93 +58 49 46.1 9.1 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 464205979529555200,2461188.8618,9.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 464205979529555200 20260528.3618 9.07CV 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 05 28.3618 2461188.8618 9.00 02:38:18.56 +57:37:39.8
136.87279 -2.32231 galactic Cas Second-epoch detections are separated by 4.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457942474103581568 | 02:38:18.15 +57:37:36.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:18.56 +57:37:39.8: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:18.56 +57:37:39.8: 11.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 38 18.56 +57 37 39.8 9.0 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 457942474103581568,2461188.8618,9.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457942474103581568 20260528.3618 9.00CV 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 05 28.3618 2461188.8618 9.12 02:27:22.97 +56:19:26.0
135.99300 -4.09534 galactic Per Second-epoch detections are separated by 2.3" and 7.2 pix
The object was found in VSX 1" Gaia DR3 457562214879587968
Type: BE|GCAS|S
# Max. Min./Amp. JD0 Period
11.540 G 11.620 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:22.97 +56:19:26.0: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:22.97 +56:19:26.0: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 27 22.97 +56 19 26.0 9.1 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 457562214879587968,2461188.8618,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457562214879587968 20260528.3618 9.12CV 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 05 28.3618 2461188.8618 9.12 02:25:30.00 +56:16:55.3
135.76374 -4.22826 galactic Per Second-epoch detections are separated by 2.3" and 7.5 pix
The object was found in VSX14" Gaia DR3 457517925178383616
Type: E
# Max. Min./Amp. JD0 Period
16.000 G 16.110 G 1.956010000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:30.00 +56:16:55.3: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:30.00 +56:16:55.3: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 25 30.00 +56 16 55.3 9.1 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 457517925178383616,2461188.8618,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457517925178383616 20260528.3618 9.12CV 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 05 28.3618 2461188.8618 9.24 02:30:16.58 +56:38:11.3
136.25011 -3.65776 galactic Per Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457587263129458432 | 02:30:17.01 +56:38:06.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:16.58 +56:38:11.3: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:16.58 +56:38:11.3: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 30 16.58 +56 38 11.3 9.2 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 457587263129458432,2461188.8618,9.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457587263129458432 20260528.3618 9.24CV 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 05 28.3618 2461188.8618 10.16 01:22:23.94 +61:13:51.2
126.64959 -1.41717 galactic Cas Second-epoch detections are separated by 1.0" and 7.7 pix
The object was found in VSX 1" NSVS J0122238+611352
Type: M
# Max. Min./Amp. JD0 Period
14.871 r Y 3.740 r 2458328.87710 325.120339600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:23.94 +61:13:51.2: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:23.94 +61:13:51.2: 15.76 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.76 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 22 23.94 +61 13 51.2 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0122238+611352,2461188.8618,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3618 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 10.39 00:52:12.67 +64:57:20.9
123.01380 2.08418 galactic Cas Second-epoch detections are separated by 3.0" 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 | Gaia DR3 524435405436784000 | 00:52:06.66 +64:57:18.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1966UppAn...5d...1O [O66] 9: 83 J-Ks=0.408+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:12.67 +64:57:20.9: 12.79 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:12.67 +64:57:20.9: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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 05 28.3618* 00 52 12.67 +64 57 20.9 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 524435405436784000,2461188.8618,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 524435405436784000 20260528.3618 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.09 01:38:21.64 +57:13:51.3
129.27457 -5.06186 galactic Cas Second-epoch detections are separated by 0.3" and 7.7 pix
The object was found in VSX 4" NSV 572
Type:
# Max. Min./Amp. JD0 Period
11.900 V Y 1.100 V M3V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:21.64 +57:13:51.3: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:21.64 +57:13:51.3: 11.28 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.28 +/- 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 05 28.3618* 01 38 21.64 +57 13 51.3 8.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 572,2461188.8618,8.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 572 20260528.3618 8.09CV 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 05 28.3618 2461188.8618 10.34 01:50:36.43 +63:53:30.1
129.38618 1.76389 galactic Cas Second-epoch detections are separated by 4.4" and 7.6 pix
The object was found in VSX 5" ASASSN-V J015036.60+635335.1
Type: SR
# Max. Min./Amp. JD0 Period
14.850 V 15.220 V 2458062.97400 59.670000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:36.43 +63:53:30.1: 11.56 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:36.43 +63:53:30.1: 14.42 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.66 +/- 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 05 28.3618* 01 50 36.43 +63 53 30.1 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J015036.60+635335.1,2461188.8618,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015036.60+635335.1 20260528.3618 10.34CV 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 05 28.3618 2461188.8618 9.71 02:41:50.08 +65:30:27.2
134.04888 5.04694 galactic Cas Second-epoch detections are separated by 0.9" 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 516122646547535360 | 02:41:50.26 +65:30:27.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.507+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:41:50.08 +65:30:27.2: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:41:50.08 +65:30:27.2: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 05 28.3618* 02 41 50.08 +65 30 27.2 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 516122646547535360,2461188.8618,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 516122646547535360 20260528.3618 9.71CV 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 05 28.3618 2461188.8618 9.26 02:09:48.70 +59:51:47.0
132.62818 -1.52504 galactic Cas Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 507141839875969024 | 02:09:48.78 +59:51:46.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.553+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:48.70 +59:51:47.0: 11.32 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:48.70 +59:51:47.0: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 09 48.70 +59 51 47.0 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507141839875969024,2461188.8618,9.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507141839875969024 20260528.3618 9.26CV 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 05 28.3618 2461188.8618 8.97 01:31:28.19 +57:20:36.7
128.33423 -5.10772 galactic Cas Second-epoch detections are separated by 0.8" and 7.7 pix
The object was found in VSX 3" GSC 03678-01834
Type: SR
# Max. Min./Amp. JD0 Period
14.581 g Y 1.075 g 2458615.68850 389.528443900000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:28.19 +57:20:36.7: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:28.19 +57:20:36.7: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 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 05 28.3618* 01 31 28.19 +57 20 36.7 9.0 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
GSC 03678-01834,2461188.8618,8.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 03678-01834 20260528.3618 8.97CV 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 05 28.3618 2461188.8618 9.01 02:24:46.68 +59:43:52.9
134.45088 -1.03648 galactic Cas Second-epoch detections are separated by 1.2" and 7.3 pix
The object was found in VSX 4" ZTF J022447.07+594349.5
Type: SR
# Max. Min./Amp. JD0 Period
16.219 g Y 0.561 g 2458393.52880 216.330969400000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:46.68 +59:43:52.9: 13.02 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:46.68 +59:43:52.9: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 24 46.68 +59 43 52.9 9.0 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 J022447.07+594349.5,2461188.8618,9.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022447.07+594349.5 20260528.3618 9.01CV 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 05 28.3618 2461188.8618 8.88 02:48:49.52 +64:11:51.9
135.28236 4.17794 galactic Cas Second-epoch detections are separated by 0.2" and 6.6 pix
The object was found in VSX 3" ASASSN-V J024850.01+641152.3
Type: SR
# Max. Min./Amp. JD0 Period
13.490 V 14.080 V 2457721.90000 186.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:48:49.52 +64:11:51.9: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:48:49.52 +64:11:51.9: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 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 05 28.3618* 02 48 49.52 +64 11 51.9 8.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J024850.01+641152.3,2461188.8618,8.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J024850.01+641152.3 20260528.3618 8.88CV 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 05 28.3618 2461188.8618 9.31 01:12:18.51 +60:20:30.2
125.51336 -2.42538 galactic Cas Second-epoch detections are separated by 0.9" and 7.8 pix
The object was found in VSX 2" ASASSN-V J011218.29+602030.0
Type: L
# Max. Min./Amp. JD0 Period
13.680 V 14.240 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:18.51 +60:20:30.2: 12.68 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:18.51 +60:20:30.2: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 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 05 28.3618* 01 12 18.51 +60 20 30.2 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J011218.29+602030.0,2461188.8618,9.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011218.29+602030.0 20260528.3618 9.31CV 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 05 28.3618 2461188.8618 8.99 02:15:20.43 +62:13:50.0
132.53409 0.93325 galactic Cas Second-epoch detections are separated by 0.6" and 7.0 pix
The object was found in VSX 0" V0930 Cas
Type: SR
# Max. Min./Amp. JD0 Period
13.300 V 14.200 V 2451443.00000 129.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:20.43 +62:13:50.0: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:20.43 +62:13:50.0: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 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 05 28.3618* 02 15 20.43 +62 13 50.0 9.0 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
V0930 Cas,2461188.8618,8.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0930 Cas 20260528.3618 8.99CV 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 05 28.3618 2461188.8618 8.62 02:05:05.77 +58:16:24.6
132.50925 -3.22196 galactic Per Second-epoch detections are separated by 1.3" and 7.2 pix
The object was found in VSX 2" V0661 Per
Type: SR:
# Max. Min./Amp. JD0 Period
13.500 V 14.200 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:05:05.77 +58:16:24.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:05:05.77 +58:16:24.6: 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 05 28.3618* 02 05 05.77 +58 16 24.6 8.6 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
V0661 Per,2461188.8618,8.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0661 Per 20260528.3618 8.62CV 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 05 28.3618 2461188.8618 9.53 02:24:05.02 +63:37:15.8
133.00666 2.57624 galactic Cas Second-epoch detections are separated by 2.3" and 7.0 pix
The object was found in VSX 1" ZTF J022405.02+633716.5
Type: SR
# Max. Min./Amp. JD0 Period
12.535 r Y 0.233 r 2458431.84820 29.152836600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:05.02 +63:37:15.8: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:05.02 +63:37:15.8: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 24 05.02 +63 37 15.8 9.5 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
ZTF J022405.02+633716.5,2461188.8618,9.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022405.02+633716.5 20260528.3618 9.53CV 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 05 28.3618 2461188.8618 9.57 01:15:48.97 +62:13:51.2
125.76735 -0.50657 galactic Cas Second-epoch detections are separated by 3.7" and 7.8 pix
The object was found in VSX 2" NSVS 1688453
Type: L
# Max. Min./Amp. JD0 Period
10.700 R1 11.100 R1
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:48.97 +62:13:51.2: 12.03 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:48.97 +62:13:51.2: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 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 05 28.3618* 01 15 48.97 +62 13 51.2 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1688453,2461188.8618,9.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1688453 20260528.3618 9.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.70 01:22:16.36 +57:23:06.8
127.09531 -5.23706 galactic Cas Second-epoch detections are separated by 1.0" and 8.1 pix
The object was found in VSX 1" V0467 Cas
Type: SRB
# Max. Min./Amp. JD0 Period
15.400 pg 16.100 pg 100.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:16.36 +57:23:06.8: 11.95 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:16.36 +57:23:06.8: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 05 28.3618* 01 22 16.36 +57 23 06.8 8.7 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
V0467 Cas,2461188.8618,8.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0467 Cas 20260528.3618 8.70CV 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 05 28.3618 2461188.8618 9.19 01:54:12.35 +65:38:24.8
129.34942 3.55357 galactic Cas Second-epoch detections are separated by 5.7" and 7.1 pix
The object was found in VSX 5" ASASSN-V J015412.96+653821.5
Type: SR
# Max. Min./Amp. JD0 Period
15.066 g Y 0.472 g 2458273.34030 131.503552200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:12.35 +65:38:24.8: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:12.35 +65:38:24.8: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 54 12.35 +65 38 24.8 9.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J015412.96+653821.5,2461188.8618,9.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015412.96+653821.5 20260528.3618 9.19CV 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 05 28.3618 2461188.8618 10.01 02:14:27.98 +64:44:14.9
131.64562 3.27972 galactic Cas Second-epoch detections are separated by 1.1" and 6.9 pix
The object was found in VSX 1" NSVS J0214284+644418
Type: SR
# Max. Min./Amp. JD0 Period
12.916 r Y 0.345 r 2458352.87040 121.127267000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:27.98 +64:44:14.9: 11.50 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:14:27.98 +64:44:14.9: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 14 27.98 +64 44 14.9 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0214284+644418,2461188.8618,10.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0214284+644418 20260528.3618 10.01CV 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 05 28.3618 2461188.8618 8.80 01:21:54.86 +61:20:56.1
126.57773 -1.30691 galactic Cas Second-epoch detections are separated by 2.2" and 7.8 pix
The object was found in ASASSN-V 2" ASASSN-V J012154.67+612055.1
Type: SR
MeanMag 14.81 m Amp. 2.24 m Period 397.1456143 d
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:54.86 +61:20:56.1: 13.28 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:54.86 +61:20:56.1: 14.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.27 +/- 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 05 28.3618* 01 21 54.86 +61 20 56.1 8.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461188.8618,8.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3618 8.80CV 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 05 28.3618 2461188.8618 8.69 02:39:22.81 +60:42:41.0
135.75827 0.55626 galactic Cas Second-epoch detections are separated by 1.0" and 6.9 pix
The object was found in VSX 1" NSVS J0239228+604243
Type: SR
# Max. Min./Amp. JD0 Period
15.176 g Y 0.404 g 2458492.18530 283.071355700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:39:22.81 +60:42:41.0: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:39:22.81 +60:42:41.0: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 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 05 28.3618* 02 39 22.81 +60 42 41.0 8.7 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
NSVS J0239228+604243,2461188.8618,8.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0239228+604243 20260528.3618 8.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.79 01:57:52.45 +64:34:23.0
129.98889 2.61545 galactic Cas Second-epoch detections are separated by 3.8" and 7.8 pix
The object was found in VSX 1" ASASSN-V J015752.36+643422.1
Type: SR
# Max. Min./Amp. JD0 Period
13.750 V 13.890 V 2457671.00000 440.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:52.45 +64:34:23.0: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:52.45 +64:34:23.0: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 57 52.45 +64 34 23.0 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J015752.36+643422.1,2461188.8618,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015752.36+643422.1 20260528.3618 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.80 02:34:40.00 +63:00:03.4
134.34112 2.43876 galactic Cas Second-epoch detections are separated by 1.0" and 6.7 pix
The object was found in VSX 2" V0677 Cas
Type: SRB
# Max. Min./Amp. JD0 Period
13.100 V 14.100 V 2457609.00000 131.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:40.00 +63:00:03.4: 13.16 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:40.00 +63:00:03.4: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 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 05 28.3618* 02 34 40.00 +63 00 03.4 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
V0677 Cas,2461188.8618,8.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0677 Cas 20260528.3618 8.80CV 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 05 28.3618 2461188.8618 8.64 02:25:13.42 +56:30:32.3
135.64702 -4.02974 galactic Per Second-epoch detections are separated by 2.3" 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 | ATO J036.2868+56.5107 | 02:25:13.36 +56:30:32.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.108+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:13.42 +56:30:32.3: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:13.42 +56:30:32.3: 10.84 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.84 +/- 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 05 28.3618* 02 25 13.42 +56 30 32.3 8.6 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 J036.2868+56.5107,2461188.8618,8.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J036.2868+56.5107 20260528.3618 8.64CV 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 05 28.3618 2461188.8618 9.45 02:19:04.00 +62:47:33.4
132.75781 1.60462 galactic Cas Second-epoch detections are separated by 2.0" and 6.7 pix
The object was found in VSX 1" ASASSN-V J021904.01+624734.4
Type: SR
# Max. Min./Amp. JD0 Period
13.890 V 14.180 V 2457429.00000 487.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:04.00 +62:47:33.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:04.00 +62:47:33.4: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 19 04.00 +62 47 33.4 9.4 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
ASASSN-V J021904.01+624734.4,2461188.8618,9.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021904.01+624734.4 20260528.3618 9.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.03 02:15:35.96 +56:21:40.4
134.44150 -4.61820 galactic Per Second-epoch detections are separated by 0.9" 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 | ATO J033.8885+56.3660 | 02:15:35.87 +56:21:38.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.581+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:35.96 +56:21:40.4: 12.85 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:35.96 +56:21:40.4: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 15 35.96 +56 21 40.4 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J033.8885+56.3660,2461188.8618,9.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J033.8885+56.3660 20260528.3618 9.03CV 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 05 28.3618 2461188.8618 8.95 01:47:43.89 +62:06:37.4
129.46316 -0.04540 galactic Cas Second-epoch detections are separated by 2.3" and 7.2 pix
The object was found in VSX 1" NSVS J0147440+620637
Type: SR
# Max. Min./Amp. JD0 Period
15.041 g Y 1.391 g 2458483.67330 389.145592000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:43.89 +62:06:37.4: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:43.89 +62:06:37.4: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 05 28.3618* 01 47 43.89 +62 06 37.4 8.9 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 J0147440+620637,2461188.8618,8.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0147440+620637 20260528.3618 8.95CV 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 05 28.3618 2461188.8618 8.49 02:31:25.66 +60:43:53.6
134.85511 0.19561 galactic Cas Second-epoch detections are separated by 1.2" and 7.1 pix
The object was found in VSX 2" ASASSN-V J023125.87+604353.3
Type: SR
# Max. Min./Amp. JD0 Period
12.740 V 13.020 V 2458409.47890 189.305491500000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:25.66 +60:43:53.6: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:25.66 +60:43:53.6: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 31 25.66 +60 43 53.6 8.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J023125.87+604353.3,2461188.8618,8.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J023125.87+604353.3 20260528.3618 8.49CV 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 05 28.3618 2461188.8618 9.40 02:45:57.12 +62:02:43.5
135.92024 2.09654 galactic Cas Second-epoch detections are separated by 3.5" and 6.8 pix
The object was found in VSX 3" NSVS J0245576+620244
Type: L:
# Max. Min./Amp. JD0 Period
11.833 R1 Y 0.378 R1 578.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:45:57.12 +62:02:43.5: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:45:57.12 +62:02:43.5: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 05 28.3618* 02 45 57.12 +62 02 43.5 9.4 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
NSVS J0245576+620244,2461188.8618,9.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0245576+620244 20260528.3618 9.40CV 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 05 28.3618 2461188.8618 8.37 02:07:48.46 +61:22:16.5
131.94857 -0.15636 galactic Cas Second-epoch detections are separated by 1.4" and 7.0 pix
The object was found in VSX 2" ASASSN-V J020748.38+612218.0
Type: L:
# Max. Min./Amp. JD0 Period
12.500 V 12.960 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:48.46 +61:22:16.5: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:48.46 +61:22:16.5: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 07 48.46 +61 22 16.5 8.4 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
ASASSN-V J020748.38+612218.0,2461188.8618,8.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020748.38+612218.0 20260528.3618 8.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.05 02:36:10.97 +60:22:42.0
135.53038 0.09421 galactic Cas Second-epoch detections are separated by 1.2" and 7.1 pix
The object was found in VSX 3" NSV 858
Type: LB
# Max. Min./Amp. JD0 Period
15.500 pg 16.500 pg 567.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:10.97 +60:22:42.0: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:10.97 +60:22:42.0: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 36 10.97 +60 22 42.0 8.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 858,2461188.8618,8.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 858 20260528.3618 8.05CV 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 05 28.3618 2461188.8618 9.52 01:23:04.06 +57:36:35.9
127.17435 -5.00100 galactic Cas Second-epoch detections are separated by 1.4" and 7.8 pix
The object was found in VSX 5" NSVS J0123038+573632
Type: L:
# Max. Min./Amp. JD0 Period
11.731 R1 Y 0.622 R1 436.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:04.06 +57:36:35.9: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:04.06 +57:36:35.9: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 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 05 28.3618* 01 23 04.06 +57 36 35.9 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0123038+573632,2461188.8618,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0123038+573632 20260528.3618 9.52CV 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 05 28.3618 2461188.8618 7.89 02:24:29.68 +59:24:31.5
134.53091 -1.35106 galactic Cas Second-epoch detections are separated by 0.1" and 7.2 pix
The object was found in VSX 2" V0672 Cas
Type: SR
# Max. Min./Amp. JD0 Period
15.000 B 17.400 B 302.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:29.68 +59:24:31.5: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:29.68 +59:24:31.5: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 24 29.68 +59 24 31.5 7.9 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
V0672 Cas,2461188.8618,7.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0672 Cas 20260528.3618 7.89CV 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 05 28.3618 2461188.8618 8.46 01:43:58.28 +58:41:06.0
129.72677 -3.49197 galactic Cas Second-epoch detections are separated by 1.3" and 7.8 pix
The object was found in VSX 1" V0918 Cas
Type: SR
# Max. Min./Amp. JD0 Period
12.100 V 13.300 V 2458494.59580 95.740940700000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:58.28 +58:41:06.0: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:58.28 +58:41:06.0: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 43 58.28 +58 41 06.0 8.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0918 Cas,2461188.8618,8.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0918 Cas 20260528.3618 8.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.91 01:36:21.66 +60:26:52.3
128.44738 -1.94193 galactic Cas Second-epoch detections are separated by 0.9" and 7.7 pix
The object was found in VSX 0" ASASSN-V J013621.62+602652.3
Type: L:
# Max. Min./Amp. JD0 Period
13.850 V 14.490 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:21.66 +60:26:52.3: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:21.66 +60:26:52.3: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 36 21.66 +60 26 52.3 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013621.62+602652.3,2461188.8618,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J013621.62+602652.3 20260528.3618 9.91CV 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 05 28.3618 2461188.8618 9.46 02:05:50.44 +62:42:31.3
131.34319 1.05831 galactic Cas Second-epoch detections are separated by 1.9" and 6.9 pix
The object was found in VSX 1" ASASSN-V J020550.42+624232.7
Type: SR
# Max. Min./Amp. JD0 Period
13.710 V 14.110 V 2458511.64170 109.004338400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:05:50.44 +62:42:31.3: 10.57 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:05:50.44 +62:42:31.3: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 05 50.44 +62 42 31.3 9.5 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 J020550.42+624232.7,2461188.8618,9.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020550.42+624232.7 20260528.3618 9.46CV 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 05 28.3618 2461188.8618 8.43 02:08:54.01 +58:42:29.5
132.86018 -2.66236 galactic Per Second-epoch detections are separated by 0.1" and 7.3 pix
The object was found in VSX 2" NSVS J0208545+584228
Type: SRB
# Max. Min./Amp. JD0 Period
13.200 V 14.100 V M7.5III
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:08:54.01 +58:42:29.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:08:54.01 +58:42:29.5: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 08 54.01 +58 42 29.5 8.4 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
NSVS J0208545+584228,2461188.8618,8.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0208545+584228 20260528.3618 8.43CV 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 05 28.3618 2461188.8618 8.48 02:31:46.08 +56:26:43.2
136.51298 -3.75772 galactic Per 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 | Gaia DR3 457393336767227264 | 02:31:45.96 +56:26:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:46.08 +56:26:43.2: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:46.08 +56:26:43.2: 10.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.75 +/- 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 05 28.3618* 02 31 46.08 +56 26 43.2 8.5 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 457393336767227264,2461188.8618,8.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457393336767227264 20260528.3618 8.48CV 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 05 28.3618 2461188.8618 9.20 02:19:12.27 +57:48:50.2
134.42956 -3.08523 galactic Per Second-epoch detections are separated by 0.5" and 7.4 pix
The object was found in VSX 1" ZTF J021912.38+574849.4
Type: SR
# Max. Min./Amp. JD0 Period
12.406 r Y 0.170 r 2458351.95870 40.759405700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:12.27 +57:48:50.2: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:12.27 +57:48:50.2: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 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 05 28.3618* 02 19 12.27 +57 48 50.2 9.2 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
ZTF J021912.38+574849.4,2461188.8618,9.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021912.38+574849.4 20260528.3618 9.20CV 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 05 28.3618 2461188.8618 9.45 02:11:32.08 +65:25:28.2
131.13767 3.83680 galactic Cas Second-epoch detections are separated by 2.5" and 7.2 pix
The object was found in VSX 4" ZTF J021131.38+652527.9
Type: SR
# Max. Min./Amp. JD0 Period
15.113 g Y 0.264 g 2458368.92030 86.377729200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:32.08 +65:25:28.2: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:32.08 +65:25:28.2: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 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 05 28.3618* 02 11 32.08 +65 25 28.2 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J021131.38+652527.9,2461188.8618,9.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021131.38+652527.9 20260528.3618 9.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.99 02:24:34.96 +61:05:35.0
133.94871 0.22948 galactic Cas Second-epoch detections are separated by 1.3" and 7.3 pix
The object was found in VSX 1" V1336 Cas
Type: SR
# Max. Min./Amp. JD0 Period
11.000 CR 11.200 CR 2451525.00000 51.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:34.96 +61:05:35.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:34.96 +61:05:35.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 05 28.3618* 02 24 34.96 +61 05 35.0 9.0 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
V1336 Cas,2461188.8618,8.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1336 Cas 20260528.3618 8.99CV 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 05 28.3618 2461188.8618 8.38 02:11:34.44 +59:06:06.6
133.07147 -2.18323 galactic Cas Second-epoch detections are separated by 0.4" and 7.2 pix
The object was found in VSX 1" V1003 Cas
Type: SR
# Max. Min./Amp. JD0 Period
14.000 pg 14.600 pg 2458423.81740 37.665780900000 M6
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:34.44 +59:06:06.6: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:34.44 +59:06:06.6: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 11 34.44 +59 06 06.6 8.4 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
V1003 Cas,2461188.8618,8.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1003 Cas 20260528.3618 8.38CV 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 05 28.3618 2461188.8618 8.44 02:24:19.53 +64:16:12.9
132.80344 3.19347 galactic Cas Second-epoch detections are separated by 0.6" and 6.9 pix
The object was found in VSX 0" ASASSN-V J022419.55+641613.2
Type: SR
# Max. Min./Amp. JD0 Period
12.270 V 12.520 V 2457609.03000 44.810000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:19.53 +64:16:12.9: 9.33 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:19.53 +64:16:12.9: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 24 19.53 +64 16 12.9 8.4 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
ASASSN-V J022419.55+641613.2,2461188.8618,8.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022419.55+641613.2 20260528.3618 8.44CV 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 05 28.3618 2461188.8618 8.43 02:19:16.53 +59:42:22.1
133.80777 -1.29792 galactic Cas Second-epoch detections are separated by 1.2" and 7.4 pix
The object was found in VSX 2" ZTF J021916.76+594221.6
Type: SR
# Max. Min./Amp. JD0 Period
14.063 g Y 0.424 g 2458349.86040 72.477681200000 MS
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:16.53 +59:42:22.1: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:16.53 +59:42:22.1: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 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 05 28.3618* 02 19 16.53 +59 42 22.1 8.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J021916.76+594221.6,2461188.8618,8.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021916.76+594221.6 20260528.3618 8.43CV 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 05 28.3618 2461188.8618 8.44 01:41:01.13 +61:31:00.7
128.80805 -0.78793 galactic Cas Second-epoch detections are separated by 1.5" and 7.5 pix
The object was found in VSX 1" ZALD J01410104+6131013
Type: SRB
# Max. Min./Amp. JD0 Period
12.400 V 13.000 V 2457358.80000 60.100000000000 M4III
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:01.13 +61:31:00.7: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:01.13 +61:31:00.7: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 41 01.13 +61 31 00.7 8.4 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
ZALD J01410104+6131013,2461188.8618,8.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZALD J01410104+6131013 20260528.3618 8.44CV 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 05 28.3618 2461188.8618 9.20 02:09:24.81 +60:03:15.6
132.52361 -1.35729 galactic Cas Second-epoch detections are separated by 8.0" and 7.5 pix
The object was found in VSX 7" ASASSN-V J020924.02+600312.9
Type: SR
# Max. Min./Amp. JD0 Period
13.330 V 13.420 V 2458034.95100 32.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:24.81 +60:03:15.6: 12.74 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:24.81 +60:03:15.6: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 09 24.81 +60 03 15.6 9.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J020924.02+600312.9,2461188.8618,9.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020924.02+600312.9 20260528.3618 9.20CV 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 05 28.3618 2461188.8618 8.38 02:01:05.84 +58:11:26.9
132.02496 -3.44581 galactic Cas Second-epoch detections are separated by 0.7" and 7.5 pix
The object was found in VSX 1" ASASSN-V J020105.84+581125.5
Type: SR
# Max. Min./Amp. JD0 Period
13.587 g Y 0.553 g 2458291.67700 79.510632800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:05.84 +58:11:26.9: 11.21 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:05.84 +58:11:26.9: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 01 05.84 +58 11 26.9 8.4 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
ASASSN-V J020105.84+581125.5,2461188.8618,8.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020105.84+581125.5 20260528.3618 8.38CV 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 05 28.3618 2461188.8618 8.95 01:56:15.73 +60:01:03.3
130.95339 -1.84072 galactic Cas Second-epoch detections are separated by 1.5" and 7.3 pix
The object was found in VSX 2" V0923 Cas
Type: SR
# Max. Min./Amp. JD0 Period
12.400 V 13.800 V 2458344.05090 130.746157700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:15.73 +60:01:03.3: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:15.73 +60:01:03.3: 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 05 28.3618* 01 56 15.73 +60 01 03.3 8.9 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
V0923 Cas,2461188.8618,8.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0923 Cas 20260528.3618 8.95CV 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 05 28.3618 2461188.8618 9.04 02:24:41.13 +58:22:35.6
134.91756 -2.30850 galactic Per Second-epoch detections are separated by 3.4" and 7.6 pix
The object was found in VSX 3" ASASSN-V J022441.46+582233.3
Type: SR
# Max. Min./Amp. JD0 Period
14.827 g Y 0.387 g 2458366.56600 67.480010700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:41.13 +58:22:35.6: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:41.13 +58:22:35.6: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 05 28.3618* 02 24 41.13 +58 22 35.6 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022441.46+582233.3,2461188.8618,9.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022441.46+582233.3 20260528.3618 9.04CV 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 05 28.3618 2461188.8618 9.09 02:20:33.64 +60:06:16.7
133.82599 -0.86848 galactic Cas Second-epoch detections are separated by 1.0" and 7.2 pix
The object was found in VSX 0" ZTF J022033.66+600616.9
Type: SR
# Max. Min./Amp. JD0 Period
14.476 g Y 0.234 g 2458278.00000 98.864770600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:33.64 +60:06:16.7: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:33.64 +60:06:16.7: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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 05 28.3618* 02 20 33.64 +60 06 16.7 9.1 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 J022033.66+600616.9,2461188.8618,9.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022033.66+600616.9 20260528.3618 9.09CV 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 05 28.3618 2461188.8618 9.93 01:27:44.43 +62:06:40.7
127.16335 -0.46182 galactic Cas Second-epoch detections are separated by 1.5" and 7.7 pix
The object was found in VSX 2" NSVS 1696374
Type: SR
# Max. Min./Amp. JD0 Period
11.950 R1 12.250 R1 2451454.00000 193.000000000000 : C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:44.43 +62:06:40.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:44.43 +62:06:40.7: 13.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.97 +/- 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 05 28.3618* 01 27 44.43 +62 06 40.7 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1696374,2461188.8618,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1696374 20260528.3618 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.24 02:03:34.92 +64:11:47.7
130.68421 2.41611 galactic Cas Second-epoch detections are separated by 1.9" and 7.4 pix
The object was found in VSX 0" GSC 04041-00983
Type: SR
# Max. Min./Amp. JD0 Period
14.801 g Y 0.368 g 2458304.54220 282.263656600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:34.92 +64:11:47.7: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:34.92 +64:11:47.7: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 05 28.3618* 02 03 34.92 +64 11 47.7 9.2 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
GSC 04041-00983,2461188.8618,9.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 04041-00983 20260528.3618 9.24CV 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 05 28.3618 2461188.8618 9.60 01:41:46.93 +59:03:48.0
129.37382 -3.17729 galactic Cas Second-epoch detections are separated by 1.8" and 7.9 pix
The object was found in VSX 1" ASASSN-V J014146.93+590346.7
Type: SR
# Max. Min./Amp. JD0 Period
13.670 V 14.220 V 2457304.00000 93.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:46.93 +59:03:48.0: 11.44 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:46.93 +59:03:48.0: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 05 28.3618* 01 41 46.93 +59 03 48.0 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014146.93+590346.7,2461188.8618,9.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J014146.93+590346.7 20260528.3618 9.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.41 02:28:12.08 +64:31:52.8
133.10122 3.58726 galactic Cas Second-epoch detections are separated by 1.2" and 7.0 pix
The object was found in VSX 1" NSVS J0228122+643156
Type: SR
# Max. Min./Amp. JD0 Period
13.081 r Y 0.937 r 2458466.24640 234.996798300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:12.08 +64:31:52.8: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:12.08 +64:31:52.8: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 28 12.08 +64 31 52.8 9.4 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
NSVS J0228122+643156,2461188.8618,9.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0228122+643156 20260528.3618 9.41CV 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 05 28.3618 2461188.8618 8.83 01:32:27.26 +60:20:31.1
127.98887 -2.12643 galactic Cas Second-epoch detections are separated by 2.9" and 7.3 pix
The object was found in VSX 2" ZTF J013227.33+602032.8
Type: SR
# Max. Min./Amp. JD0 Period
13.814 g Y 0.161 g 2458339.10650 60.766191500000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:27.26 +60:20:31.1: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:27.26 +60:20:31.1: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 32 27.26 +60 20 31.1 8.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J013227.33+602032.8,2461188.8618,8.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J013227.33+602032.8 20260528.3618 8.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.51 01:54:09.12 +61:13:07.0
130.40861 -0.73945 galactic Cas Second-epoch detections are separated by 2.2" and 7.3 pix
The object was found in VSX 1" NSVS 1818095
Type: SR
# Max. Min./Amp. JD0 Period
15.101 g Y 0.350 R1 2458534.94430 54.890150000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:09.12 +61:13:07.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:09.12 +61:13:07.0: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 54 09.12 +61 13 07.0 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1818095,2461188.8618,9.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1818095 20260528.3618 9.51CV 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 05 28.3618 2461188.8618 8.21 01:36:20.44 +58:31:43.2
128.77830 -3.83245 galactic Cas Second-epoch detections are separated by 0.8" and 7.8 pix
The object was found in VSX 1" V0908 Cas
Type: SR
# Max. Min./Amp. JD0 Period
12.000 V 13.200 V 2458279.23010 120.038430700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:20.44 +58:31:43.2: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:20.44 +58:31:43.2: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 36 20.44 +58 31 43.2 8.2 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
V0908 Cas,2461188.8618,8.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0908 Cas 20260528.3618 8.21CV 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 05 28.3618 2461188.8618 8.26 01:40:46.01 +60:51:39.7
128.90327 -1.43753 galactic Cas Second-epoch detections are separated by 0.7" and 7.7 pix
The object was found in VSX 0" NSV 582
Type: SR
# Max. Min./Amp. JD0 Period
13.281 g Y 0.383 g 2458327.88610 56.751554300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:46.01 +60:51:39.7: 10.73 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:46.01 +60:51:39.7: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 40 46.01 +60 51 39.7 8.3 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
NSV 582,2461188.8618,8.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 582 20260528.3618 8.26CV 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 05 28.3618 2461188.8618 9.84 01:25:43.43 +60:50:05.7
127.09911 -1.75912 galactic Cas Second-epoch detections are separated by 2.5" and 8.2 pix
The object was found in VSX 1" ZTF J012543.34+605006.2
Type: SR
# Max. Min./Amp. JD0 Period
14.923 g Y 0.462 g 2458271.66140 289.704203100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:43.43 +60:50:05.7: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:43.43 +60:50:05.7: 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 05 28.3618* 01 25 43.43 +60 50 05.7 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J012543.34+605006.2,2461188.8618,9.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J012543.34+605006.2 20260528.3618 9.84CV 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 05 28.3618 2461188.8618 8.22 01:16:28.97 +60:14:00.5
126.03867 -2.48711 galactic Cas Second-epoch detections are separated by 0.6" and 8.0 pix
The object was found in ASASSN-V 1" ASASSN-V J011628.82+601400.9
Type: SR
MeanMag 13.24 m Amp. 0.36 m Period 128.0 d
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:28.97 +60:14:00.5: 12.36 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:28.97 +60:14:00.5: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 16 28.97 +60 14 00.5 8.2 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
VARIABLE_NAME,2461188.8618,8.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3618 8.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.82 02:14:45.13 +57:39:36.6
133.91681 -3.42378 galactic Per Second-epoch detections are separated by 1.5" and 7.6 pix
The object was found in VSX 2" ZTF J021445.28+573934.7
Type: SR
# Max. Min./Amp. JD0 Period
13.843 g Y 0.223 g 2458496.34340 257.923980800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:45.13 +57:39:36.6: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:14:45.13 +57:39:36.6: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 14 45.13 +57 39 36.6 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J021445.28+573934.7,2461188.8618,8.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021445.28+573934.7 20260528.3618 8.82CV 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 05 28.3618 2461188.8618 8.01 02:28:12.53 +58:37:11.5
135.26014 -1.91629 galactic Per Second-epoch detections are separated by 2.6" and 7.4 pix
The object was found in VSX 3" NSVS J0228131+583707
Type: SR
# Max. Min./Amp. JD0 Period
14.320 g Y 0.523 g 2458299.22460 159.265202100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:12.53 +58:37:11.5: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:12.53 +58:37:11.5: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 28 12.53 +58 37 11.5 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0228131+583707,2461188.8618,8.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0228131+583707 20260528.3618 8.01CV 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 05 28.3618 2461188.8618 9.24 02:14:26.77 +64:29:24.6
131.72180 3.04440 galactic Cas Second-epoch detections are separated by 0.6" and 7.1 pix
The object was found in VSX 1" NSVS 1829693
Type: SR
# Max. Min./Amp. JD0 Period
15.478 g Y 0.301 g 2458303.52260 86.820733800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:26.77 +64:29:24.6: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:14:26.77 +64:29:24.6: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 05 28.3618* 02 14 26.77 +64 29 24.6 9.2 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
NSVS 1829693,2461188.8618,9.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1829693 20260528.3618 9.24CV 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 05 28.3618 2461188.8618 9.29 02:15:26.81 +62:47:45.7
132.36538 1.47312 galactic Cas Second-epoch detections are separated by 0.5" and 7.1 pix
The object was found in VSX 1" ASASSN-V J021526.89+624746.2
Type: SR
# Max. Min./Amp. JD0 Period
14.070 V 14.780 V 2458439.05750 300.903027600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:26.81 +62:47:45.7: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:26.81 +62:47:45.7: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 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 05 28.3618* 02 15 26.81 +62 47 45.7 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J021526.89+624746.2,2461188.8618,9.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021526.89+624746.2 20260528.3618 9.29CV 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 05 28.3618 2461188.8618 8.38 02:33:31.95 +57:34:09.2
136.30657 -2.62709 galactic Per Second-epoch detections are separated by 2.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3788+57.5785 | 02:33:31.90 +57:34:09.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B1:V 1965ApJS...12..215H Cl* NGC 957 Hoag 6 J-Ks=0.120+/-0.027 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:31.95 +57:34:09.2: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:31.95 +57:34:09.2: 10.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 33 31.95 +57 34 09.2 8.4 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
ATO J038.3788+57.5785,2461188.8618,8.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.3788+57.5785 20260528.3618 8.38CV 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 05 28.3618 2461188.8618 9.03 01:26:01.01 +59:55:35.7
127.25619 -2.65452 galactic Cas Second-epoch detections are separated by 0.7" and 7.9 pix
The object was found in VSX 1" NSVS J0125599+595536
Type: SR
# Max. Min./Amp. JD0 Period
14.287 g Y 0.715 g 2458378.98230 189.433201900000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:01.01 +59:55:35.7: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:01.01 +59:55:35.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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 05 28.3618* 01 26 01.01 +59 55 35.7 9.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0125599+595536,2461188.8618,9.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0125599+595536 20260528.3618 9.03CV 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 05 28.3618 2461188.8618 9.66 02:07:46.89 +62:11:10.9
131.70835 0.62255 galactic Cas Second-epoch detections are separated by 0.9" and 7.3 pix
The object was found in ASASSN-V 1" ASASSN-V J020746.87+621112.3
Type: SR
MeanMag 15.53 m Amp. 1.57 m Period 397.2118966 d
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:46.89 +62:11:10.9: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:46.89 +62:11:10.9: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 07 46.89 +62 11 10.9 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461188.8618,9.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3618 9.66CV 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 05 28.3618 2461188.8618 9.76 01:55:07.62 +62:47:31.4
130.13829 0.81482 galactic Cas Second-epoch detections are separated by 2.9" and 7.4 pix
The object was found in VSX 1" ASASSN-V J015507.48+624731.1
Type: SR
# Max. Min./Amp. JD0 Period
14.130 V 14.500 V 2457618.00000 81.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:07.62 +62:47:31.4: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:07.62 +62:47:31.4: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 55 07.62 +62 47 31.4 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J015507.48+624731.1,2461188.8618,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015507.48+624731.1 20260528.3618 9.76CV 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 05 28.3618 2461188.8618 9.45 02:33:47.87 +61:42:03.3
134.75034 1.20064 galactic Cas Second-epoch detections are separated by 2.4" and 7.2 pix
The object was found in VSX 1" 2MASS J02334807+6142036
Type: SR
# Max. Min./Amp. JD0 Period
13.500 V 13.820 V 2457022.00000 849.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:47.87 +61:42:03.3: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:47.87 +61:42:03.3: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 33 47.87 +61 42 03.3 9.4 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
2MASS J02334807+6142036,2461188.8618,9.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J02334807+6142036 20260528.3618 9.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.41 02:34:32.44 +64:22:56.6
133.79173 3.70668 galactic Cas Second-epoch detections are separated by 0.3" and 6.7 pix
The object was found in VSX 3" NSVS J0234320+642254
Type: SR
# Max. Min./Amp. JD0 Period
15.225 g Y 0.463 g 2458279.07310 360.302079200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:32.44 +64:22:56.6: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:32.44 +64:22:56.6: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 34 32.44 +64 22 56.6 9.4 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
NSVS J0234320+642254,2461188.8618,9.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0234320+642254 20260528.3618 9.41CV 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 05 28.3618 2461188.8618 9.39 02:23:38.25 +61:24:57.1
133.72923 0.49205 galactic Cas Second-epoch detections are separated by 2.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 513519179112924288 | 02:23:38.53 +61:24:57.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M3Ib/II 2018MNRAS.475.2003D IRAS 02198+6111 J-Ks=2.573+/-0.343 (Very red!)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:38.25 +61:24:57.1: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:38.25 +61:24:57.1: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 23 38.25 +61 24 57.1 9.4 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 513519179112924288,2461188.8618,9.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 513519179112924288 20260528.3618 9.39CV 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 05 28.3618 2461188.8618 8.02 01:47:07.73 +57:00:34.1
130.48953 -5.04284 galactic Cas Second-epoch detections are separated by 3.9" and 8.2 pix
The object was found in VSX 6" ZTF J014707.47+570028.9
Type: SR
# Max. Min./Amp. JD0 Period
13.341 g Y 0.257 g 2458277.84220 112.366103100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:07.73 +57:00:34.1: 11.98 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:07.73 +57:00:34.1: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 47 07.73 +57 00 34.1 8.0 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 J014707.47+570028.9,2461188.8618,8.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J014707.47+570028.9 20260528.3618 8.02CV 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 05 28.3618 2461188.8618 9.47 01:47:21.78 +58:08:40.5
130.27519 -3.92758 galactic Cas Second-epoch detections are separated by 4.5" and 7.6 pix
The object was found in VSX 3" NSVS 1763417
Type: SR
# Max. Min./Amp. JD0 Period
13.097 r Y 0.475 r 2458312.13540 289.666941400000 M7:
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:21.78 +58:08:40.5: 12.30 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:21.78 +58:08:40.5: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 05 28.3618* 01 47 21.78 +58 08 40.5 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1763417,2461188.8618,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1763417 20260528.3618 9.47CV 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 05 28.3618 2461188.8618 8.06 01:39:46.89 +59:42:30.5
129.00047 -2.59245 galactic Cas Second-epoch detections are separated by 1.2" and 7.4 pix
The object was found in VSX 1" V0911 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
12.100 V 13.000 V M4
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:46.89 +59:42:30.5: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:46.89 +59:42:30.5: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 39 46.89 +59 42 30.5 8.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0911 Cas,2461188.8618,8.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0911 Cas 20260528.3618 8.06CV 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 05 28.3618 2461188.8618 9.07 01:44:48.84 +59:53:34.1
129.58542 -2.28763 galactic Cas Second-epoch detections are separated by 1.4" and 7.7 pix
The object was found in VSX 1" ASASSN-V J014448.76+595333.5
Type: SR
# Max. Min./Amp. JD0 Period
13.130 V 13.330 V 2458098.00000 300.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:48.84 +59:53:34.1: 12.98 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:48.84 +59:53:34.1: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 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 05 28.3618* 01 44 48.84 +59 53 34.1 9.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014448.76+595333.5,2461188.8618,9.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J014448.76+595333.5 20260528.3618 9.07CV 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 05 28.3618 2461188.8618 9.13 01:04:58.46 +60:30:20.5
124.59867 -2.32224 galactic Cas Second-epoch detections are separated by 0.8" and 8.1 pix
The object was found in VSX 2" V0454 Cas
Type: LB:
# Max. Min./Amp. JD0 Period
15.000 pg 16.000 pg
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:04:58.46 +60:30:20.5: 11.61 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:04:58.46 +60:30:20.5: 12.85 +/- 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 05 28.3618* 01 04 58.46 +60 30 20.5 9.1 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
V0454 Cas,2461188.8618,9.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0454 Cas 20260528.3618 9.13CV 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 05 28.3618 2461188.8618 9.07 01:09:49.42 +65:08:28.8
124.86408 2.33858 galactic Cas Second-epoch detections are separated by 1.8" and 7.8 pix
The object was found in VSX 1" NSVS J0109489+650828
Type: SR
# Max. Min./Amp. JD0 Period
15.535 g Y 0.494 g 2458443.71020 168.437245800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:49.42 +65:08:28.8: 12.62 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:49.42 +65:08:28.8: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 05 28.3618* 01 09 49.42 +65 08 28.8 9.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0109489+650828,2461188.8618,9.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0109489+650828 20260528.3618 9.07CV 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 05 28.3618 2461188.8618 8.78 02:22:32.05 +64:22:11.7
132.58648 3.21931 galactic Cas Second-epoch detections are separated by 0.0" and 7.0 pix
The object was found in VSX 1" ASASSN-V J022232.03+642212.7
Type: L
# Max. Min./Amp. JD0 Period
13.010 V 13.290 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:32.05 +64:22:11.7: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:32.05 +64:22:11.7: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 22 32.05 +64 22 11.7 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
ASASSN-V J022232.03+642212.7,2461188.8618,8.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022232.03+642212.7 20260528.3618 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 05 28.3618 2461188.8618 9.88 01:11:51.39 +58:59:24.6
125.56492 -3.77716 galactic Cas Second-epoch detections are separated by 2.0" and 7.7 pix
The object was found in VSX 2" ASASSN-V J011151.17+585923.3
Type: SR
# Max. Min./Amp. JD0 Period
13.990 V 14.310 V 2458378.86210 49.038099800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:51.39 +58:59:24.6: 12.97 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:51.39 +58:59:24.6: 13.55 +/- 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 05 28.3618* 01 11 51.39 +58 59 24.6 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J011151.17+585923.3,2461188.8618,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011151.17+585923.3 20260528.3618 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.36 02:18:24.73 +58:37:25.8
134.06224 -2.35572 galactic Per Second-epoch detections are separated by 2.8" and 6.8 pix
The object was found in VSX 1" TSVSC1 TN-N311132011-556-86-2
Type: SR
# Max. Min./Amp. JD0 Period
13.035 r Y 0.802 r 2458469.04980 210.487596000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:24.73 +58:37:25.8: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:24.73 +58:37:25.8: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 18 24.73 +58 37 25.8 9.4 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
TSVSC1 TN-N311132011-556-86-2,2461188.8618,9.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TSVSC1 TN-N311132011-556-86-2 20260528.3618 9.36CV 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 05 28.3618 2461188.8618 9.56 01:57:53.16 +63:48:41.1
130.18421 1.87924 galactic Cas Second-epoch detections are separated by 1.7" and 7.4 pix
The object was found in VSX 5" ASASSN-V J015753.42+634846.1
Type: SR
# Max. Min./Amp. JD0 Period
13.590 V 13.970 V 2458299.91990 150.638151100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:53.16 +63:48:41.1: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:53.16 +63:48:41.1: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 57 53.16 +63 48 41.1 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J015753.42+634846.1,2461188.8618,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015753.42+634846.1 20260528.3618 9.56CV 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 05 28.3618 2461188.8618 9.69 02:12:24.62 +63:16:01.2
131.89060 1.81237 galactic Cas Second-epoch detections are separated by 1.2" and 6.9 pix
The object was found in VSX 2" NSVS 1829376
Type: SR
# Max. Min./Amp. JD0 Period
13.292 r Y 0.485 r 2458421.47120 181.452212200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:12:24.62 +63:16:01.2: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:12:24.62 +63:16:01.2: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 05 28.3618* 02 12 24.62 +63 16 01.2 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1829376,2461188.8618,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1829376 20260528.3618 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.21 02:42:10.42 +61:03:22.2
135.92751 1.00981 galactic Cas Second-epoch detections are separated by 1.1" and 7.0 pix
The object was found in VSX 3" NSVS 1880787
Type: L
# Max. Min./Amp. JD0 Period
10.450 R1 10.650 R1
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:42:10.42 +61:03:22.2: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:42:10.42 +61:03:22.2: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 42 10.42 +61 03 22.2 8.2 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
NSVS 1880787,2461188.8618,8.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1880787 20260528.3618 8.21CV 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 05 28.3618 2461188.8618 8.31 02:19:34.19 +58:23:57.9
134.27955 -2.51720 galactic Per Second-epoch detections are separated by 0.2" and 7.3 pix
The object was found in VSX 2" NSVS 1909158
Type: SR
# Max. Min./Amp. JD0 Period
14.589 g Y 0.328 g 2458495.63840 62.731476600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:34.19 +58:23:57.9: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:34.19 +58:23:57.9: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 05 28.3618* 02 19 34.19 +58 23 57.9 8.3 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
NSVS 1909158,2461188.8618,8.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1909158 20260528.3618 8.31CV 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 05 28.3618 2461188.8618 9.98 01:01:19.84 +58:00:01.2
124.24690 -4.84615 galactic Cas Second-epoch detections are separated by 0.4" and 8.3 pix
The object was found in VSX 3" NSVS 1724224
Type: SR
# Max. Min./Amp. JD0 Period
13.713 r Y 0.550 R1 2458387.94790 203.067280800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:01:19.84 +58:00:01.2: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:01:19.84 +58:00:01.2: 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 05 28.3618* 01 01 19.84 +58 00 01.2 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1724224,2461188.8618,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1724224 20260528.3618 9.98CV 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 05 28.3618 2461188.8618 8.21 01:16:04.83 +58:33:49.3
126.14895 -4.15404 galactic Cas Second-epoch detections are separated by 0.8" and 8.1 pix
The object was found in VSX 1" ASASSN-V J011604.72+583348.5
Type: SR
# Max. Min./Amp. JD0 Period
13.410 g Y 0.635 g 2458509.58130 80.686544600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:04.83 +58:33:49.3: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:04.83 +58:33:49.3: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 16 04.83 +58 33 49.3 8.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J011604.72+583348.5,2461188.8618,8.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011604.72+583348.5 20260528.3618 8.21CV 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 05 28.3618 2461188.8618 9.10 01:24:30.64 +59:38:48.6
127.10482 -2.95669 galactic Cas Second-epoch detections are separated by 1.1" and 8.0 pix
The object was found in VSX 1" ASASSN-V J012430.51+593847.9
Type: SR
# Max. Min./Amp. JD0 Period
13.360 V 13.950 V 2458378.66340 139.847766200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:30.64 +59:38:48.6: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:30.64 +59:38:48.6: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 24 30.64 +59 38 48.6 9.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J012430.51+593847.9,2461188.8618,9.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J012430.51+593847.9 20260528.3618 9.10CV 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 05 28.3618 2461188.8618 9.02 02:00:17.58 +57:43:39.7
132.04507 -3.92063 galactic Per Second-epoch detections are separated by 8.0" and 6.5 pix
The object was found in VSX 5" ASASSN-V J020018.03+574337.1
Type: SR
# Max. Min./Amp. JD0 Period
13.250 V 13.770 V 2458556.53250 49.147314800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:17.58 +57:43:39.7: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:17.58 +57:43:39.7: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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 05 28.3618* 02 00 17.58 +57 43 39.7 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J020018.03+574337.1,2461188.8618,9.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020018.03+574337.1 20260528.3618 9.02CV 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 05 28.3618 2461188.8618 6.83 01:17:41.64 +59:18:24.2
126.28293 -3.39409 galactic Cas Second-epoch detections are separated by 0.4" and 7.9 pix
The object was found in VSX 2" BQ Cas
Type: LB
# Max. Min./Amp. JD0 Period
13.500 pg 14.400 pg 275.000000000000 : M6.5
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:41.64 +59:18:24.2: 11.93 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:41.64 +59:18:24.2: 10.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.52 +/- 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 05 28.3618* 01 17 41.64 +59 18 24.2 6.8 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
BQ Cas,2461188.8618,6.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BQ Cas 20260528.3618 6.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.04 02:13:08.99 +63:06:22.8
132.01967 1.68540 galactic Cas Second-epoch detections are separated by 1.4" and 6.9 pix
The object was found in VSX 1" ASASSN-V J021308.99+630623.7
Type: L:
# Max. Min./Amp. JD0 Period
13.290 V 13.540 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:08.99 +63:06:22.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:08.99 +63:06:22.8: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 13 08.99 +63 06 22.8 9.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J021308.99+630623.7,2461188.8618,9.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021308.99+630623.7 20260528.3618 9.04CV 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 05 28.3618 2461188.8618 9.38 02:07:16.67 +60:08:10.8
132.24500 -1.35693 galactic Cas Second-epoch detections are separated by 0.9" and 7.3 pix
The object was found in VSX 2" ASASSN-V J020716.81+600809.8
Type: SR
# Max. Min./Amp. JD0 Period
14.850 g Y 0.810 g 2459552.87600 444.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:16.67 +60:08:10.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:16.67 +60:08:10.8: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 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 05 28.3618* 02 07 16.67 +60 08 10.8 9.4 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
ASASSN-V J020716.81+600809.8,2461188.8618,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020716.81+600809.8 20260528.3618 9.38CV 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 05 28.3618 2461188.8618 8.35 02:33:40.04 +57:40:02.5
136.28552 -2.52954 galactic Per Second-epoch detections are separated by 0.7" 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 J038.4074+57.6734 | 02:33:40.23 +57:40:02.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.238+/-0.026 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:40.04 +57:40:02.5: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:40.04 +57:40:02.5: 10.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.78 +/- 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 05 28.3618* 02 33 40.04 +57 40 02.5 8.3 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 J038.4074+57.6734,2461188.8618,8.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.4074+57.6734 20260528.3618 8.35CV 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 05 28.3618 2461188.8618 9.40 01:30:50.42 +60:32:14.2
127.76173 -1.96444 galactic Cas Second-epoch detections are separated by 1.8" and 7.6 pix
The object was found in VSX 1" NSVS J0130502+603215
Type: SR
# Max. Min./Amp. JD0 Period
15.151 g Y 0.873 g 2458510.15640 105.353214200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:50.42 +60:32:14.2: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:50.42 +60:32:14.2: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 30 50.42 +60 32 14.2 9.4 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
NSVS J0130502+603215,2461188.8618,9.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0130502+603215 20260528.3618 9.40CV 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 05 28.3618 2461188.8618 9.65 01:09:38.03 +59:05:13.6
125.27196 -3.70194 galactic Cas Second-epoch detections are separated by 4.0" and 8.7 pix
The object was found in VSX 1" NSVS 1731355
Type: SR
# Max. Min./Amp. JD0 Period
13.050 r Y 0.760 r 2458523.08150 271.469883000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:38.03 +59:05:13.6: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:38.03 +59:05:13.6: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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 05 28.3618* 01 09 38.03 +59 05 13.6 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1731355,2461188.8618,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1731355 20260528.3618 9.65CV 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 05 28.3618 2461188.8618 6.71 02:27:23.77 +60:40:47.8
134.41581 -0.03431 galactic Cas Second-epoch detections are separated by 1.3" and 7.2 pix
The object was found in VSX 2" V0703 Cas
Type: LC
# Max. Min./Amp. JD0 Period
10.770 V 12.520 V M2Iab
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:23.77 +60:40:47.8: 12.76 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:23.77 +60:40:47.8: 10.32 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.32 +/- 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 05 28.3618* 02 27 23.77 +60 40 47.8 6.7 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
V0703 Cas,2461188.8618,6.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0703 Cas 20260528.3618 6.71CV 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 05 28.3618 2461188.8618 6.53 01:54:28.56 +57:17:51.0
131.39663 -4.53459 galactic Per Second-epoch detections are separated by 1.0" and 7.6 pix
The object was found in VSX 2" NSVS 1769612
Type: L
# Max. Min./Amp. JD0 Period
8.700 R1 9.100 R1
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:28.56 +57:17:51.0: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:28.56 +57:17:51.0: 10.32 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.32 +/- 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 05 28.3618* 01 54 28.56 +57 17 51.0 6.5 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
NSVS 1769612,2461188.8618,6.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1769612 20260528.3618 6.53CV 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 05 28.3618 2461188.8618 9.85 01:23:02.01 +61:59:41.5
126.63192 -0.64969 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 | Gaia DR3 510939209439852544 | 01:23:01.88 +61:59:40.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: S 1954ApJ...120..478N CSS 30 J-Ks=2.365+/-0.317 (Very red!)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:02.01 +61:59:41.5: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:02.01 +61:59:41.5: 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 05 28.3618* 01 23 02.01 +61 59 41.5 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510939209439852544,2461188.8618,9.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510939209439852544 20260528.3618 9.85CV 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 05 28.3618 2461188.8618 9.80 01:14:57.02 +59:42:13.2
125.89753 -3.03263 galactic Cas Second-epoch detections are separated by 2.4" and 8.2 pix
The object was found in VSX 2" NSVS J0114566+594210
Type: SR
# Max. Min./Amp. JD0 Period
13.340 r Y 0.273 r 2458345.86300 105.806803300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:57.02 +59:42:13.2: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:57.02 +59:42:13.2: 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 05 28.3618* 01 14 57.02 +59 42 13.2 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0114566+594210,2461188.8618,9.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0114566+594210 20260528.3618 9.80CV 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 05 28.3618 2461188.8618 9.70 01:49:47.69 +65:03:21.3
129.03765 2.87825 galactic Cas Second-epoch detections are separated by 1.0" and 7.5 pix
The object was found in VSX 0" ASASSN-V J014947.64+650321.4
Type: SR
# Max. Min./Amp. JD0 Period
14.000 V 15.100 V 2458390.66790 121.379022800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:47.69 +65:03:21.3: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:47.69 +65:03:21.3: 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 05 28.3618* 01 49 47.69 +65 03 21.3 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014947.64+650321.4,2461188.8618,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J014947.64+650321.4 20260528.3618 9.70CV 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 05 28.3618 2461188.8618 8.08 01:18:52.86 +58:09:31.4
126.55648 -4.51976 galactic Cas Second-epoch detections are separated by 0.3" and 7.9 pix
The object was found in VSX 1" V0645 Cas
Type: SRA
# Max. Min./Amp. JD0 Period
12.200 V 13.100 V 2441900.00000 425.000000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:52.86 +58:09:31.4: 12.77 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:52.86 +58:09:31.4: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 18 52.86 +58 09 31.4 8.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0645 Cas,2461188.8618,8.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0645 Cas 20260528.3618 8.08CV 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 05 28.3618 2461188.8618 6.48 02:08:15.60 +59:15:57.1
132.61709 -2.15364 galactic Cas Second-epoch detections are separated by 0.2" and 7.3 pix
The object was found in VSX 2" V0927 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
10.900 V 11.800 V M7
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:08:15.60 +59:15:57.1: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:08:15.60 +59:15:57.1: 10.25 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.25 +/- 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 05 28.3618* 02 08 15.60 +59 15 57.1 6.5 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
V0927 Cas,2461188.8618,6.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0927 Cas 20260528.3618 6.48CV 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 05 28.3618 2461188.8618 9.50 02:27:21.83 +62:38:26.5
133.70264 1.79219 galactic Cas Second-epoch detections are separated by 0.5" and 6.9 pix
The object was found in VSX 2" V0937 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
13.700 V 14.500 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:21.83 +62:38:26.5: 11.15 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:21.83 +62:38:26.5: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.67 +/- 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 05 28.3618* 02 27 21.83 +62 38 26.5 9.5 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
V0937 Cas,2461188.8618,9.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0937 Cas 20260528.3618 9.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.99 02:14:46.56 +57:37:03.4
133.93336 -3.46313 galactic Per Second-epoch detections are separated by 1.3" and 7.2 pix
The object was found in VSX 2" ASASSN-V J021446.65+573702.0
Type: L
# Max. Min./Amp. JD0 Period
13.070 V 13.650 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:46.56 +57:37:03.4: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:14:46.56 +57:37:03.4: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 14 46.56 +57 37 03.4 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J021446.65+573702.0,2461188.8618,8.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021446.65+573702.0 20260528.3618 8.99CV 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 05 28.3618 2461188.8618 7.38 02:34:06.44 +56:37:23.7
136.74347 -3.47007 galactic Per 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 457763322428148096 | 02:34:05.91 +56:37:27.7 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:06.44 +56:37:23.7: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:06.44 +56:37:23.7: 9.61 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.61 +/- 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 05 28.3618* 02 34 06.44 +56 37 23.7 7.4 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 457763322428148096,2461188.8618,7.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457763322428148096 20260528.3618 7.38CV 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 05 28.3618 2461188.8618 9.63 01:10:29.41 +57:08:53.0
125.52615 -5.62769 galactic Cas Second-epoch detections are separated by 1.1" and 8.0 pix
The object was found in VSX 4" NSVS J0110292+570849
Type: L:
# Max. Min./Amp. JD0 Period
11.576 R1 Y 0.714 R1 120.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:29.41 +57:08:53.0: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:29.41 +57:08:53.0: 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 05 28.3618* 01 10 29.41 +57 08 53.0 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0110292+570849,2461188.8618,9.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0110292+570849 20260528.3618 9.63CV 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 05 28.3618 2461188.8618 9.28 01:01:55.32 +59:00:14.3
124.28438 -3.84024 galactic Cas Second-epoch detections are separated by 0.9" and 8.1 pix
The object was found in VSX 4" ASASSN-V J010154.82+590013.9
Type: SR
# Max. Min./Amp. JD0 Period
15.747 g Y 0.376 g 2458410.99490 279.414821500000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:01:55.32 +59:00:14.3: 11.95 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:01:55.32 +59:00:14.3: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 05 28.3618* 01 01 55.32 +59 00 14.3 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J010154.82+590013.9,2461188.8618,9.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010154.82+590013.9 20260528.3618 9.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 10.06 01:21:36.46 +63:33:51.0
126.28240 0.88885 galactic Cas Second-epoch detections are separated by 1.3" and 7.7 pix
The object was found in VSX 1" NSVS 1692766
Type: SR
# Max. Min./Amp. JD0 Period
13.414 r Y 0.380 r 2458570.63480 356.621563700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:36.46 +63:33:51.0: 12.75 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:36.46 +63:33:51.0: 14.16 +/- 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 05 28.3618* 01 21 36.46 +63 33 51.0 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
NSVS 1692766,2461188.8618,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1692766 20260528.3618 10.06CV 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 05 28.3618 2461188.8618 9.03 01:23:21.85 +60:18:14.4
126.87956 -2.32281 galactic Cas Second-epoch detections are separated by 1.8" and 7.8 pix
The object was found in ASASSN-V 3" 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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:21.85 +60:18:14.4: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:21.85 +60:18:14.4: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 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 05 28.3618* 01 23 21.85 +60 18 14.4 9.0 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
VARIABLE_NAME,2461188.8618,9.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3618 9.03CV 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 05 28.3618 2461188.8618 9.48 02:23:18.51 +64:21:47.0
132.66754 3.24189 galactic Cas Second-epoch detections are separated by 2.2" and 6.7 pix
The object was found in VSX 1" ASASSN-V J022318.63+642146.2
Type: SR
# Max. Min./Amp. JD0 Period
14.150 V 14.710 V 2458362.83350 282.186156800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:18.51 +64:21:47.0: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:18.51 +64:21:47.0: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 23 18.51 +64 21 47.0 9.5 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 J022318.63+642146.2,2461188.8618,9.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022318.63+642146.2 20260528.3618 9.48CV 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 05 28.3618 2461188.8618 9.51 02:21:20.02 +61:23:53.5
133.47652 0.38055 galactic Cas Second-epoch detections are separated by 2.6" and 7.5 pix
The object was found in VSX 2" NSVS 1836971
Type: SR
# Max. Min./Amp. JD0 Period
13.572 r Y 0.349 r 2458494.57560 121.420963500000 CS:
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:20.02 +61:23:53.5: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:20.02 +61:23:53.5: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 21 20.02 +61 23 53.5 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1836971,2461188.8618,9.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1836971 20260528.3618 9.51CV 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 05 28.3618 2461188.8618 9.28 02:38:33.43 +61:54:31.0
135.18586 1.61247 galactic Cas Second-epoch detections are separated by 1.5" and 6.7 pix
The object was found in VSX 0" ASASSN-V J023833.47+615431.3
Type: L:
# Max. Min./Amp. JD0 Period
13.230 V 13.740 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:33.43 +61:54:31.0: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:33.43 +61:54:31.0: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 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 05 28.3618* 02 38 33.43 +61 54 31.0 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J023833.47+615431.3,2461188.8618,9.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J023833.47+615431.3 20260528.3618 9.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.71 01:20:18.43 +64:28:04.9
126.03747 1.77049 galactic Cas Second-epoch detections are separated by 1.3" and 7.6 pix
The object was found in VSX 2" V0898 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
12.800 V 13.800 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:18.43 +64:28:04.9: 10.39 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:18.43 +64:28:04.9: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 20 18.43 +64 28 04.9 8.7 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
V0898 Cas,2461188.8618,8.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0898 Cas 20260528.3618 8.71CV 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 05 28.3618 2461188.8618 9.73 01:36:43.18 +61:14:25.3
128.35240 -1.15392 galactic Cas Second-epoch detections are separated by 0.9" and 7.7 pix
The object was found in VSX 1" ASASSN-V J013643.22+611426.0
Type: L
# Max. Min./Amp. JD0 Period
13.880 V 14.350 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:43.18 +61:14:25.3: 12.89 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:43.18 +61:14:25.3: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 36 43.18 +61 14 25.3 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013643.22+611426.0,2461188.8618,9.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3618 9.73CV 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 05 28.3618 2461188.8618 9.69 02:00:13.56 +60:43:20.6
131.24678 -1.03405 galactic Cas Second-epoch detections are separated by 2.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 508045535357127552 | 02:00:13.69 +60:43:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.530+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:13.56 +60:43:20.6: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:13.56 +60:43:20.6: 13.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 05 28.3618* 02 00 13.56 +60 43 20.6 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508045535357127552,2461188.8618,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508045535357127552 20260528.3618 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.61 01:20:05.35 +59:00:13.2
126.62112 -3.66270 galactic Cas Second-epoch detections are separated by 2.8" and 8.0 pix
The object was found in VSX 1" ASASSN-V J012005.20+590012.5
Type: SR
# Max. Min./Amp. JD0 Period
14.850 g Y 0.490 g 2458417.86600 46.110000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:05.35 +59:00:13.2: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:05.35 +59:00:13.2: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 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 05 28.3618* 01 20 05.35 +59 00 13.2 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J012005.20+590012.5,2461188.8618,9.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J012005.20+590012.5 20260528.3618 9.61CV 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 05 28.3618 2461188.8618 9.23 00:58:01.37 +59:33:23.2
123.76735 -3.30462 galactic Cas Second-epoch detections are separated by 1.3" and 8.5 pix
The object was found in VSX 5" NSVS J0058007+593326
Type: L:
# Max. Min./Amp. JD0 Period
11.361 R1 Y 0.400 R1 70.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:58:01.37 +59:33:23.2: 11.62 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:58:01.37 +59:33:23.2: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 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 05 28.3618* 00 58 01.37 +59 33 23.2 9.2 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
NSVS J0058007+593326,2461188.8618,9.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0058007+593326 20260528.3618 9.23CV 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 05 28.3618 2461188.8618 9.82 01:51:45.69 +65:36:52.8
129.11000 3.46908 galactic Cas Second-epoch detections are separated by 2.1" and 7.1 pix
The object was found in VSX 2" ZTF J015145.40+653652.9
Type: SR
# Max. Min./Amp. JD0 Period
12.822 r Y 0.125 r 2458384.93560 45.688336700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:45.69 +65:36:52.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:45.69 +65:36:52.8: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 51 45.69 +65 36 52.8 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J015145.40+653652.9,2461188.8618,9.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015145.40+653652.9 20260528.3618 9.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.06 01:28:36.28 +61:12:06.7
127.39411 -1.34747 galactic Cas Second-epoch detections are separated by 0.7" and 7.6 pix
The object was found in VSX 1" PQ Cas
Type: SR
# Max. Min./Amp. JD0 Period
14.963 g Y 0.540 g 2458436.69130 77.771904400000 S
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:36.28 +61:12:06.7: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:36.28 +61:12:06.7: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 28 36.28 +61 12 06.7 9.1 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
PQ Cas,2461188.8618,9.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
PQ Cas 20260528.3618 9.06CV 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 05 28.3618 2461188.8618 9.24 02:02:39.14 +59:22:44.0
131.89853 -2.24741 galactic Cas Second-epoch detections are separated by 2.2" and 7.3 pix
The object was found in VSX 1" ASASSN-V J020239.29+592244.9
Type: SR
# Max. Min./Amp. JD0 Period
14.580 g Y 0.320 g 2458904.62800 100.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:39.14 +59:22:44.0: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:39.14 +59:22:44.0: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 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 05 28.3618* 02 02 39.14 +59 22 44.0 9.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J020239.29+592244.9,2461188.8618,9.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020239.29+592244.9 20260528.3618 9.24CV 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 05 28.3618 2461188.8618 8.07 02:03:00.34 +58:36:13.4
132.15424 -2.98069 galactic Cas Second-epoch detections are separated by 0.3" and 7.4 pix
The object was found in VSX 1" V0925 Cas
Type: SR
# Max. Min./Amp. JD0 Period
11.800 V 12.500 V 2458534.41920 125.392415100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:00.34 +58:36:13.4: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:00.34 +58:36:13.4: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 03 00.34 +58 36 13.4 8.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0925 Cas,2461188.8618,8.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0925 Cas 20260528.3618 8.07CV 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 05 28.3618 2461188.8618 8.84 01:31:04.89 +57:13:14.0
128.30126 -5.23732 galactic Cas Second-epoch detections are separated by 1.3" and 7.9 pix
The object was found in VSX 2" NSVS J0131044+571311
Type: SR
# Max. Min./Amp. JD0 Period
15.493 g Y 0.930 g 2458391.33620 157.055384600000 M7:
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:04.89 +57:13:14.0: 11.36 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:04.89 +57:13:14.0: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.81 +/- 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 05 28.3618* 01 31 04.89 +57 13 14.0 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
NSVS J0131044+571311,2461188.8618,8.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0131044+571311 20260528.3618 8.84CV 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 05 28.3618 2461188.8618 9.96 01:04:09.24 +61:46:55.9
124.43469 -1.05245 galactic Cas Second-epoch detections are separated by 0.8" and 8.0 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 522740405182260480 | 01:04:09.16 +61:46:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:04:09.24 +61:46:55.9: 11.31 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:04:09.24 +61:46:55.9: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.79 +/- 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 05 28.3618* 01 04 09.24 +61 46 55.9 10.0 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 522740405182260480,2461188.8618,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522740405182260480 20260528.3618 9.96CV 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 05 28.3618 2461188.8618 10.07 01:32:44.39 +61:45:35.6
127.79743 -0.72107 galactic Cas Second-epoch detections are separated by 1.0" and 7.7 pix
The object was found in VSX 0" NSVS 1803986
Type: SR
# Max. Min./Amp. JD0 Period
12.100 R1 12.400 R1 2451468.00000 92.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:44.39 +61:45:35.6: 11.51 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:44.39 +61:45:35.6: 14.05 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 05 28.3618* 01 32 44.39 +61 45 35.6 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
NSVS 1803986,2461188.8618,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1803986 20260528.3618 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 7.64 02:37:50.65 +57:54:15.4
136.70529 -2.09358 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 | Gaia DR3 457950376842758784 | 02:37:50.90 +57:54:16.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +57 74 J-Ks=0.095+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:50.65 +57:54:15.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:50.65 +57:54:15.4: 9.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.96 +/- 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 05 28.3618* 02 37 50.65 +57 54 15.4 7.6 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 457950376842758784,2461188.8618,7.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457950376842758784 20260528.3618 7.64CV 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 05 28.3618 2461188.8618 8.54 02:32:40.32 +62:07:15.6
134.46712 1.53807 galactic Cas Second-epoch detections are separated by 0.7" and 7.0 pix
The object was found in VSX 3" NSVS J0232406+620718
Type: L:
# Max. Min./Amp. JD0 Period
10.285 R1 Y 0.457 R1 207.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:40.32 +62:07:15.6: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:40.32 +62:07:15.6: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 32 40.32 +62 07 15.6 8.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0232406+620718,2461188.8618,8.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0232406+620718 20260528.3618 8.54CV 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 05 28.3618 2461188.8618 8.75 02:03:07.41 +57:18:14.7
132.52636 -4.22623 galactic Per Second-epoch detections are separated by 1.5" and 7.4 pix
The object was found in VSX 2" ASASSN-V J020307.46+571813.2
Type: SR
# Max. Min./Amp. JD0 Period
13.470 V 13.900 V 2458312.63550 148.824620900000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:07.41 +57:18:14.7: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:07.41 +57:18:14.7: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 05 28.3618* 02 03 07.41 +57 18 14.7 8.8 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 J020307.46+571813.2,2461188.8618,8.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020307.46+571813.2 20260528.3618 8.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 6.11 02:19:36.15 +64:09:18.0
132.35983 2.90905 galactic Cas Second-epoch detections are separated by 0.2" and 7.0 pix
The object was found in VSX 1" NSV 783
Type:
# Max. Min./Amp. JD0 Period
6.400 I 6.720 I M5
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:36.15 +64:09:18.0: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:36.15 +64:09:18.0: 9.74 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.74 +/- 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 05 28.3618* 02 19 36.15 +64 09 18.0 6.1 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
NSV 783,2461188.8618,6.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 783 20260528.3618 6.11CV 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 05 28.3618 2461188.8618 8.47 02:31:46.25 +55:57:57.3
136.69510 -4.20138 galactic Per Second-epoch detections are separated by 6.5" 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 | ATO J037.9520+55.9630 | 02:31:46.12 +55:57:58.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.866+/-0.036 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:46.25 +55:57:57.3: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:46.25 +55:57:57.3: 10.94 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.94 +/- 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 05 28.3618* 02 31 46.25 +55 57 57.3 8.5 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 J037.9520+55.9630,2461188.8618,8.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.9520+55.9630 20260528.3618 8.47CV 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 05 28.3618 2461188.8618 9.47 00:41:52.39 +59:10:02.9
121.70409 -3.68147 galactic Cas Second-epoch detections are separated by 0.8" and 8.4 pix
The object was found in VSX 7" NSVS J0041521+590958
Type: SR
# Max. Min./Amp. JD0 Period
13.312 r Y 0.450 r 2458478.54780 283.542164100000 M7
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:41:52.39 +59:10:02.9: 11.30 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:41:52.39 +59:10:02.9: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 05 28.3618* 00 41 52.39 +59 10 02.9 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0041521+590958,2461188.8618,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0041521+590958 20260528.3618 9.47CV 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 05 28.3618 2461188.8618 8.12 02:33:23.67 +64:25:00.1
133.66401 3.69056 galactic Cas Second-epoch detections are separated by 0.7" and 6.6 pix
The object was found in VSX 2" V0940 Cas
Type: SR
# Max. Min./Amp. JD0 Period
13.300 V 14.100 V 2458188.78170 420.688461000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:23.67 +64:25:00.1: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:23.67 +64:25:00.1: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 33 23.67 +64 25 00.1 8.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0940 Cas,2461188.8618,8.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0940 Cas 20260528.3618 8.12CV 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 05 28.3618 2461188.8618 9.11 01:52:19.54 +57:19:07.3
131.10868 -4.58324 galactic Per Second-epoch detections are separated by 1.6" and 7.6 pix
The object was found in VSX 2" BX Per
Type: LB
# Max. Min./Amp. JD0 Period
14.400 pg 15.000 pg M6
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:19.54 +57:19:07.3: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:19.54 +57:19:07.3: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 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 05 28.3618* 01 52 19.54 +57 19 07.3 9.1 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
BX Per,2461188.8618,9.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BX Per 20260528.3618 9.11CV 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 05 28.3618 2461188.8618 9.34 01:41:34.22 +56:56:31.6
129.75903 -5.26363 galactic Cas Second-epoch detections are separated by 1.8" and 7.6 pix
The object was found in VSX 7" ASASSN-V J014134.49+565625.6
Type: SR
# Max. Min./Amp. JD0 Period
14.230 V 14.790 V 2458303.15380 380.445432700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:34.22 +56:56:31.6: 11.89 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:34.22 +56:56:31.6: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 05 28.3618* 01 41 34.22 +56 56 31.6 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014134.49+565625.6,2461188.8618,9.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J014134.49+565625.6 20260528.3618 9.34CV 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 05 28.3618 2461188.8618 9.01 02:31:18.98 +56:20:50.6
136.49202 -3.87201 galactic Per Second-epoch detections are separated by 3.3" 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 457386739697519488 | 02:31:19.13 +56:20:48.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.854+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:18.98 +56:20:50.6: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:18.98 +56:20:50.6: 11.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 31 18.98 +56 20 50.6 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457386739697519488,2461188.8618,9.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457386739697519488 20260528.3618 9.01CV 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 05 28.3618 2461188.8618 9.51 02:24:19.74 +63:24:35.5
133.10646 2.38807 galactic Cas Second-epoch detections are separated by 6.0" and 7.5 pix
The object was found in VSX 2" NSVS 1836899
Type: SR
# Max. Min./Amp. JD0 Period
14.940 g Y 0.207 g 2458298.04330 84.697770600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:19.74 +63:24:35.5: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:19.74 +63:24:35.5: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 24 19.74 +63 24 35.5 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1836899,2461188.8618,9.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1836899 20260528.3618 9.51CV 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 05 28.3618 2461188.8618 9.01 02:43:55.93 +64:48:54.7
134.53972 4.50970 galactic Cas Second-epoch detections are separated by 1.8" and 7.0 pix
The object was found in VSX 4" ASASSN-V J024356.44+644856.8
Type: SRS
# Max. Min./Amp. JD0 Period
13.380 V 13.620 V 2457415.70000 25.170000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:43:55.93 +64:48:54.7: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:43:55.93 +64:48:54.7: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 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 05 28.3618* 02 43 55.93 +64 48 54.7 9.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J024356.44+644856.8,2461188.8618,9.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J024356.44+644856.8 20260528.3618 9.01CV 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 05 28.3618 2461188.8618 9.46 01:45:16.05 +57:55:46.8
130.04906 -4.19631 galactic Cas Second-epoch detections are separated by 1.8" and 7.9 pix
The object was found in VSX 0" ASASSN-V J014516.03+575546.6
Type: SR
# Max. Min./Amp. JD0 Period
14.913 g Y 1.157 g 2458341.54630 111.087059600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:16.05 +57:55:46.8: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:16.05 +57:55:46.8: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 45 16.05 +57 55 46.8 9.5 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 J014516.03+575546.6,2461188.8618,9.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J014516.03+575546.6 20260528.3618 9.46CV 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 05 28.3618 2461188.8618 9.51 02:13:47.58 +63:11:26.0
132.06242 1.78807 galactic Cas Second-epoch detections are separated by 2.7" and 7.3 pix
The object was found in VSX 2" NSVS J0213478+631127
Type: L:
# Max. Min./Amp. JD0 Period
11.122 R1 Y 0.644 R1 355.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:47.58 +63:11:26.0: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:47.58 +63:11:26.0: 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 05 28.3618* 02 13 47.58 +63 11 26.0 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0213478+631127,2461188.8618,9.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0213478+631127 20260528.3618 9.51CV 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 05 28.3618 2461188.8618 7.77 02:19:59.14 +59:17:32.1
134.03110 -1.65790 galactic Cas Second-epoch detections are separated by 0.7" and 7.3 pix
The object was found in VSX 3" ASASSN-V J021959.04+591728.9
Type: SR
# Max. Min./Amp. JD0 Period
12.190 V 12.450 V 2458297.46040 162.355102800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:59.14 +59:17:32.1: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:59.14 +59:17:32.1: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 19 59.14 +59 17 32.1 7.8 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 J021959.04+591728.9,2461188.8618,7.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021959.04+591728.9 20260528.3618 7.77CV 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 05 28.3618 2461188.8618 5.52 01:56:16.77 +62:11:52.2
130.41363 0.27168 galactic Cas Second-epoch detections are separated by 0.1" and 7.3 pix
The object was found in VSX 9" Gaia DR3 508726133049293952
Type: L
# Max. Min./Amp. JD0 Period
17.860 G 17.980 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:16.77 +62:11:52.2: 11.76 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:16.77 +62:11:52.2: 9.29 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.29 +/- 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 05 28.3618* 01 56 16.77 +62 11 52.2 5.5 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 508726133049293952,2461188.8618,5.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508726133049293952 20260528.3618 5.52CV 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 05 28.3618 2461188.8618 8.48 01:02:09.20 +57:21:42.2
124.38297 -5.47983 galactic Cas Second-epoch detections are separated by 0.1" and 8.3 pix
The object was found in VSX 3" ASASSN-V J010208.89+572141.1
Type: SR
# Max. Min./Amp. JD0 Period
12.640 V 13.250 V 2457703.90000 114.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:09.20 +57:21:42.2: 12.34 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:09.20 +57:21:42.2: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 02 09.20 +57 21 42.2 8.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J010208.89+572141.1,2461188.8618,8.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010208.89+572141.1 20260528.3618 8.48CV 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 05 28.3618 2461188.8618 9.68 02:07:37.49 +62:22:07.0
131.63793 0.79163 galactic Cas Second-epoch detections are separated by 0.9" and 7.3 pix
The object was found in VSX 0" ASASSN-V J020737.47+622206.6
Type: SR
# Max. Min./Amp. JD0 Period
13.640 V 13.820 V 2458317.00000 487.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:37.49 +62:22:07.0: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:37.49 +62:22:07.0: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 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 05 28.3618* 02 07 37.49 +62 22 07.0 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J020737.47+622206.6,2461188.8618,9.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020737.47+622206.6 20260528.3618 9.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.98 02:07:21.55 +64:28:11.9
130.99952 2.79400 galactic Cas Second-epoch detections are separated by 1.7" and 7.3 pix
The object was found in VSX 2" ASASSN-V J020721.72+642813.5
Type: SR
# Max. Min./Amp. JD0 Period
13.950 V 14.600 V 2458359.55260 379.951148200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:21.55 +64:28:11.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:21.55 +64:28:11.9: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 07 21.55 +64 28 11.9 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J020721.72+642813.5,2461188.8618,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020721.72+642813.5 20260528.3618 9.98CV 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 05 28.3618 2461188.8618 9.86 01:23:28.70 +62:35:10.1
126.61041 -0.05655 galactic Cas Second-epoch detections are separated by 3.5" and 7.3 pix
The object was found in VSX 2" NSVS 1693673
Type: L
# Max. Min./Amp. JD0 Period
11.450 R1 11.700 R1
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:28.70 +62:35:10.1: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:28.70 +62:35:10.1: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 23 28.70 +62 35 10.1 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1693673,2461188.8618,9.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1693673 20260528.3618 9.86CV 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 05 28.3618 2461188.8618 8.39 02:16:28.46 +58:16:12.0
133.93803 -2.77294 galactic Per Second-epoch detections are separated by 1.4" and 7.2 pix
The object was found in VSX 1" NSV 765
Type: SR:
# Max. Min./Amp. JD0 Period
13.500 pg 15.000 pg M3
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:28.46 +58:16:12.0: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:28.46 +58:16:12.0: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 16 28.46 +58 16 12.0 8.4 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
NSV 765,2461188.8618,8.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 765 20260528.3618 8.39CV 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 05 28.3618 2461188.8618 5.35 01:46:05.47 +60:59:36.6
129.51059 -1.17824 galactic Cas Second-epoch detections are separated by 0.1" and 7.5 pix
The object was found in VSX 0" V0589 Cas
Type: LC
# Max. Min./Amp. JD0 Period
8.700 V 9.400 V M3Iab-Ib
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:05.47 +60:59:36.6: 10.55 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:05.47 +60:59:36.6: 8.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 8.97 +/- 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 05 28.3618* 01 46 05.47 +60 59 36.6 5.3 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
V0589 Cas,2461188.8618,5.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0589 Cas 20260528.3618 5.35CV 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 05 28.3618 2461188.8618 9.31 01:43:45.28 +58:23:45.8
129.75757 -3.78066 galactic Cas Second-epoch detections are separated by 1.2" and 7.7 pix
The object was found in VSX 1" ASASSN-V J014345.26+582344.7
Type: SR
# Max. Min./Amp. JD0 Period
13.860 V 14.440 V 2458355.00070 93.081983100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:45.28 +58:23:45.8: 13.31 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:45.28 +58:23:45.8: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 43 45.28 +58 23 45.8 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014345.26+582344.7,2461188.8618,9.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J014345.26+582344.7 20260528.3618 9.31CV 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 05 28.3618 2461188.8618 8.10 02:41:04.44 +62:17:31.5
135.29951 2.08239 galactic Cas Second-epoch detections are separated by 0.7" and 6.7 pix
The object was found in VSX 3" Gaia DR3 465996190622642816
Type: L
# Max. Min./Amp. JD0 Period
18.500 G 18.870 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:41:04.44 +62:17:31.5: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:41:04.44 +62:17:31.5: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 41 04.44 +62 17 31.5 8.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 465996190622642816,2461188.8618,8.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 465996190622642816 20260528.3618 8.10CV 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 05 28.3618 2461188.8618 9.58 01:35:57.20 +59:47:27.0
128.51088 -2.59785 galactic Cas Second-epoch detections are separated by 1.6" and 7.6 pix
The object was found in VSX 3" NSVS 1751621
Type: SR
# Max. Min./Amp. JD0 Period
13.544 r Y 0.700 R1 2458310.71820 267.909793200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:57.20 +59:47:27.0: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:57.20 +59:47:27.0: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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 05 28.3618* 01 35 57.20 +59 47 27.0 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1751621,2461188.8618,9.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1751621 20260528.3618 9.58CV 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 05 28.3618 2461188.8618 10.12 01:36:47.30 +63:02:42.6
128.04473 0.62449 galactic Cas Second-epoch detections are separated by 1.4" and 7.7 pix
The object was found in VSX 1" NSVS 1806131
Type: L
# Max. Min./Amp. JD0 Period
11.350 R1 11.800 R1
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:47.30 +63:02:42.6: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:47.30 +63:02:42.6: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 36 47.30 +63 02 42.6 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
NSVS 1806131,2461188.8618,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1806131 20260528.3618 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 8.11 01:37:01.41 +61:15:57.1
128.38390 -1.12241 galactic Cas Second-epoch detections are separated by 0.7" and 7.5 pix
The object was found in VSX 2" V0910 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
12.500 V 13.700 V 80.000000000000 :
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:01.41 +61:15:57.1: 12.16 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:01.41 +61:15:57.1: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 37 01.41 +61 15 57.1 8.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0910 Cas,2461188.8618,8.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0910 Cas 20260528.3618 8.11CV 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 05 28.3618 2461188.8618 7.78 02:43:44.79 +60:40:26.6
136.26066 0.74206 galactic Cas Second-epoch detections are separated by 2.1" and 6.8 pix
The object was found in VSX 3" ASASSN-V J024345.19+604024.9
Type: SR
# Max. Min./Amp. JD0 Period
12.280 V 12.780 V 2458438.22180 247.570678700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:43:44.79 +60:40:26.6: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:43:44.79 +60:40:26.6: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 43 44.79 +60 40 26.6 7.8 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 J024345.19+604024.9,2461188.8618,7.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J024345.19+604024.9 20260528.3618 7.78CV 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 05 28.3618 2461188.8618 10.09 01:13:09.77 +64:46:43.6
125.24482 2.00464 galactic Cas Second-epoch detections are separated by 0.3" and 7.8 pix
The object was found in VSX 1" NSVS 1687963
Type: SR
# Max. Min./Amp. JD0 Period
13.242 r Y 0.307 r 2458282.08260 63.013608400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:09.77 +64:46:43.6: 12.62 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:09.77 +64:46:43.6: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 13 09.77 +64 46 43.6 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
NSVS 1687963,2461188.8618,10.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1687963 20260528.3618 10.09CV 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 05 28.3618 2461188.8618 9.95 01:25:56.70 +62:14:49.4
126.93724 -0.35604 galactic Cas Second-epoch detections are separated by 4.3" and 7.7 pix
The object was found in VSX 0" GSC 04035-02300
Type: SR
# Max. Min./Amp. JD0 Period
11.100 R1 11.600 R1 2451545.00000 120.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:56.70 +62:14:49.4: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:56.70 +62:14:49.4: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.58 +/- 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 05 28.3618* 01 25 56.70 +62 14 49.4 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 04035-02300,2461188.8618,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 04035-02300 20260528.3618 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3618 2461188.8618 9.35 02:30:58.99 +62:56:15.2
133.97811 2.22058 galactic Cas Second-epoch detections are separated by 0.5" and 6.9 pix
The object was found in VSX 2" ASASSN-V J023059.14+625616.4
Type: SR
# Max. Min./Amp. JD0 Period
14.260 V 14.860 V 2458288.72730 254.943657400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:58.99 +62:56:15.2: 10.73 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:58.99 +62:56:15.2: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.05 +/- 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 05 28.3618* 02 30 58.99 +62 56 15.2 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J023059.14+625616.4,2461188.8618,9.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J023059.14+625616.4 20260528.3618 9.35CV 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 05 28.3618 2461188.8618 8.63 02:18:22.56 +58:47:09.8
134.00424 -2.20413 galactic Per Second-epoch detections are separated by 1.3" and 7.3 pix
The object was found in VSX 2" NSVS J0218236+584716
Type: SR
# Max. Min./Amp. JD0 Period
12.694 r Y 0.560 r 2458351.79460 241.646383300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:22.56 +58:47:09.8: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:22.56 +58:47:09.8: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 02 18 22.56 +58 47 09.8 8.6 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
NSVS J0218236+584716,2461188.8618,8.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J0218236+584716 20260528.3618 8.63CV 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 05 28.3618 2461188.8618 8.92 01:35:09.89 +60:17:10.6
128.32929 -2.12643 galactic Cas Second-epoch detections are separated by 1.2" and 7.5 pix
The object was found in VSX 1" Mis V0883
Type: L:
# Max. Min./Amp. JD0 Period
10.600 CR 11.500 CR 188.000000000000 S
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:09.89 +60:17:10.6: 13.07 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:09.89 +60:17:10.6: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 28.3618* 01 35 09.89 +60 17 10.6 8.9 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
Mis V0883,2461188.8618,8.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V0883 20260528.3618 8.92CV 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
## 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-Q1b1x1_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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461188.86216514 28.05.2026 08:41:21.068 /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 67
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 29499
Objects passed selection criteria: 29293
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 18803.5
Average stars matched: 18210 (96.8437 %)
Memory usage VmPeak: 132912 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 26 15:05:11 CDT 2026
VaST build number 1.0rc89-83-g49118af2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu May 28 03:44:55 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-Q1b1x1_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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461188.86216514 28.05.2026 08:41:21.068 /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 554
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 54 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): 200669
Objects passed selection criteria: 200013
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 128861
Average stars matched: 123956 (96.194 %)
Memory usage VmPeak: 1957316 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 26 15:05:11 CDT 2026
VaST build number 1.0rc89-83-g49118af2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu May 28 03:52:52 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
SExtractor catalog cache: saved Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q1b1x1_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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.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: 2461188.86142984
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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits'
wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q1b1x1_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-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
Image size: 942.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:52.902 +62:00:03.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:52.902 +62:00:03.17
Angular distance between the image centers 0.0499 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
Image size: 942.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:55.690 +61:59:22.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:55.690 +61:59:22.79
Angular distance between the image centers 0.0530 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:42:52.902 +62:00:03.17
Second-epoch second image center 01:42:55.690 +61:59:22.79
Angular distance between the image centers 0.01247 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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.rDyzUrlfr5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_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-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.MSWDqwYRxw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_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_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits &> /tmp/tmp.tEks5XwfO2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits &> /tmp/tmp.A657ISr0K2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q1b1x1_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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.937800
a=0.000000 b=1.000000 c=22.937800
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.30
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.30
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-Q1b1x1_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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=5.9)
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-Q1b1x1_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-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 63 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
4.4 pix fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
4.3 pix fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
2.2 pix wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.3 mag. Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
12.8 mag. fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
12.9 mag. fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 10.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.rDyzUrlfr5 (6) ############
Parsing command line arguments...
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_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q1b1x1_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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, passed=31559
Got 31559 stars (including 27744 good ones) from the SExtractor catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 31559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 280 matched stars entering correct_measured_positions(), 228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 267 matched stars entering correct_measured_positions(), 10048 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 403 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 336 matched stars entering correct_measured_positions(), 10093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.75"
Excluding outliers - 331 stars left (next iteration limit 293)
WCS_QUALITY_DIAG: file=Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=331 sigma_overall_arcsec=7.291 sigma_q1_arcsec=27.811 sigma_q2_arcsec=12.006 sigma_q3_arcsec=24.661 sigma_q4_arcsec=4.199 n_q1=15 n_q2=98 n_q3=37 n_q4=181 worst_quadrant_to_overall_ratio=3.814
The image catalog is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MSWDqwYRxw (6) ############
Parsing command line arguments...
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_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q1b1x1_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-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, passed=31681
Got 31681 stars (including 27947 good ones) from the SExtractor catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 31681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=973 sigma_overall_arcsec=0.406 sigma_q1_arcsec=0.531 sigma_q2_arcsec=0.401 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.344 n_q1=119 n_q2=244 n_q3=303 n_q4=307 worst_quadrant_to_overall_ratio=1.308
The image catalog is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.tEks5XwfO2 (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_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.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_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=277, passed=6189
Got 6189 stars (including 5911 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits.cat
util/solve_plate_with_UCAC5 got 6189 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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 729 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 6052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 6053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 6053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits N_match=962 sigma_overall_arcsec=0.541 sigma_q1_arcsec=0.605 sigma_q2_arcsec=0.665 sigma_q3_arcsec=0.416 sigma_q4_arcsec=0.623 n_q1=291 n_q2=231 n_q3=279 n_q4=161 worst_quadrant_to_overall_ratio=1.230
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits -region wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.A657ISr0K2 (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_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.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_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=260, passed=6240
Got 6240 stars (including 5977 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits.cat
util/solve_plate_with_UCAC5 got 6240 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 6112 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 6108 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 6101 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 959 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits N_match=959 sigma_overall_arcsec=0.523 sigma_q1_arcsec=0.541 sigma_q2_arcsec=0.548 sigma_q3_arcsec=0.435 sigma_q4_arcsec=0.591 n_q1=293 n_q2=231 n_q3=276 n_q4=159 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits -region wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=7.291 worst_q_ratio=3.814
ref2=Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=0.406 worst_q_ratio=1.308
new1=fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits sigma_overall=0.541 worst_q_ratio=1.230
new2=fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits sigma_overall=0.523 worst_q_ratio=1.130
reference average sigma_overall=3.8485 worst_q_ratio=2.561
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018_astrometric_residuals.png (331 matched stars from wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019_astrometric_residuals.png (973 matched stars from wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318_astrometric_residuals.png (962 matched stars from wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319_astrometric_residuals.png (959 matched stars from wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-40-17_20.00sec_-0.00C_LIGHTs_0318.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cas-03-Q1b1x1_034157_TTUQ1b1x1_2130603_bC1lTaT9/wcs_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319.fits'
Preparing the HTML report for the field Cas-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:18.15 +56:19:03.5: 13.25 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:03.52 +56:50:28.4: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:18.15 +56:19:03.5: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:33:18.15 +56:19:03.5: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:03.52 +56:50:28.4: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:31:03.52 +56:50:28.4: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:45.51 +55:56:55.3: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:27.65 +56:46:55.7: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:26.71 +56:41:40.1: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:49.89 +57:35:26.1: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:45.51 +55:56:55.3: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:30:45.51 +55:56:55.3: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:27.65 +56:46:55.7: 9.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.64 +/- 0.00
Forced photometry filter REJECTED candidate at 02:25:27.65 +56:46:55.7: ref_mag=9.64 +/- 0.00 new_mean_mag=9.5037 delta=0.14 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:09.01 +56:37:12.8: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:58.36 +56:02:39.0: 14.70 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:26.71 +56:41:40.1: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:32:26.71 +56:41:40.1: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:05.65 +56:39:57.4: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:49.89 +57:35:26.1: 9.32 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:38:49.89 +57:35:26.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:10.06 +56:27:14.2: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:30.83 +55:55:54.0: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:26.36 +55:59:07.5: 15.37 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:09.01 +56:37:12.8: 9.22 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:05.65 +56:39:57.4: 9.25 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.22 +/- 0.00
Forced photometry filter REJECTED candidate at 02:29:09.01 +56:37:12.8: ref_mag=9.22 +/- 0.00 new_mean_mag=9.6675 delta=-0.45 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:30.83 +55:55:54.0: 9.69 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:34:30.83 +55:55:54.0: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 9.25 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:58.36 +56:02:39.0: 9.39 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:32:05.65 +56:39:57.4: ref_mag=9.25 +/- 0.00 new_mean_mag=9.6554 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:10.06 +56:27:14.2: 9.57 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.39 +/- 0.00
Forced photometry filter REJECTED candidate at 02:27:58.36 +56:02:39.0: ref_mag=9.39 +/- 0.00 new_mean_mag=9.7699 delta=-0.38 (need > 0.90)
Forced photometry reference-image weighted average: 9.57 +/- 0.00
Forced photometry filter REJECTED candidate at 02:29:10.06 +56:27:14.2: ref_mag=9.57 +/- 0.00 new_mean_mag=9.8529 delta=-0.28 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:26.36 +55:59:07.5: 9.41 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.41 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:26.36 +55:59:07.5: ref_mag=9.41 +/- 0.00 new_mean_mag=9.8791 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:38.13 +57:29:11.2: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:11.09 +55:49:59.4: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:54.07 +56:14:28.5: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:18.20 +57:14:07.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:51.62 +57:23:37.1: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:26.21 +56:53:00.1: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:38.13 +57:29:11.2: 9.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.60 +/- 0.00
Forced photometry filter REJECTED candidate at 02:35:38.13 +57:29:11.2: ref_mag=9.60 +/- 0.00 new_mean_mag=9.9444 delta=-0.35 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:54.07 +56:14:28.5: 9.91 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:11.09 +55:49:59.4: 9.39 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:34:11.09 +55:49:59.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 9.91 +/- 0.00
Forced photometry filter REJECTED candidate at 02:30:54.07 +56:14:28.5: ref_mag=9.91 +/- 0.00 new_mean_mag=9.9217 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:24.34 +56:23:03.7: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:18.20 +57:14:07.2: 9.78 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:38:18.20 +57:14:07.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:51.62 +57:23:37.1: 9.51 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:38:51.62 +57:23:37.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:46.68 +56:48:23.0: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:26.21 +56:53:00.1: 9.61 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:37:26.21 +56:53:00.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:05.61 +57:22:04.2: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:24.34 +56:23:03.7: 9.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.59 +/- 0.00
Forced photometry filter REJECTED candidate at 02:27:24.34 +56:23:03.7: ref_mag=9.59 +/- 0.00 new_mean_mag=10.0480 delta=-0.46 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:46.68 +56:48:23.0: 9.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.54 +/- 0.00
Forced photometry filter REJECTED candidate at 02:32:46.68 +56:48:23.0: ref_mag=9.54 +/- 0.00 new_mean_mag=9.9832 delta=-0.45 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:05.61 +57:22:04.2: 10.19 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:35.25 +56:21:51.4: 15.65 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 10.19 +/- 0.00
Forced photometry filter REJECTED candidate at 02:32:05.61 +57:22:04.2: ref_mag=10.19 +/- 0.00 new_mean_mag=10.1230 delta=0.07 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:08.76 +57:25:19.3: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:35.25 +56:21:51.4: 9.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.58 +/- 0.00
Forced photometry filter REJECTED candidate at 02:34:35.25 +56:21:51.4: ref_mag=9.58 +/- 0.00 new_mean_mag=10.1295 delta=-0.55 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:08.76 +57:25:19.3: 9.90 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.90 +/- 0.00
Forced photometry filter REJECTED candidate at 02:37:08.76 +57:25:19.3: ref_mag=9.90 +/- 0.00 new_mean_mag=10.0705 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:57.02 +58:36:59.3: 14.61 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:28.10 +58:18:15.0: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:57.02 +58:36:59.3: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Forced photometry filter KEPT candidate at 02:00:57.02 +58:36:59.3: ref_mag=11.45 +/- 0.01 new_mean_mag=10.1538 delta=1.30 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:12.04 +59:15:22.9: 13.51 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:28.10 +58:18:15.0: 10.43 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:23.58 +57:43:21.9: 14.71 +/- 0.13 detection
Forced photometry reference-image weighted average: 10.43 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:06.44 +56:37:23.9: 15.66 +/- 99.00 upperlimit
Forced photometry filter KEPT candidate at 02:01:28.10 +58:18:15.0: ref_mag=10.43 +/- 0.00 new_mean_mag=9.3564 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:23.58 +57:43:21.9: 10.66 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:06.44 +56:37:23.9: 9.61 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.66 +/- 0.00
Forced photometry filter KEPT candidate at 02:03:23.58 +57:43:21.9: ref_mag=10.66 +/- 0.00 new_mean_mag=9.7114 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 9.61 +/- 0.00
Forced photometry filter REJECTED candidate at 02:34:06.44 +56:37:23.9: ref_mag=9.61 +/- 0.00 new_mean_mag=10.0705 delta=-0.46 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:12.04 +59:15:22.9: 11.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 0.01
Forced photometry filter KEPT candidate at 01:16:12.04 +59:15:22.9: ref_mag=11.50 +/- 0.01 new_mean_mag=10.5060 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:00.77 +64:39:24.1: 11.62 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.06 +59:15:34.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:36.46 +58:48:08.9: 14.68 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:35.29 +65:02:04.9: 11.89 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.06 +59:15:34.2: 9.75 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:00.77 +64:39:24.1: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter KEPT candidate at 01:56:38.06 +59:15:34.2: ref_mag=9.75 +/- 0.00 new_mean_mag=8.6714 delta=1.08 (need > 0.90)
Forced photometry reference-image weighted average: 11.39 +/- 0.00
Forced photometry filter KEPT candidate at 01:23:00.77 +64:39:24.1: ref_mag=11.39 +/- 0.00 new_mean_mag=10.3456 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:36.46 +58:48:08.9: 10.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.22 +/- 0.00
Forced photometry filter KEPT candidate at 01:43:36.46 +58:48:08.9: ref_mag=10.22 +/- 0.00 new_mean_mag=9.0896 delta=1.13 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:35.29 +65:02:04.9: 10.79 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.92 +/- 0.00
Forced photometry filter KEPT candidate at 01:29:35.29 +65:02:04.9: ref_mag=10.92 +/- 0.00 new_mean_mag=9.6950 delta=1.22 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:40.62 +60:54:41.8: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:40.62 +60:54:41.8: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Forced photometry filter KEPT candidate at 02:21:40.62 +60:54:41.8: ref_mag=11.02 +/- 0.00 new_mean_mag=9.2098 delta=1.81 (need > 0.90)
Adding exclusion_list_local.txt__out03912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25175.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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: 5s
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Considering the candidate 52192_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52192_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:36:59.87 +63:08:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52196_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52196_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:25:58.12 +56:06:09.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52199_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52199_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:30:05.05 +56:40:24.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52204_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52204_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:38:38.22 +57:48:59.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52206_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52206_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:22:56.90 +56:21:06.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52208_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52208_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52212_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52212_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52216_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52216_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:55.56 +56:35:49.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52220_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52220_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:24:41.67 +56:26:14.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52227_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52227_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:31:19.52 +56:53:52.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52228_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52228_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52232_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52232_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:28:23.78 +56:15:13.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52237_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52237_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:33:16.62 +57:14:04.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52240_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52240_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:34:06.49 +57:00:22.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52243_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52243_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52249_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52249_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52254_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52254_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:34:58.94 +55:59:00.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52258_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52258_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:33:24.90 +56:01:04.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52265_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52265_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52270_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52270_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52278_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52278_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52281_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52281_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52288_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52288_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52289_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52289_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52291_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52291_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52292_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52292_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:13.30 +56:42:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52295_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52295_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52298_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52298_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52303_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52303_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52310_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52310_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:56.85 +56:38:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52314_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52314_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52316_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52316_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52317_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52317_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52320_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52320_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52322_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52322_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52328_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52328_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52331_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52331_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 52334_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52334_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 17307_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 17307_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:25:50.53 +60:14:05.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 06468_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 06468_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:54:23.50 +63:40:00.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 26424_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 26424_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:51:53.18 +57:12:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23244_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 23244_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 22258_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 22258_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 21628_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 21628_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 25035_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 25035_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 51449_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 51449_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:30:27.32 +62:31:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01829_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 01829_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:10:22.61 +66:07:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27684_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 27684_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:06:39.44 +56:51:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25175_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 25175_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 04981_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 04981_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 20109_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 20109_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 22210_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 22210_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 03912_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 03912_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 12304_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 12304_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 23703_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 23703_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:54:54.01 +58:33:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21078_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 21078_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:33:56.03 +59:13:57.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 25301_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 25301_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:33:25.88 +58:19:39.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 28196_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 28196_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:38:07.66 +57:58:40.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 23009_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 23009_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:18:00.06 +57:53:59.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 30188_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 30188_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:20:05.20 +58:13:54.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 27918_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 27918_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:18:14.14 +57:48:12.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 28043_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 28043_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:49:09.98 +57:48:39.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 14927_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 14927_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:50:10.03 +63:07:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250664_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250664_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:40:31.54 +64:17:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250666_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250666_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 250668_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250668_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 250674_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250674_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 250676_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250676_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 250677_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250677_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 250680_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250680_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 250684_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250684_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:16:20.68 +62:42:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250685_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250685_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 250687_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250687_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 250696_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250696_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 250697_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250697_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 250698_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250698_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:46:28.32 +57:49:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250724_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250724_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:33:32.91 +57:32:16.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250729_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250729_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:25:58.14 +56:06:09.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250732_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250732_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:30:05.03 +56:40:24.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250735_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250735_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:38:38.19 +57:48:60.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250737_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250737_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:22:56.80 +56:21:08.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250738_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250738_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:32:24.79 +57:25:44.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250740_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250740_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 250741_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250741_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 250745_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250745_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:30:02.46 +57:14:56.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250746_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250746_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 250752_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250752_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:36:35.77 +57:43:12.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250753_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250753_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:55.58 +56:35:49.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250756_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250756_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:24:41.65 +56:26:15.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250759_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250759_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:29:21.70 +57:05:22.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250767_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250767_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 250768_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250768_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:31:19.53 +56:53:52.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250770_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250770_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:25:59.02 +56:39:28.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250779_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250779_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:33:16.61 +57:14:04.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250780_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250780_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:28:23.80 +56:15:13.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250781_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250781_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:34:06.50 +57:00:22.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250782_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250782_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250792_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250792_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250793_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250793_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:36:13.72 +57:43:39.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250794_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250794_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:34:58.96 +55:59:00.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250800_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250800_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:33:24.91 +56:01:04.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250808_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250808_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250811_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250811_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250813_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250813_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250819_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250819_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250822_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250822_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250829_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250829_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250830_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250830_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250832_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250832_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250839_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250839_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250841_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250841_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:13.32 +56:42:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250844_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250844_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250850_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250850_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250851_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250851_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:26:33.90 +56:48:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250855_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250855_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:56.89 +56:38:22.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250858_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250858_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250859_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250859_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250865_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250865_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250867_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250867_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250868_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250868_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250872_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250872_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250874_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250874_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250875_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250875_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250876_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250876_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250878_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250878_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250879_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250879_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250880_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250880_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250887_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250887_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250888_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250888_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250895_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250895_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250896_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250896_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250898_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250898_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250899_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250899_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250900_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250900_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250904_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250904_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250906_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250906_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250908_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250908_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250910_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250910_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250911_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250911_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250913_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250913_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:03.15 +56:50:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250918_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250918_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250927_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250927_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250932_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250932_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250934_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250934_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250943_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250943_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250949_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250949_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250951_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250951_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:29:45.54 +56:46:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250953_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250953_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250959_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250959_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:26:41.05 +60:46:45.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250964_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250964_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250966_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250966_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:26:29.19 +56:54:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250976_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250976_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250977_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250977_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:28:23.97 +56:37:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250978_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250978_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250983_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250983_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250984_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250984_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:26:47.84 +56:36:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250987_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250987_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250988_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250988_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250989_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250989_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250990_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 250990_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250991_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250991_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:28:54.17 +56:38:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250998_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 250998_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251000_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251000_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251003_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251003_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:32:00.57 +56:41:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251010_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251010_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251015_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251015_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251018_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251018_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251020_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251020_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251022_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251022_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:22.89 +56:43:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251023_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251023_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251031_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251031_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251034_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251034_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251035_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251035_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251036_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251036_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251037_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251037_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251045_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251045_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251055_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251055_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251057_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251057_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251059_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251059_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251060_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251060_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:28:18.09 +56:48:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251062_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251062_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251065_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251065_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251070_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251070_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251071_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251071_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251072_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251072_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251073_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251073_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 251077_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251077_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251082_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251082_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251085_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251085_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251089_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251089_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:18:49.88 +57:07:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251090_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251090_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251091_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251091_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251097_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251097_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251098_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251098_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251101_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251101_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251103_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251103_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251106_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251106_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251109_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251109_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251112_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251112_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251116_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251116_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251117_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251117_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:56:38.50 +59:13:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251127_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251127_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251131_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251131_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251133_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251133_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:26:55.86 +56:44:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251138_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251138_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251144_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251144_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251151_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251151_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:49.07 +56:39:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251152_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251152_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251153_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251153_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251157_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251157_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251164_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251164_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 251166_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251166_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:19:12.10 +65:36:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251174_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251174_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251179_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251179_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:36.03 +56:56:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251182_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251182_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251187_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251187_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251191_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251191_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251193_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251193_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251194_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251194_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251196_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251196_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251200_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251200_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251211_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251211_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:08:42.47 +58:16:26.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251220_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251220_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:29:19.49 +56:49:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251221_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251221_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251223_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251223_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:49:48.22 +65:05:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251225_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251225_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251228_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251228_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251233_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251233_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251240_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251240_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251243_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251243_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251248_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251248_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251253_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251253_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:53:16.18 +61:08:53.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251256_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251256_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251259_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251259_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:51:37.33 +63:46:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251263_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251263_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251270_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251270_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251274_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251274_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251276_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251276_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251278_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251278_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251282_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251282_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:58.04 +56:42:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251289_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251289_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251290_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251290_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251293_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251293_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251294_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251294_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:53:11.58 +61:06:00.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251297_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251297_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251298_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251298_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251299_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251299_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 251304_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251304_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:03:46.76 +61:03:19.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251305_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251305_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251310_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251310_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251313_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251313_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251331_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251331_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:41:44.72 +65:51:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251333_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251333_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251336_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251336_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251338_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251338_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251339_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251339_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251344_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251344_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251347_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251347_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:29:00.21 +56:46:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251348_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251348_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251349_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251349_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251351_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251351_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:01.19 +56:41:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251352_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251352_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251353_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251353_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251359_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251359_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251360_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251360_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251362_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251362_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251363_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251363_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251364_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251364_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251369_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251369_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251371_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251371_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251374_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251374_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:46:48.44 +59:52:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251375_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251375_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251392_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251392_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251403_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251403_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251404_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251404_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251406_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251406_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:26:27.53 +56:51:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251413_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251413_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251415_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251415_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251423_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251423_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251424_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251424_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251426_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251426_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251430_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251430_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:26:44.58 +56:50:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251437_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251437_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251438_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251438_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251443_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251443_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251449_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251449_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:35:14.87 +63:00:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251460_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251460_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:27:22.51 +56:52:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251463_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251463_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251471_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251471_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251473_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251473_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:28:04.34 +57:06:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251492_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251492_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251496_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251496_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
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Considering the candidate 251504_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251504_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251509_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251509_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251529_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251529_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:31:04.15 +66:05:03.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251547_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251547_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:40:50.63 +64:17:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251548_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251548_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251555_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251555_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251558_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251558_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:32:46.33 +56:29:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251563_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251563_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251564_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251564_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:00:36.59 +63:32:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251571_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251571_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251579_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251579_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251585_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251585_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251589_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251589_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 251597_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251597_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:55:40.84 +63:34:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251623_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251623_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251685_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251685_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251722_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251722_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251740_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251740_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:39:56.88 +60:52:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251745_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 251745_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 251750_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 251750_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:11:50.35 +59:02:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211163_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 211163_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 52771_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 52771_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 83217_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 83217_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:51:14.25 +62:38:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05499_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 05499_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 132860_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 132860_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 41626_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 41626_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:23:00.80 +64:39:24.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 14814_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 14814_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:10:22.53 +66:07:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11582_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 11582_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:47:22.20 +66:08:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212460_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 212460_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 104399_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 104399_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:21:40.61 +60:54:41.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 125561_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 125561_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 17104_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 17104_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 137179_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 137179_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 70010_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 70010_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:22:18.00 +62:28:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79932_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 79932_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 211999_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 211999_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:51:53.17 +57:12:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198104_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 198104_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 43239_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 43239_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 161725_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 161725_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:53:42.57 +59:14:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94914_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 94914_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 21138_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 21138_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:15:23.75 +65:01:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212283_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 212283_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 17836_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 17836_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 67097_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 67097_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:36:59.88 +63:08:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26060_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 26060_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 112593_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 112593_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 214517_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 214517_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:06:39.51 +56:51:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94485_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 94485_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 35970_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 35970_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 49419_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 49419_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 219961_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 219961_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 64480_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 64480_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 208550_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 208550_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 62860_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 62860_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:11:58.93 +63:39:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93692_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 93692_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 99657_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 99657_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 60369_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 60369_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 46105_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 46105_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:38:00.97 +63:01:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100659_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 100659_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 104143_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 104143_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 218278_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 218278_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 134816_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 134816_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 198752_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 198752_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 132193_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 132193_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 64440_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 64440_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:18:52.47 +62:48:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72532_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 72532_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:45:35.91 +63:07:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211875_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 211875_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:11:03.61 +57:20:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74963_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 74963_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 162256_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 162256_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 174355_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 174355_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 197208_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 197208_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 16262_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 16262_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 14863_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 14863_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:12:35.09 +65:31:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97026_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 97026_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 128710_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 128710_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:29:38.77 +60:38:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150819_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 150819_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 29996_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 29996_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 130602_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 130602_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 107137_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 107137_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 128330_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 128330_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 194834_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 194834_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 136934_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 136934_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 158689_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 158689_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 119923_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 119923_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 34270_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 34270_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:29:35.31 +65:02:04.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 96282_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 96282_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 42095_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 42095_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09190_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 09190_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:57:10.19 +66:18:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165523_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 165523_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 23392_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 23392_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 135883_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 135883_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 109215_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 109215_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193233_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 193233_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121739_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 121739_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124320_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 124320_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09761_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 09761_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:43:34.12 +65:01:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140285_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 140285_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189533_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 189533_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64411_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 64411_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:54:26.38 +63:33:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150443_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 150443_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34359_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 34359_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:34:27.19 +64:32:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31018_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 31018_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66586_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 66586_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169916_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 169916_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06001_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 06001_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:40:48.62 +66:47:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147117_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 147117_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84591_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 84591_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 70271_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:20:32.70 +62:32:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77217_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 77217_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183784_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 183784_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:03:23.59 +57:43:21.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 79040_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 79040_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 08613_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 08613_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:38:31.97 +65:19:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22320_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 22320_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91176_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 91176_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 209823_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 209823_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186491_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 186491_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151243_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 151243_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 143925_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 143925_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 132234_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 132234_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 33327_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 33327_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 29588_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 29588_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 170536_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 170536_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 157256_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 157256_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52486_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 52486_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57702_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 57702_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86122_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 86122_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162641_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 162641_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178697_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 178697_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173490_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 173490_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:22:51.71 +57:50:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235808_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 235808_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:53:03.10 +60:35:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191638_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 191638_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 154238_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 154238_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182343_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 182343_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167800_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 167800_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 61091_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 61091_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196494_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 196494_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:01:28.08 +58:18:15.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 12765_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 12765_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:15:15.23 +65:42:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127654_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 127654_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108178_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 108178_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:57:35.97 +61:28:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122256_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 122256_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:03:28.65 +60:53:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167698_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 167698_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 131046_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 131046_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 168042_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 168042_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 39378_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 39378_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:47:55.77 +64:32:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201907_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 201907_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:43:36.46 +58:48:08.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 104733_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 104733_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 218902_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 218902_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 99262_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 99262_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 152727_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 152727_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 28797_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 28797_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 181306_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 181306_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 150154_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 150154_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 62555_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 62555_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 188873_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 188873_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 213360_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 213360_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:37:01.90 +57:20:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180134_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 180134_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 206858_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 206858_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 169253_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 169253_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 65408_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 65408_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 234011_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 234011_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 28836_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 28836_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 92825_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 92825_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133678_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 133678_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:55:19.05 +60:21:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70015_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 70015_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 45963_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 45963_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113164_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 113164_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117190_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 117190_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 170381_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 170381_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 154592_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 154592_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 18681_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 18681_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115890_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 115890_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 149005_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 149005_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169062_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 169062_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209662_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 209662_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07627_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 07627_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:25:13.38 +65:50:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103250_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 103250_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102951_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 102951_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 157757_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 157757_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189549_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 189549_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:26:31.09 +57:15:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71276_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 71276_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189956_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 189956_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:57:41.52 +58:24:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173182_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 173182_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156692_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 156692_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:56:38.06 +59:15:34.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 169994_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 169994_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:00:57.04 +58:36:59.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 46369_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 46369_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:39:02.95 +64:04:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178813_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 178813_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:04:41.95 +57:30:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37338_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 37338_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 213271_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 213271_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 63215_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 63215_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:30:27.31 +62:31:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159068_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 159068_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 22840_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 22840_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32774_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 32774_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:11:21.06 +65:02:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218524_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 218524_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 52199_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 52199_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:33:00.80 +62:55:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165063_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 165063_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:16:12.08 +59:15:23.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 08171_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 08171_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:18:51.02 +66:40:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193780_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 193780_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:54:54.03 +58:33:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205464_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 205464_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 221536_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 221536_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47584_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 47584_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11752_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 11752_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16151_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 16151_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:35:34.13 +65:57:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180648_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 180648_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19108_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 19108_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:16:22.43 +65:06:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173077_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 173077_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:50:59.58 +57:36:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58464_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 58464_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 140363_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 140363_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 92223_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 92223_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 212839_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 212839_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 81003_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 81003_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 34115_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 34115_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 03631_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 03631_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:06:04.77 +66:39:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87644_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 87644_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 167724_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 167724_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 119069_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 119069_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 191949_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 191949_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 60293_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 60293_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 148734_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 148734_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 76362_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 76362_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 42016_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 42016_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113819_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 113819_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 92055_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 92055_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 38313_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 38313_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94003_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 94003_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
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Considering the candidate 104341_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 104341_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:40:38.97 +60:07:56.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137699_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 137699_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:54:00.46 +60:09:11.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 95851_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 95851_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:01:59.02 +61:54:17.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123657_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 123657_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:39:51.69 +60:54:08.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53518_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 53518_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118439_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 118439_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:39:07.14 +61:04:44.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91675_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 91675_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:38:12.60 +62:21:06.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 130634_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 130634_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:42:36.84 +60:32:52.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 92255_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 92255_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:00:48.39 +62:16:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119210_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 119210_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:42:02.95 +61:02:17.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138010_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 138010_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:59:39.29 +60:00:27.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 77887_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 77887_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:35:24.22 +63:04:54.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 110464_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 110464_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:42:58.33 +61:25:15.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 209628_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 209628_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:10:15.70 +56:33:34.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 152648_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 152648_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:30:18.34 +59:46:55.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130177_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 130177_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:43:19.82 +60:33:04.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 154479_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 154479_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:43:21.75 +59:37:56.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99961_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 99961_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:58:33.18 +61:41:51.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 57636_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 57636_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:47:47.09 +63:50:58.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172562_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 172562_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:22:06.68 +56:36:17.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59296_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 59296_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:15:55.35 +63:14:09.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132300_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 132300_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:10:25.71 +59:58:45.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61006_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 61006_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:54:23.62 +63:40:05.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183446_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 183446_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:47:18.03 +58:01:15.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146540_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 146540_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:25:50.54 +60:14:05.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34107_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 34107_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:51:16.89 +64:51:15.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197508_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 197508_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:42:17.77 +58:37:38.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37245_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 37245_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:59:37.94 +64:37:12.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41238_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 41238_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:02:59.97 +64:23:20.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167582_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 167582_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:33:56.02 +59:13:57.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209544_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 209544_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:49:13.98 +57:04:30.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29461_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 29461_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:02:52.32 +64:54:03.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187039_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 187039_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:33:25.87 +58:19:39.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220118_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 220118_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:44:17.95 +57:32:13.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178877_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 178877_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:38:07.63 +57:58:40.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53389_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 53389_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:11:26.12 +64:12:05.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165386_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 165386_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:13:41.62 +58:33:38.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180632_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 180632_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:23:21.84 +58:08:32.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163793_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 163793_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:31:26.83 +58:01:29.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201275_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 201275_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:03:37.27 +58:54:32.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209716_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 209716_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:44:45.88 +57:05:25.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153703_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 153703_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110212_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 110212_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:04:19.44 +61:34:46.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183006_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 183006_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:20:05.16 +58:13:54.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186343_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 186343_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:11:29.20 +57:38:43.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120817_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 120817_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:03:37.23 +61:04:27.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189206_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 189206_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:18:04.41 +57:30:59.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179947_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 179947_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:56:13.09 +57:59:46.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12740_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 12740_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:56:24.22 +64:19:54.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102620_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 102620_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:51:16.75 +61:48:18.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134016_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 134016_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:56:43.09 +60:42:58.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136163_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 136163_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:56:47.30 +60:21:45.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117510_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 117510_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:53:04.41 +61:07:29.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171259_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 171259_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:55:00.38 +58:58:19.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168448_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 168448_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:56:39.97 +59:10:49.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183651_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 183651_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:08:33.63 +58:15:47.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188414_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 188414_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:18:00.05 +57:53:59.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172645_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 172645_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 01:18:14.12 +57:48:12.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 221182_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 221182_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 00:49:09.97 +57:48:39.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137025_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
Preparing report for the candidate 137025_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05877_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319
The candidate 05877_fd_Cas-03-Q1b1x1_2026-05-28_03-41-21_20.00sec_-0.00C_LIGHTs_0319 did not pass the final checks
**** FOUND 02:37:36.13 +65:44:41.0 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 18s
make_report_in_HTML.sh TOTAL: 481s
Prepared the HTML report for the field Cas-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:29:35.29 +65:02:04.9
01:23:00.77 +64:39:24.1
02:21:40.62 +60:54:41.8
01:56:38.06 +59:15:34.2
01:16:12.04 +59:15:22.9
01:43:36.46 +58:48:08.9
02:00:57.02 +58:36:59.3
02:01:28.10 +58:18:15.0
02:03:23.58 +57:43:21.9
02:41:50.08 +65:30:27.2
02:07:48.46 +61:22:16.5
01:32:44.39 +61:45:35.6
01:04:09.24 +61:46:55.9
02:36:10.97 +60:22:42.0
02:27:23.77 +60:40:47.8
01:41:01.13 +61:31:00.7
01:54:09.12 +61:13:07.0
01:21:54.86 +61:20:56.1
01:36:43.18 +61:14:25.3
01:37:01.41 +61:15:57.1
01:28:36.28 +61:12:06.7
02:00:13.56 +60:43:20.6
02:43:55.93 +64:48:54.7
01:46:05.47 +60:59:36.6
02:20:33.64 +60:06:16.7
01:40:46.01 +60:51:39.7
01:25:43.43 +60:50:05.7
02:24:46.68 +59:43:52.9
02:07:16.67 +60:08:10.8
02:09:24.81 +60:03:15.6
02:19:16.53 +59:42:22.1
01:30:50.42 +60:32:14.2
01:36:21.66 +60:26:52.3
01:04:58.46 +60:30:20.5
02:09:48.70 +59:51:47.0
02:24:29.68 +59:24:31.5
01:32:27.26 +60:20:31.1
01:56:15.73 +60:01:03.3
01:35:09.89 +60:17:10.6
01:12:18.51 +60:20:30.2
01:16:28.97 +60:14:00.5
02:19:59.14 +59:17:32.1
01:44:48.84 +59:53:34.1
01:26:01.01 +59:55:35.7
01:35:57.20 +59:47:27.0
02:02:39.14 +59:22:44.0
02:08:15.60 +59:15:57.1
02:28:12.53 +58:37:11.5
02:11:34.44 +59:06:06.6
01:39:46.89 +59:42:30.5
01:14:57.02 +59:42:13.2
02:18:22.56 +58:47:09.8
01:24:30.64 +59:38:48.6
00:58:01.37 +59:33:23.2
02:18:24.73 +58:37:25.8
02:37:50.65 +57:54:15.4
02:24:41.13 +58:22:35.6
00:41:52.39 +59:10:02.9
02:08:54.01 +58:42:29.5
02:11:32.08 +65:25:28.2
02:19:34.19 +58:23:57.9
01:41:46.93 +59:03:48.0
02:33:40.04 +57:40:02.5
02:16:28.46 +58:16:12.0
01:17:41.64 +59:18:24.2
01:09:38.03 +59:05:13.6
02:03:00.34 +58:36:13.4
01:01:55.32 +59:00:14.3
02:33:31.95 +57:34:09.2
01:20:05.35 +59:00:13.2
01:11:51.39 +58:59:24.6
02:48:49.52 +64:11:51.9
02:03:07.41 +57:18:14.7
02:31:46.08 +56:26:43.2
01:54:12.35 +65:38:24.8
01:01:19.84 +58:00:01.2
02:34:06.44 +56:37:23.7
01:45:16.05 +57:55:46.8
01:18:52.86 +58:09:31.4
02:00:17.58 +57:43:39.7
01:47:21.78 +58:08:40.5
01:51:45.69 +65:36:52.8
02:14:46.56 +57:37:03.4
02:14:45.13 +57:39:36.6
01:16:04.83 +58:33:49.3
01:43:45.28 +58:23:45.8
01:36:20.44 +58:31:43.2
02:01:05.84 +58:11:26.9
02:19:12.27 +57:48:50.2
02:05:05.77 +58:16:24.6
01:43:58.28 +58:41:06.0
01:41:34.22 +56:56:31.6
01:10:29.41 +57:08:53.0
02:15:35.96 +56:21:40.4
01:31:04.89 +57:13:14.0
01:47:07.73 +57:00:34.1
01:38:21.64 +57:13:51.3
01:22:16.36 +57:23:06.8
01:31:28.19 +57:20:36.7
01:02:09.20 +57:21:42.2
02:31:46.25 +55:57:57.3
01:23:04.06 +57:36:35.9
01:52:19.54 +57:19:07.3
01:54:28.56 +57:17:51.0
02:25:13.42 +56:30:32.3
02:31:18.98 +56:20:50.6
02:34:32.44 +64:22:56.6
02:33:23.67 +64:25:00.1
02:28:12.08 +64:31:52.8
01:23:21.85 +60:18:14.4
01:43:02.78 +61:34:06.4
00:51:08.53 +64:31:35.6
02:00:14.31 +65:03:58.2
01:02:16.17 +57:08:41.8
01:25:39.69 +59:16:07.4
02:19:45.31 +57:01:15.4
01:46:35.86 +59:12:14.3
02:03:11.16 +62:07:52.0
00:36:55.23 +62:40:46.4
00:51:15.99 +58:39:34.3
02:25:27.64 +56:46:55.8
02:29:09.02 +56:37:12.7
02:18:53.85 +57:08:41.8
02:32:05.67 +56:39:57.3
02:27:58.38 +56:02:38.8
02:31:26.37 +55:59:07.4
02:29:10.08 +56:27:14.1
02:34:11.11 +55:49:59.2
02:35:38.10 +57:29:11.6
02:30:54.10 +56:14:28.3
02:27:24.36 +56:23:03.5
02:32:05.62 +57:22:03.9
02:32:46.69 +56:48:22.9
02:34:35.28 +56:21:51.3
02:34:44.75 +56:06:07.7
02:33:35.26 +55:54:24.6
02:37:08.74 +57:25:19.6
02:36:33.17 +57:54:38.3
02:27:20.52 +56:01:48.8
02:31:26.05 +56:07:04.8
02:35:52.05 +57:47:21.5
02:26:59.10 +56:01:58.1
02:32:16.04 +56:38:48.1
02:24:11.88 +56:35:43.2
02:36:29.15 +57:11:43.0
02:33:01.83 +57:02:06.6
02:21:16.42 +57:08:40.1
02:34:06.21 +56:25:27.6
02:36:36.23 +57:46:58.2
02:20:54.00 +56:16:37.9
02:29:12.20 +56:18:00.7
02:22:35.24 +56:18:15.4
02:32:55.76 +56:39:38.1
02:30:44.92 +56:56:13.4
02:37:36.90 +57:51:16.6
02:21:55.26 +56:25:09.3
02:28:50.68 +56:20:50.4
02:31:06.61 +56:30:44.0
02:30:12.73 +56:11:27.6
02:24:41.97 +56:55:48.3
02:31:11.88 +57:09:48.4
02:35:34.11 +57:09:17.2
02:37:55.13 +57:39:02.3
02:27:07.81 +56:33:54.6
02:38:46.94 +57:49:57.0
02:25:28.20 +56:11:20.2
02:34:04.70 +56:30:40.2
02:25:34.10 +56:34:22.3
02:32:45.29 +57:08:07.3
02:31:38.17 +56:33:35.0
02:32:05.15 +56:49:22.4
02:22:10.11 +56:24:22.8
02:30:51.88 +57:04:10.0
02:25:20.49 +56:12:13.5
02:19:52.90 +56:15:39.2
02:33:49.42 +57:35:11.7
02:33:29.99 +57:42:17.0
02:31:38.51 +57:13:48.2
02:33:48.99 +57:01:45.0
02:24:06.55 +56:30:01.1
02:36:56.79 +57:06:43.6
02:31:18.98 +55:53:51.0
02:24:09.75 +56:34:02.5
02:37:31.97 +57:28:17.7
00:52:30.58 +59:43:27.9
02:30:37.35 +56:23:01.5
02:36:19.99 +57:15:26.8
02:35:18.58 +57:31:37.0
02:32:18.76 +56:21:25.6
02:21:59.04 +56:30:02.2
02:22:31.60 +56:14:10.7
02:30:30.72 +57:30:28.2
02:36:08.67 +57:39:33.5
02:22:04.64 +57:10:39.2
02:33:05.67 +56:13:01.3
02:27:33.00 +56:13:09.5
02:31:59.20 +56:42:22.0
02:26:07.28 +56:25:11.5
02:36:35.17 +57:36:34.3
02:35:20.47 +57:29:29.4
02:37:41.05 +57:33:20.1
02:30:49.77 +56:11:02.6
00:57:05.28 +57:30:11.8
02:30:33.01 +56:53:08.7
02:19:44.52 +56:42:25.7
02:21:04.81 +56:15:32.5
02:26:13.37 +56:36:45.1
02:29:33.40 +55:57:20.3
02:36:22.57 +57:40:03.4
02:33:09.48 +57:00:39.2
02:29:50.72 +56:19:10.9
02:29:41.24 +56:20:06.8
02:28:09.92 +56:10:50.3
02:34:26.97 +56:29:12.2
02:31:06.05 +56:37:19.1
02:40:07.39 +58:29:00.9
02:35:08.80 +57:36:14.7
02:34:05.16 +56:42:26.1
02:32:26.23 +56:47:10.1
02:33:13.67 +57:44:32.4
02:30:52.97 +56:54:21.1
02:29:40.98 +56:18:42.4
02:35:43.04 +56:44:19.4
02:32:59.22 +57:28:35.8
02:28:41.20 +56:12:06.5
02:18:24.04 +56:23:24.4
02:29:57.20 +56:36:49.0
02:29:58.23 +56:08:53.2
02:35:04.79 +57:26:52.8
02:19:36.25 +56:23:22.4
02:31:28.99 +57:11:53.7
02:37:50.62 +57:45:48.2
02:29:28.85 +56:33:09.5
02:29:39.44 +56:11:35.3
02:26:43.32 +56:24:14.7
02:29:59.81 +56:13:02.8
02:21:34.70 +56:26:46.5
02:31:09.60 +57:16:15.9
02:26:55.68 +56:30:21.4
02:35:30.33 +57:03:27.8
02:28:49.65 +56:07:39.2
02:26:10.82 +56:48:29.2
02:32:17.90 +57:17:10.0
02:34:24.43 +57:28:27.5
02:31:51.85 +56:45:48.0
02:25:42.03 +56:37:15.5
02:36:59.24 +57:56:30.4
02:33:03.14 +57:03:26.9
02:36:07.89 +57:21:40.2
02:20:24.36 +56:41:46.0
02:20:07.34 +56:27:53.6
02:26:02.45 +56:20:59.5
02:26:00.91 +56:46:18.9
02:33:37.63 +57:40:23.9
02:24:52.65 +56:43:13.3
02:40:00.93 +58:49:46.1
02:38:18.56 +57:37:39.8
02:27:22.97 +56:19:26.0
02:25:30.00 +56:16:55.3
02:30:16.58 +56:38:11.3
01:22:23.94 +61:13:51.2
00:52:12.67 +64:57:20.9
02:14:27.98 +64:44:14.9
01:49:47.69 +65:03:21.3
02:23:18.51 +64:21:47.0
02:22:32.05 +64:22:11.7
02:24:19.53 +64:16:12.9
02:14:26.77 +64:29:24.6
01:09:49.42 +65:08:28.8
02:07:21.55 +64:28:11.9
01:57:52.45 +64:34:23.0
02:19:36.15 +64:09:18.0
01:13:09.77 +64:46:43.6
02:03:34.92 +64:11:47.7
02:24:05.02 +63:37:15.8
01:20:18.43 +64:28:04.9
02:24:19.74 +63:24:35.5
02:34:40.00 +63:00:03.4
01:57:53.16 +63:48:41.1
01:50:36.43 +63:53:30.1
02:30:58.99 +62:56:15.2
02:12:24.62 +63:16:01.2
02:13:47.58 +63:11:26.0
02:41:04.44 +62:17:31.5
02:45:57.12 +62:02:43.5
02:13:08.99 +63:06:22.8
02:27:21.83 +62:38:26.5
02:19:04.00 +62:47:33.4
01:21:36.46 +63:33:51.0
02:15:26.81 +62:47:45.7
02:38:33.43 +61:54:31.0
02:32:40.32 +62:07:15.6
02:05:50.44 +62:42:31.3
01:36:47.30 +63:02:42.6
01:55:07.62 +62:47:31.4
02:33:47.87 +61:42:03.3
02:15:20.43 +62:13:50.0
02:07:37.49 +62:22:07.0
02:07:46.89 +62:11:10.9
02:42:10.42 +61:03:22.2
01:23:28.70 +62:35:10.1
02:23:38.25 +61:24:57.1
02:43:44.79 +60:40:26.6
01:56:16.77 +62:11:52.2
02:21:20.02 +61:23:53.5
01:47:43.89 +62:06:37.4
01:25:56.70 +62:14:49.4
02:39:22.81 +60:42:41.0
01:15:48.97 +62:13:51.2
01:27:44.43 +62:06:40.7
02:24:34.96 +61:05:35.0
01:23:02.01 +61:59:41.5
02:31:25.66 +60:43:53.6
########### Completed Cas-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
02:01:28.10 +58:18:15.0
02:00:57.02 +58:36:59.3
01:16:12.04 +59:15:22.9
02:03:23.58 +57:43:21.9
01:23:00.77 +64:39:24.1
01:56:38.06 +59:15:34.2
01:43:36.46 +58:48:08.9
01:29:35.29 +65:02:04.9
02:21:40.62 +60:54:41.8
01:43:02.78 +61:34:06.4
00:51:08.53 +64:31:35.6
02:00:14.31 +65:03:58.2
01:02:16.17 +57:08:41.8
01:25:39.69 +59:16:07.4
02:19:45.31 +57:01:15.4
01:46:35.86 +59:12:14.3
02:03:11.16 +62:07:52.0
00:36:55.23 +62:40:46.4
00:51:15.99 +58:39:34.3
02:25:27.64 +56:46:55.8
02:29:09.02 +56:37:12.7
02:18:53.85 +57:08:41.8
02:32:05.67 +56:39:57.3
02:27:58.38 +56:02:38.8
02:31:26.37 +55:59:07.4
02:29:10.08 +56:27:14.1
02:34:11.11 +55:49:59.2
02:35:38.10 +57:29:11.6
02:30:54.10 +56:14:28.3
02:27:24.36 +56:23:03.5
02:32:05.62 +57:22:03.9
02:32:46.69 +56:48:22.9
02:34:35.28 +56:21:51.3
02:34:44.75 +56:06:07.7
02:33:35.26 +55:54:24.6
02:37:08.74 +57:25:19.6
02:36:33.17 +57:54:38.3
02:27:20.52 +56:01:48.8
02:31:26.05 +56:07:04.8
02:35:52.05 +57:47:21.5
02:26:59.10 +56:01:58.1
02:32:16.04 +56:38:48.1
02:24:11.88 +56:35:43.2
02:36:29.15 +57:11:43.0
02:33:01.83 +57:02:06.6
02:21:16.42 +57:08:40.1
02:34:06.21 +56:25:27.6
02:36:36.23 +57:46:58.2
02:20:54.00 +56:16:37.9
02:29:12.20 +56:18:00.7
02:22:35.24 +56:18:15.4
02:32:55.76 +56:39:38.1
02:30:44.92 +56:56:13.4
02:37:36.90 +57:51:16.6
02:21:55.26 +56:25:09.3
02:28:50.68 +56:20:50.4
02:31:06.61 +56:30:44.0
02:30:12.73 +56:11:27.6
02:24:41.97 +56:55:48.3
02:31:11.88 +57:09:48.4
02:35:34.11 +57:09:17.2
02:37:55.13 +57:39:02.3
02:27:07.81 +56:33:54.6
02:38:46.94 +57:49:57.0
02:25:28.20 +56:11:20.2
02:34:04.70 +56:30:40.2
02:25:34.10 +56:34:22.3
02:32:45.29 +57:08:07.3
02:31:38.17 +56:33:35.0
02:32:05.15 +56:49:22.4
02:22:10.11 +56:24:22.8
02:30:51.88 +57:04:10.0
02:25:20.49 +56:12:13.5
02:19:52.90 +56:15:39.2
02:33:49.42 +57:35:11.7
02:33:29.99 +57:42:17.0
02:31:38.51 +57:13:48.2
02:33:48.99 +57:01:45.0
02:24:06.55 +56:30:01.1
02:36:56.79 +57:06:43.6
02:31:18.98 +55:53:51.0
02:24:09.75 +56:34:02.5
02:37:31.97 +57:28:17.7
00:52:30.58 +59:43:27.9
02:30:37.35 +56:23:01.5
02:36:19.99 +57:15:26.8
02:35:18.58 +57:31:37.0
02:32:18.76 +56:21:25.6
02:21:59.04 +56:30:02.2
02:22:31.60 +56:14:10.7
02:30:30.72 +57:30:28.2
02:36:08.67 +57:39:33.5
02:22:04.64 +57:10:39.2
02:33:05.67 +56:13:01.3
02:27:33.00 +56:13:09.5
02:31:59.20 +56:42:22.0
02:26:07.28 +56:25:11.5
02:36:35.17 +57:36:34.3
02:35:20.47 +57:29:29.4
02:37:41.05 +57:33:20.1
02:30:49.77 +56:11:02.6
00:57:05.28 +57:30:11.8
02:30:33.01 +56:53:08.7
02:19:44.52 +56:42:25.7
02:21:04.81 +56:15:32.5
02:26:13.37 +56:36:45.1
02:29:33.40 +55:57:20.3
02:36:22.57 +57:40:03.4
02:33:09.48 +57:00:39.2
02:29:50.72 +56:19:10.9
02:29:41.24 +56:20:06.8
02:28:09.92 +56:10:50.3
02:34:26.97 +56:29:12.2
02:31:06.05 +56:37:19.1
02:40:07.39 +58:29:00.9
02:35:08.80 +57:36:14.7
02:34:05.16 +56:42:26.1
02:32:26.23 +56:47:10.1
02:33:13.67 +57:44:32.4
02:30:52.97 +56:54:21.1
02:29:40.98 +56:18:42.4
02:35:43.04 +56:44:19.4
02:32:59.22 +57:28:35.8
02:28:41.20 +56:12:06.5
02:18:24.04 +56:23:24.4
02:29:57.20 +56:36:49.0
02:29:58.23 +56:08:53.2
02:35:04.79 +57:26:52.8
02:19:36.25 +56:23:22.4
02:31:28.99 +57:11:53.7
02:37:50.62 +57:45:48.2
02:29:28.85 +56:33:09.5
02:29:39.44 +56:11:35.3
02:26:43.32 +56:24:14.7
02:29:59.81 +56:13:02.8
02:21:34.70 +56:26:46.5
02:31:09.60 +57:16:15.9
02:26:55.68 +56:30:21.4
02:35:30.33 +57:03:27.8
02:28:49.65 +56:07:39.2
02:26:10.82 +56:48:29.2
02:32:17.90 +57:17:10.0
02:34:24.43 +57:28:27.5
02:31:51.85 +56:45:48.0
02:25:42.03 +56:37:15.5
02:36:59.24 +57:56:30.4
02:33:03.14 +57:03:26.9
02:36:07.89 +57:21:40.2
02:20:24.36 +56:41:46.0
02:20:07.34 +56:27:53.6
02:26:02.45 +56:20:59.5
02:26:00.91 +56:46:18.9
02:33:37.63 +57:40:23.9
02:24:52.65 +56:43:13.3
02:40:00.93 +58:49:46.1
02:38:18.56 +57:37:39.8
02:27:22.97 +56:19:26.0
02:25:30.00 +56:16:55.3
02:30:16.58 +56:38:11.3
01:22:23.94 +61:13:51.2
00:52:12.67 +64:57:20.9
01:38:21.64 +57:13:51.3
01:50:36.43 +63:53:30.1
02:41:50.08 +65:30:27.2
02:09:48.70 +59:51:47.0
01:31:28.19 +57:20:36.7
02:24:46.68 +59:43:52.9
02:48:49.52 +64:11:51.9
01:12:18.51 +60:20:30.2
02:15:20.43 +62:13:50.0
02:05:05.77 +58:16:24.6
02:24:05.02 +63:37:15.8
01:15:48.97 +62:13:51.2
01:22:16.36 +57:23:06.8
01:54:12.35 +65:38:24.8
02:14:27.98 +64:44:14.9
01:21:54.86 +61:20:56.1
02:39:22.81 +60:42:41.0
01:57:52.45 +64:34:23.0
02:34:40.00 +63:00:03.4
02:25:13.42 +56:30:32.3
02:19:04.00 +62:47:33.4
02:15:35.96 +56:21:40.4
01:47:43.89 +62:06:37.4
02:31:25.66 +60:43:53.6
02:45:57.12 +62:02:43.5
02:07:48.46 +61:22:16.5
02:36:10.97 +60:22:42.0
01:23:04.06 +57:36:35.9
02:24:29.68 +59:24:31.5
01:43:58.28 +58:41:06.0
01:36:21.66 +60:26:52.3
02:05:50.44 +62:42:31.3
02:08:54.01 +58:42:29.5
02:31:46.08 +56:26:43.2
02:19:12.27 +57:48:50.2
02:11:32.08 +65:25:28.2
02:24:34.96 +61:05:35.0
02:11:34.44 +59:06:06.6
02:24:19.53 +64:16:12.9
02:19:16.53 +59:42:22.1
01:41:01.13 +61:31:00.7
02:09:24.81 +60:03:15.6
02:01:05.84 +58:11:26.9
01:56:15.73 +60:01:03.3
02:24:41.13 +58:22:35.6
02:20:33.64 +60:06:16.7
01:27:44.43 +62:06:40.7
02:03:34.92 +64:11:47.7
01:41:46.93 +59:03:48.0
02:28:12.08 +64:31:52.8
01:32:27.26 +60:20:31.1
01:54:09.12 +61:13:07.0
01:36:20.44 +58:31:43.2
01:40:46.01 +60:51:39.7
01:25:43.43 +60:50:05.7
01:16:28.97 +60:14:00.5
02:14:45.13 +57:39:36.6
02:28:12.53 +58:37:11.5
02:14:26.77 +64:29:24.6
02:15:26.81 +62:47:45.7
02:33:31.95 +57:34:09.2
01:26:01.01 +59:55:35.7
02:07:46.89 +62:11:10.9
01:55:07.62 +62:47:31.4
02:33:47.87 +61:42:03.3
02:34:32.44 +64:22:56.6
02:23:38.25 +61:24:57.1
01:47:07.73 +57:00:34.1
01:47:21.78 +58:08:40.5
01:39:46.89 +59:42:30.5
01:44:48.84 +59:53:34.1
01:04:58.46 +60:30:20.5
01:09:49.42 +65:08:28.8
02:22:32.05 +64:22:11.7
01:11:51.39 +58:59:24.6
02:18:24.73 +58:37:25.8
01:57:53.16 +63:48:41.1
02:12:24.62 +63:16:01.2
02:42:10.42 +61:03:22.2
02:19:34.19 +58:23:57.9
01:01:19.84 +58:00:01.2
01:16:04.83 +58:33:49.3
01:24:30.64 +59:38:48.6
02:00:17.58 +57:43:39.7
01:17:41.64 +59:18:24.2
02:13:08.99 +63:06:22.8
02:07:16.67 +60:08:10.8
02:33:40.04 +57:40:02.5
01:30:50.42 +60:32:14.2
01:09:38.03 +59:05:13.6
02:27:23.77 +60:40:47.8
01:54:28.56 +57:17:51.0
01:23:02.01 +61:59:41.5
01:14:57.02 +59:42:13.2
01:49:47.69 +65:03:21.3
01:18:52.86 +58:09:31.4
02:08:15.60 +59:15:57.1
02:27:21.83 +62:38:26.5
02:14:46.56 +57:37:03.4
02:34:06.44 +56:37:23.7
01:10:29.41 +57:08:53.0
01:01:55.32 +59:00:14.3
01:21:36.46 +63:33:51.0
01:23:21.85 +60:18:14.4
02:23:18.51 +64:21:47.0
02:21:20.02 +61:23:53.5
02:38:33.43 +61:54:31.0
01:20:18.43 +64:28:04.9
01:36:43.18 +61:14:25.3
02:00:13.56 +60:43:20.6
01:20:05.35 +59:00:13.2
00:58:01.37 +59:33:23.2
01:51:45.69 +65:36:52.8
01:28:36.28 +61:12:06.7
02:02:39.14 +59:22:44.0
02:03:00.34 +58:36:13.4
01:31:04.89 +57:13:14.0
01:04:09.24 +61:46:55.9
01:32:44.39 +61:45:35.6
02:37:50.65 +57:54:15.4
02:32:40.32 +62:07:15.6
02:03:07.41 +57:18:14.7
02:19:36.15 +64:09:18.0
02:31:46.25 +55:57:57.3
00:41:52.39 +59:10:02.9
02:33:23.67 +64:25:00.1
01:52:19.54 +57:19:07.3
01:41:34.22 +56:56:31.6
02:31:18.98 +56:20:50.6
02:24:19.74 +63:24:35.5
02:43:55.93 +64:48:54.7
01:45:16.05 +57:55:46.8
02:13:47.58 +63:11:26.0
02:19:59.14 +59:17:32.1
01:56:16.77 +62:11:52.2
01:02:09.20 +57:21:42.2
02:07:37.49 +62:22:07.0
02:07:21.55 +64:28:11.9
01:23:28.70 +62:35:10.1
02:16:28.46 +58:16:12.0
01:46:05.47 +60:59:36.6
01:43:45.28 +58:23:45.8
02:41:04.44 +62:17:31.5
01:35:57.20 +59:47:27.0
01:36:47.30 +63:02:42.6
01:37:01.41 +61:15:57.1
02:43:44.79 +60:40:26.6
01:13:09.77 +64:46:43.6
01:25:56.70 +62:14:49.4
02:30:58.99 +62:56:15.2
02:18:22.56 +58:47:09.8
01:35:09.89 +60:17:10.6
###################################################################################
02:01:28.10 +58:18:15.0 -- not an asteroid (will add it to exclusion list)
02:00:57.02 +58:36:59.3 -- not an asteroid (will add it to exclusion list)
01:16:12.04 +59:15:22.9 -- not an asteroid (will add it to exclusion list)
02:03:23.58 +57:43:21.9 -- not an asteroid (will add it to exclusion list)
01:23:00.77 +64:39:24.1 -- not an asteroid (will add it to exclusion list)
01:56:38.06 +59:15:34.2 -- not an asteroid (will add it to exclusion list)
01:43:36.46 +58:48:08.9 -- not an asteroid (will add it to exclusion list)
01:29:35.29 +65:02:04.9 -- not an asteroid (will add it to exclusion list)
02:21:40.62 +60:54:41.8 -- not an asteroid (will add it to exclusion list)
01:43:02.78 +61:34:06.4 -- not an asteroid (will add it to exclusion list)
00:51:08.53 +64:31:35.6 -- not an asteroid (will add it to exclusion list)
02:00:14.31 +65:03:58.2 -- not an asteroid (will add it to exclusion list)
01:02:16.17 +57:08:41.8 -- not an asteroid (will add it to exclusion list)
01:25:39.69 +59:16:07.4 -- not an asteroid (will add it to exclusion list)
02:19:45.31 +57:01:15.4 -- not an asteroid (will add it to exclusion list)
01:46:35.86 +59:12:14.3 -- not an asteroid (will add it to exclusion list)
02:03:11.16 +62:07:52.0 -- not an asteroid (will add it to exclusion list)
00:36:55.23 +62:40:46.4 -- not an asteroid (will add it to exclusion list)
00:51:15.99 +58:39:34.3 -- not an asteroid (will add it to exclusion list)
02:25:27.64 +56:46:55.8 -- not an asteroid (will add it to exclusion list)
02:29:09.02 +56:37:12.7 -- not an asteroid (will add it to exclusion list)
02:18:53.85 +57:08:41.8 -- not an asteroid (will add it to exclusion list)
02:32:05.67 +56:39:57.3 -- not an asteroid (will add it to exclusion list)
02:27:58.38 +56:02:38.8 -- not an asteroid (will add it to exclusion list)
02:31:26.37 +55:59:07.4 -- not an asteroid (will add it to exclusion list)
02:29:10.08 +56:27:14.1 -- not an asteroid (will add it to exclusion list)
02:34:11.11 +55:49:59.2 -- not an asteroid (will add it to exclusion list)
02:35:38.10 +57:29:11.6 -- not an asteroid (will add it to exclusion list)
02:30:54.10 +56:14:28.3 -- not an asteroid (will add it to exclusion list)
02:27:24.36 +56:23:03.5 -- not an asteroid (will add it to exclusion list)
02:32:05.62 +57:22:03.9 -- not an asteroid (will add it to exclusion list)
02:32:46.69 +56:48:22.9 -- not an asteroid (will add it to exclusion list)
02:34:35.28 +56:21:51.3 -- not an asteroid (will add it to exclusion list)
02:34:44.75 +56:06:07.7 -- not an asteroid (will add it to exclusion list)
02:33:35.26 +55:54:24.6 -- not an asteroid (will add it to exclusion list)
02:37:08.74 +57:25:19.6 -- not an asteroid (will add it to exclusion list)
02:36:33.17 +57:54:38.3 -- not an asteroid (will add it to exclusion list)
02:27:20.52 +56:01:48.8 -- not an asteroid (will add it to exclusion list)
02:31:26.05 +56:07:04.8 -- not an asteroid (will add it to exclusion list)
02:35:52.05 +57:47:21.5 -- not an asteroid (will add it to exclusion list)
02:26:59.10 +56:01:58.1 -- not an asteroid (will add it to exclusion list)
02:32:16.04 +56:38:48.1 -- not an asteroid (will add it to exclusion list)
02:24:11.88 +56:35:43.2 -- not an asteroid (will add it to exclusion list)
02:36:29.15 +57:11:43.0 -- not an asteroid (will add it to exclusion list)
02:33:01.83 +57:02:06.6 -- not an asteroid (will add it to exclusion list)
02:21:16.42 +57:08:40.1 -- not an asteroid (will add it to exclusion list)
02:34:06.21 +56:25:27.6 -- not an asteroid (will add it to exclusion list)
02:36:36.23 +57:46:58.2 -- not an asteroid (will add it to exclusion list)
02:20:54.00 +56:16:37.9 -- not an asteroid (will add it to exclusion list)
02:29:12.20 +56:18:00.7 -- not an asteroid (will add it to exclusion list)
02:22:35.24 +56:18:15.4 -- not an asteroid (will add it to exclusion list)
02:32:55.76 +56:39:38.1 -- not an asteroid (will add it to exclusion list)
02:30:44.92 +56:56:13.4 -- not an asteroid (will add it to exclusion list)
02:37:36.90 +57:51:16.6 -- not an asteroid (will add it to exclusion list)
02:21:55.26 +56:25:09.3 -- not an asteroid (will add it to exclusion list)
02:28:50.68 +56:20:50.4 -- not an asteroid (will add it to exclusion list)
02:31:06.61 +56:30:44.0 -- not an asteroid (will add it to exclusion list)
02:30:12.73 +56:11:27.6 -- not an asteroid (will add it to exclusion list)
02:24:41.97 +56:55:48.3 -- not an asteroid (will add it to exclusion list)
02:31:11.88 +57:09:48.4 -- not an asteroid (will add it to exclusion list)
02:35:34.11 +57:09:17.2 -- not an asteroid (will add it to exclusion list)
02:37:55.13 +57:39:02.3 -- not an asteroid (will add it to exclusion list)
02:27:07.81 +56:33:54.6 -- not an asteroid (will add it to exclusion list)
02:38:46.94 +57:49:57.0 -- not an asteroid (will add it to exclusion list)
02:25:28.20 +56:11:20.2 -- not an asteroid (will add it to exclusion list)
02:34:04.70 +56:30:40.2 -- not an asteroid (will add it to exclusion list)
02:25:34.10 +56:34:22.3 -- not an asteroid (will add it to exclusion list)
02:32:45.29 +57:08:07.3 -- not an asteroid (will add it to exclusion list)
02:31:38.17 +56:33:35.0 -- not an asteroid (will add it to exclusion list)
02:32:05.15 +56:49:22.4 -- not an asteroid (will add it to exclusion list)
02:22:10.11 +56:24:22.8 -- not an asteroid (will add it to exclusion list)
02:30:51.88 +57:04:10.0 -- not an asteroid (will add it to exclusion list)
02:25:20.49 +56:12:13.5 -- not an asteroid (will add it to exclusion list)
02:19:52.90 +56:15:39.2 -- not an asteroid (will add it to exclusion list)
02:33:49.42 +57:35:11.7 -- not an asteroid (will add it to exclusion list)
02:33:29.99 +57:42:17.0 -- not an asteroid (will add it to exclusion list)
02:31:38.51 +57:13:48.2 -- not an asteroid (will add it to exclusion list)
02:33:48.99 +57:01:45.0 -- not an asteroid (will add it to exclusion list)
02:24:06.55 +56:30:01.1 -- not an asteroid (will add it to exclusion list)
02:36:56.79 +57:06:43.6 -- not an asteroid (will add it to exclusion list)
02:31:18.98 +55:53:51.0 -- not an asteroid (will add it to exclusion list)
02:24:09.75 +56:34:02.5 -- not an asteroid (will add it to exclusion list)
02:37:31.97 +57:28:17.7 -- not an asteroid (will add it to exclusion list)
00:52:30.58 +59:43:27.9 -- not an asteroid (will add it to exclusion list)
02:30:37.35 +56:23:01.5 -- not an asteroid (will add it to exclusion list)
02:36:19.99 +57:15:26.8 -- not an asteroid (will add it to exclusion list)
02:35:18.58 +57:31:37.0 -- not an asteroid (will add it to exclusion list)
02:32:18.76 +56:21:25.6 -- not an asteroid (will add it to exclusion list)
02:21:59.04 +56:30:02.2 -- not an asteroid (will add it to exclusion list)
02:22:31.60 +56:14:10.7 -- not an asteroid (will add it to exclusion list)
02:30:30.72 +57:30:28.2 -- not an asteroid (will add it to exclusion list)
02:36:08.67 +57:39:33.5 -- not an asteroid (will add it to exclusion list)
02:22:04.64 +57:10:39.2 -- not an asteroid (will add it to exclusion list)
02:33:05.67 +56:13:01.3 -- not an asteroid (will add it to exclusion list)
02:27:33.00 +56:13:09.5 -- not an asteroid (will add it to exclusion list)
02:31:59.20 +56:42:22.0 -- not an asteroid (will add it to exclusion list)
02:26:07.28 +56:25:11.5 -- not an asteroid (will add it to exclusion list)
02:36:35.17 +57:36:34.3 -- not an asteroid (will add it to exclusion list)
02:35:20.47 +57:29:29.4 -- not an asteroid (will add it to exclusion list)
02:37:41.05 +57:33:20.1 -- not an asteroid (will add it to exclusion list)
02:30:49.77 +56:11:02.6 -- not an asteroid (will add it to exclusion list)
00:57:05.28 +57:30:11.8 -- not an asteroid (will add it to exclusion list)
02:30:33.01 +56:53:08.7 -- not an asteroid (will add it to exclusion list)
02:19:44.52 +56:42:25.7 -- not an asteroid (will add it to exclusion list)
02:21:04.81 +56:15:32.5 -- not an asteroid (will add it to exclusion list)
02:26:13.37 +56:36:45.1 -- not an asteroid (will add it to exclusion list)
02:29:33.40 +55:57:20.3 -- not an asteroid (will add it to exclusion list)
02:36:22.57 +57:40:03.4 -- not an asteroid (will add it to exclusion list)
02:33:09.48 +57:00:39.2 -- not an asteroid (will add it to exclusion list)
02:29:50.72 +56:19:10.9 -- not an asteroid (will add it to exclusion list)
02:29:41.24 +56:20:06.8 -- not an asteroid (will add it to exclusion list)
02:28:09.92 +56:10:50.3 -- not an asteroid (will add it to exclusion list)
02:34:26.97 +56:29:12.2 -- not an asteroid (will add it to exclusion list)
02:31:06.05 +56:37:19.1 -- not an asteroid (will add it to exclusion list)
02:40:07.39 +58:29:00.9 -- not an asteroid (will add it to exclusion list)
02:35:08.80 +57:36:14.7 -- not an asteroid (will add it to exclusion list)
02:34:05.16 +56:42:26.1 -- not an asteroid (will add it to exclusion list)
02:32:26.23 +56:47:10.1 -- not an asteroid (will add it to exclusion list)
02:33:13.67 +57:44:32.4 -- not an asteroid (will add it to exclusion list)
02:30:52.97 +56:54:21.1 -- not an asteroid (will add it to exclusion list)
02:29:40.98 +56:18:42.4 -- not an asteroid (will add it to exclusion list)
02:35:43.04 +56:44:19.4 -- not an asteroid (will add it to exclusion list)
02:32:59.22 +57:28:35.8 -- not an asteroid (will add it to exclusion list)
02:28:41.20 +56:12:06.5 -- not an asteroid (will add it to exclusion list)
02:18:24.04 +56:23:24.4 -- not an asteroid (will add it to exclusion list)
02:29:57.20 +56:36:49.0 -- not an asteroid (will add it to exclusion list)
02:29:58.23 +56:08:53.2 -- not an asteroid (will add it to exclusion list)
02:35:04.79 +57:26:52.8 -- not an asteroid (will add it to exclusion list)
02:19:36.25 +56:23:22.4 -- not an asteroid (will add it to exclusion list)
02:31:28.99 +57:11:53.7 -- not an asteroid (will add it to exclusion list)
02:37:50.62 +57:45:48.2 -- not an asteroid (will add it to exclusion list)
02:29:28.85 +56:33:09.5 -- not an asteroid (will add it to exclusion list)
02:29:39.44 +56:11:35.3 -- not an asteroid (will add it to exclusion list)
02:26:43.32 +56:24:14.7 -- not an asteroid (will add it to exclusion list)
02:29:59.81 +56:13:02.8 -- not an asteroid (will add it to exclusion list)
02:21:34.70 +56:26:46.5 -- not an asteroid (will add it to exclusion list)
02:31:09.60 +57:16:15.9 -- not an asteroid (will add it to exclusion list)
02:26:55.68 +56:30:21.4 -- not an asteroid (will add it to exclusion list)
02:35:30.33 +57:03:27.8 -- not an asteroid (will add it to exclusion list)
02:28:49.65 +56:07:39.2 -- not an asteroid (will add it to exclusion list)
02:26:10.82 +56:48:29.2 -- not an asteroid (will add it to exclusion list)
02:32:17.90 +57:17:10.0 -- not an asteroid (will add it to exclusion list)
02:34:24.43 +57:28:27.5 -- not an asteroid (will add it to exclusion list)
02:31:51.85 +56:45:48.0 -- not an asteroid (will add it to exclusion list)
02:25:42.03 +56:37:15.5 -- not an asteroid (will add it to exclusion list)
02:36:59.24 +57:56:30.4 -- not an asteroid (will add it to exclusion list)
02:33:03.14 +57:03:26.9 -- not an asteroid (will add it to exclusion list)
02:36:07.89 +57:21:40.2 -- not an asteroid (will add it to exclusion list)
02:20:24.36 +56:41:46.0 -- not an asteroid (will add it to exclusion list)
02:20:07.34 +56:27:53.6 -- not an asteroid (will add it to exclusion list)
02:26:02.45 +56:20:59.5 -- not an asteroid (will add it to exclusion list)
02:26:00.91 +56:46:18.9 -- not an asteroid (will add it to exclusion list)
02:33:37.63 +57:40:23.9 -- not an asteroid (will add it to exclusion list)
02:24:52.65 +56:43:13.3 -- not an asteroid (will add it to exclusion list)
02:40:00.93 +58:49:46.1 -- not an asteroid (will add it to exclusion list)
02:38:18.56 +57:37:39.8 -- not an asteroid (will add it to exclusion list)
02:27:22.97 +56:19:26.0 -- not an asteroid (will add it to exclusion list)
02:25:30.00 +56:16:55.3 -- not an asteroid (will add it to exclusion list)
02:30:16.58 +56:38:11.3 -- not an asteroid (will add it to exclusion list)
01:22:23.94 +61:13:51.2 -- not an asteroid (will add it to exclusion list)
00:52:12.67 +64:57:20.9 -- not an asteroid (will add it to exclusion list)
01:38:21.64 +57:13:51.3 -- not an asteroid (will add it to exclusion list)
01:50:36.43 +63:53:30.1 -- not an asteroid (will add it to exclusion list)
02:41:50.08 +65:30:27.2 -- not an asteroid (will add it to exclusion list)
02:09:48.70 +59:51:47.0 -- not an asteroid (will add it to exclusion list)
01:31:28.19 +57:20:36.7 -- not an asteroid (will add it to exclusion list)
02:24:46.68 +59:43:52.9 -- not an asteroid (will add it to exclusion list)
02:48:49.52 +64:11:51.9 -- not an asteroid (will add it to exclusion list)
01:12:18.51 +60:20:30.2 -- not an asteroid (will add it to exclusion list)
02:15:20.43 +62:13:50.0 -- not an asteroid (will add it to exclusion list)
02:05:05.77 +58:16:24.6 -- not an asteroid (will add it to exclusion list)
02:24:05.02 +63:37:15.8 -- not an asteroid (will add it to exclusion list)
01:15:48.97 +62:13:51.2 -- not an asteroid (will add it to exclusion list)
01:22:16.36 +57:23:06.8 -- not an asteroid (will add it to exclusion list)
01:54:12.35 +65:38:24.8 -- not an asteroid (will add it to exclusion list)
02:14:27.98 +64:44:14.9 -- not an asteroid (will add it to exclusion list)
01:21:54.86 +61:20:56.1 -- not an asteroid (will add it to exclusion list)
02:39:22.81 +60:42:41.0 -- not an asteroid (will add it to exclusion list)
01:57:52.45 +64:34:23.0 -- not an asteroid (will add it to exclusion list)
02:34:40.00 +63:00:03.4 -- not an asteroid (will add it to exclusion list)
02:25:13.42 +56:30:32.3 -- not an asteroid (will add it to exclusion list)
02:19:04.00 +62:47:33.4 -- not an asteroid (will add it to exclusion list)
02:15:35.96 +56:21:40.4 -- not an asteroid (will add it to exclusion list)
01:47:43.89 +62:06:37.4 -- not an asteroid (will add it to exclusion list)
02:31:25.66 +60:43:53.6 -- not an asteroid (will add it to exclusion list)
02:45:57.12 +62:02:43.5 -- not an asteroid (will add it to exclusion list)
02:07:48.46 +61:22:16.5 -- not an asteroid (will add it to exclusion list)
02:36:10.97 +60:22:42.0 -- not an asteroid (will add it to exclusion list)
01:23:04.06 +57:36:35.9 -- not an asteroid (will add it to exclusion list)
02:24:29.68 +59:24:31.5 -- not an asteroid (will add it to exclusion list)
01:43:58.28 +58:41:06.0 -- not an asteroid (will add it to exclusion list)
01:36:21.66 +60:26:52.3 -- not an asteroid (will add it to exclusion list)
02:05:50.44 +62:42:31.3 -- not an asteroid (will add it to exclusion list)
02:08:54.01 +58:42:29.5 -- not an asteroid (will add it to exclusion list)
02:31:46.08 +56:26:43.2 -- not an asteroid (will add it to exclusion list)
02:19:12.27 +57:48:50.2 -- not an asteroid (will add it to exclusion list)
02:11:32.08 +65:25:28.2 -- not an asteroid (will add it to exclusion list)
02:24:34.96 +61:05:35.0 -- not an asteroid (will add it to exclusion list)
02:11:34.44 +59:06:06.6 -- not an asteroid (will add it to exclusion list)
02:24:19.53 +64:16:12.9 -- not an asteroid (will add it to exclusion list)
02:19:16.53 +59:42:22.1 -- not an asteroid (will add it to exclusion list)
01:41:01.13 +61:31:00.7 -- not an asteroid (will add it to exclusion list)
02:09:24.81 +60:03:15.6 -- not an asteroid (will add it to exclusion list)
02:01:05.84 +58:11:26.9 -- not an asteroid (will add it to exclusion list)
01:56:15.73 +60:01:03.3 -- not an asteroid (will add it to exclusion list)
02:24:41.13 +58:22:35.6 -- not an asteroid (will add it to exclusion list)
02:20:33.64 +60:06:16.7 -- not an asteroid (will add it to exclusion list)
01:27:44.43 +62:06:40.7 -- not an asteroid (will add it to exclusion list)
02:03:34.92 +64:11:47.7 -- not an asteroid (will add it to exclusion list)
01:41:46.93 +59:03:48.0 -- not an asteroid (will add it to exclusion list)
02:28:12.08 +64:31:52.8 -- not an asteroid (will add it to exclusion list)
01:32:27.26 +60:20:31.1 -- not an asteroid (will add it to exclusion list)
01:54:09.12 +61:13:07.0 -- not an asteroid (will add it to exclusion list)
01:36:20.44 +58:31:43.2 -- not an asteroid (will add it to exclusion list)
01:40:46.01 +60:51:39.7 -- not an asteroid (will add it to exclusion list)
01:25:43.43 +60:50:05.7 -- not an asteroid (will add it to exclusion list)
01:16:28.97 +60:14:00.5 -- not an asteroid (will add it to exclusion list)
02:14:45.13 +57:39:36.6 -- not an asteroid (will add it to exclusion list)
02:28:12.53 +58:37:11.5 -- not an asteroid (will add it to exclusion list)
02:14:26.77 +64:29:24.6 -- not an asteroid (will add it to exclusion list)
02:15:26.81 +62:47:45.7 -- not an asteroid (will add it to exclusion list)
02:33:31.95 +57:34:09.2 -- not an asteroid (will add it to exclusion list)
01:26:01.01 +59:55:35.7 -- not an asteroid (will add it to exclusion list)
02:07:46.89 +62:11:10.9 -- not an asteroid (will add it to exclusion list)
01:55:07.62 +62:47:31.4 -- not an asteroid (will add it to exclusion list)
02:33:47.87 +61:42:03.3 -- not an asteroid (will add it to exclusion list)
02:34:32.44 +64:22:56.6 -- not an asteroid (will add it to exclusion list)
02:23:38.25 +61:24:57.1 -- not an asteroid (will add it to exclusion list)
01:47:07.73 +57:00:34.1 -- not an asteroid (will add it to exclusion list)
01:47:21.78 +58:08:40.5 -- not an asteroid (will add it to exclusion list)
01:39:46.89 +59:42:30.5 -- not an asteroid (will add it to exclusion list)
01:44:48.84 +59:53:34.1 -- not an asteroid (will add it to exclusion list)
01:04:58.46 +60:30:20.5 -- not an asteroid (will add it to exclusion list)
01:09:49.42 +65:08:28.8 -- not an asteroid (will add it to exclusion list)
02:22:32.05 +64:22:11.7 -- not an asteroid (will add it to exclusion list)
01:11:51.39 +58:59:24.6 -- not an asteroid (will add it to exclusion list)
02:18:24.73 +58:37:25.8 -- not an asteroid (will add it to exclusion list)
01:57:53.16 +63:48:41.1 -- not an asteroid (will add it to exclusion list)
02:12:24.62 +63:16:01.2 -- not an asteroid (will add it to exclusion list)
02:42:10.42 +61:03:22.2 -- not an asteroid (will add it to exclusion list)
02:19:34.19 +58:23:57.9 -- not an asteroid (will add it to exclusion list)
01:01:19.84 +58:00:01.2 -- not an asteroid (will add it to exclusion list)
01:16:04.83 +58:33:49.3 -- not an asteroid (will add it to exclusion list)
01:24:30.64 +59:38:48.6 -- not an asteroid (will add it to exclusion list)
02:00:17.58 +57:43:39.7 -- not an asteroid (will add it to exclusion list)
01:17:41.64 +59:18:24.2 -- not an asteroid (will add it to exclusion list)
02:13:08.99 +63:06:22.8 -- not an asteroid (will add it to exclusion list)
02:07:16.67 +60:08:10.8 -- not an asteroid (will add it to exclusion list)
02:33:40.04 +57:40:02.5 -- not an asteroid (will add it to exclusion list)
01:30:50.42 +60:32:14.2 -- not an asteroid (will add it to exclusion list)
01:09:38.03 +59:05:13.6 -- not an asteroid (will add it to exclusion list)
02:27:23.77 +60:40:47.8 -- not an asteroid (will add it to exclusion list)
01:54:28.56 +57:17:51.0 -- not an asteroid (will add it to exclusion list)
01:23:02.01 +61:59:41.5 -- not an asteroid (will add it to exclusion list)
01:14:57.02 +59:42:13.2 -- not an asteroid (will add it to exclusion list)
01:49:47.69 +65:03:21.3 -- not an asteroid (will add it to exclusion list)
01:18:52.86 +58:09:31.4 -- not an asteroid (will add it to exclusion list)
02:08:15.60 +59:15:57.1 -- not an asteroid (will add it to exclusion list)
02:27:21.83 +62:38:26.5 -- not an asteroid (will add it to exclusion list)
02:14:46.56 +57:37:03.4 -- not an asteroid (will add it to exclusion list)
02:34:06.44 +56:37:23.7 -- not an asteroid (will add it to exclusion list)
01:10:29.41 +57:08:53.0 -- not an asteroid (will add it to exclusion list)
01:01:55.32 +59:00:14.3 -- not an asteroid (will add it to exclusion list)
01:21:36.46 +63:33:51.0 -- not an asteroid (will add it to exclusion list)
01:23:21.85 +60:18:14.4 -- not an asteroid (will add it to exclusion list)
02:23:18.51 +64:21:47.0 -- not an asteroid (will add it to exclusion list)
02:21:20.02 +61:23:53.5 -- not an asteroid (will add it to exclusion list)
02:38:33.43 +61:54:31.0 -- not an asteroid (will add it to exclusion list)
01:20:18.43 +64:28:04.9 -- not an asteroid (will add it to exclusion list)
01:36:43.18 +61:14:25.3 -- not an asteroid (will add it to exclusion list)
02:00:13.56 +60:43:20.6 -- not an asteroid (will add it to exclusion list)
01:20:05.35 +59:00:13.2 -- not an asteroid (will add it to exclusion list)
00:58:01.37 +59:33:23.2 -- not an asteroid (will add it to exclusion list)
01:51:45.69 +65:36:52.8 -- not an asteroid (will add it to exclusion list)
01:28:36.28 +61:12:06.7 -- not an asteroid (will add it to exclusion list)
02:02:39.14 +59:22:44.0 -- not an asteroid (will add it to exclusion list)
02:03:00.34 +58:36:13.4 -- not an asteroid (will add it to exclusion list)
01:31:04.89 +57:13:14.0 -- not an asteroid (will add it to exclusion list)
01:04:09.24 +61:46:55.9 -- not an asteroid (will add it to exclusion list)
01:32:44.39 +61:45:35.6 -- not an asteroid (will add it to exclusion list)
02:37:50.65 +57:54:15.4 -- not an asteroid (will add it to exclusion list)
02:32:40.32 +62:07:15.6 -- not an asteroid (will add it to exclusion list)
02:03:07.41 +57:18:14.7 -- not an asteroid (will add it to exclusion list)
02:19:36.15 +64:09:18.0 -- not an asteroid (will add it to exclusion list)
02:31:46.25 +55:57:57.3 -- not an asteroid (will add it to exclusion list)
00:41:52.39 +59:10:02.9 -- not an asteroid (will add it to exclusion list)
02:33:23.67 +64:25:00.1 -- not an asteroid (will add it to exclusion list)
01:52:19.54 +57:19:07.3 -- not an asteroid (will add it to exclusion list)
01:41:34.22 +56:56:31.6 -- not an asteroid (will add it to exclusion list)
02:31:18.98 +56:20:50.6 -- not an asteroid (will add it to exclusion list)
02:24:19.74 +63:24:35.5 -- not an asteroid (will add it to exclusion list)
02:43:55.93 +64:48:54.7 -- not an asteroid (will add it to exclusion list)
01:45:16.05 +57:55:46.8 -- not an asteroid (will add it to exclusion list)
02:13:47.58 +63:11:26.0 -- not an asteroid (will add it to exclusion list)
02:19:59.14 +59:17:32.1 -- not an asteroid (will add it to exclusion list)
01:56:16.77 +62:11:52.2 -- not an asteroid (will add it to exclusion list)
01:02:09.20 +57:21:42.2 -- not an asteroid (will add it to exclusion list)
02:07:37.49 +62:22:07.0 -- not an asteroid (will add it to exclusion list)
02:07:21.55 +64:28:11.9 -- not an asteroid (will add it to exclusion list)
01:23:28.70 +62:35:10.1 -- not an asteroid (will add it to exclusion list)
02:16:28.46 +58:16:12.0 -- not an asteroid (will add it to exclusion list)
01:46:05.47 +60:59:36.6 -- not an asteroid (will add it to exclusion list)
01:43:45.28 +58:23:45.8 -- not an asteroid (will add it to exclusion list)
02:41:04.44 +62:17:31.5 -- not an asteroid (will add it to exclusion list)
01:35:57.20 +59:47:27.0 -- not an asteroid (will add it to exclusion list)
01:36:47.30 +63:02:42.6 -- not an asteroid (will add it to exclusion list)
01:37:01.41 +61:15:57.1 -- not an asteroid (will add it to exclusion list)
02:43:44.79 +60:40:26.6 -- not an asteroid (will add it to exclusion list)
01:13:09.77 +64:46:43.6 -- not an asteroid (will add it to exclusion list)
01:25:56.70 +62:14:49.4 -- not an asteroid (will add it to exclusion list)
02:30:58.99 +62:56:15.2 -- not an asteroid (will add it to exclusion list)
02:18:22.56 +58:47:09.8 -- not an asteroid (will add it to exclusion list)
01:35:09.89 +60:17:10.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:36:55.23 +62:40:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:52.39 +59:10:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:08.53 +64:31:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:15.99 +58:39:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:12.67 +64:57:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:30.58 +59:43:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:57:05.28 +57:30:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:58:01.37 +59:33:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:19.84 +58:00:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:55.32 +59:00:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:09.20 +57:21:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:16.17 +57:08:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:04:09.24 +61:46:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:04:58.46 +60:30:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:38.03 +59:05:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:49.42 +65:08:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:29.41 +57:08:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:51.39 +58:59:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:18.51 +60:20:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:09.77 +64:46:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:57.02 +59:42:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:48.97 +62:13:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:04.83 +58:33:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:12.04 +59:15:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:28.97 +60:14:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:41.64 +59:18:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:52.86 +58:09:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:05.35 +59:00:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:18.43 +64:28:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:36.46 +63:33:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:54.86 +61:20:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:16.36 +57:23:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:23.94 +61:13:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:00.77 +64:39:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:02.01 +61:59:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:04.06 +57:36:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:21.85 +60:18:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:28.70 +62:35:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:30.64 +59:38:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:39.69 +59:16:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:43.43 +60:50:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:56.70 +62:14:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:01.01 +59:55:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:44.43 +62:06:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:36.28 +61:12:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:35.29 +65:02:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:50.42 +60:32:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:04.89 +57:13:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:28.19 +57:20:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:27.26 +60:20:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:44.39 +61:45:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:09.89 +60:17:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:57.20 +59:47:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:20.44 +58:31:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:21.66 +60:26:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:43.18 +61:14:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:47.30 +63:02:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:01.41 +61:15:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:21.64 +57:13:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:46.89 +59:42:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:46.01 +60:51:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:01.13 +61:31:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:34.22 +56:56:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:46.93 +59:03:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:02.78 +61:34:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:36.46 +58:48:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:45.28 +58:23:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:58.28 +58:41:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:48.84 +59:53:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:16.05 +57:55:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:05.47 +60:59:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:35.86 +59:12:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:07.73 +57:00:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:21.78 +58:08:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:43.89 +62:06:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:47.69 +65:03:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:36.43 +63:53:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:45.69 +65:36:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:19.54 +57:19:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:09.12 +61:13:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:12.35 +65:38:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:28.56 +57:17:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:07.62 +62:47:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:15.73 +60:01:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:16.77 +62:11:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:38.06 +59:15:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:52.45 +64:34:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:53.16 +63:48:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:13.56 +60:43:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:14.31 +65:03:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:17.58 +57:43:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:57.02 +58:36:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:05.84 +58:11:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:28.10 +58:18:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:39.14 +59:22:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:00.34 +58:36:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:07.41 +57:18:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:11.16 +62:07:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:23.58 +57:43:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:34.92 +64:11:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:05.77 +58:16:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:50.44 +62:42:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:16.67 +60:08:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:21.55 +64:28:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:37.49 +62:22:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:46.89 +62:11:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:48.46 +61:22:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:15.60 +59:15:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:54.01 +58:42:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:24.81 +60:03:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:48.70 +59:51:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:32.08 +65:25:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:34.44 +59:06:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:24.62 +63:16:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:08.99 +63:06:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:47.58 +63:11:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:26.77 +64:29:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:27.98 +64:44:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:45.13 +57:39:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:46.56 +57:37:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:20.43 +62:13:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:26.81 +62:47:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:35.96 +56:21:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:28.46 +58:16:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:22.56 +58:47:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:24.04 +56:23:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:24.73 +58:37:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:53.85 +57:08:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:04.00 +62:47:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:12.27 +57:48:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:16.53 +59:42:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:34.19 +58:23:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:36.15 +64:09:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:36.25 +56:23:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:44.52 +56:42:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:45.31 +57:01:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:52.90 +56:15:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:59.14 +59:17:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:07.34 +56:27:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:24.36 +56:41:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:33.64 +60:06:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:54.00 +56:16:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:04.81 +56:15:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:16.42 +57:08:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:20.02 +61:23:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:34.70 +56:26:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:40.62 +60:54:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:55.26 +56:25:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:59.04 +56:30:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:04.64 +57:10:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:10.11 +56:24:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:31.60 +56:14:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:32.05 +64:22:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:35.24 +56:18:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:18.51 +64:21:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:38.25 +61:24:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:05.02 +63:37:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:06.55 +56:30:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:09.75 +56:34:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:11.88 +56:35:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:19.53 +64:16:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:19.74 +63:24:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:29.68 +59:24:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:34.96 +61:05:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:41.13 +58:22:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:41.97 +56:55:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:46.68 +59:43:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:52.65 +56:43:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:13.42 +56:30:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:20.49 +56:12:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:27.64 +56:46:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:28.20 +56:11:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:30.00 +56:16:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:34.10 +56:34:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:42.03 +56:37:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:00.91 +56:46:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:02.45 +56:20:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:07.28 +56:25:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:10.82 +56:48:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:13.37 +56:36:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:43.32 +56:24:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:55.68 +56:30:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:59.10 +56:01:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:07.81 +56:33:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:20.52 +56:01:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:21.83 +62:38:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:22.97 +56:19:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:23.77 +60:40:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:24.36 +56:23:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:33.00 +56:13:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:58.38 +56:02:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:09.92 +56:10:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:12.08 +64:31:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:12.53 +58:37:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:41.20 +56:12:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:49.65 +56:07:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:50.68 +56:20:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:09.02 +56:37:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:10.08 +56:27:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:12.20 +56:18:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:28.85 +56:33:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:33.40 +55:57:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:39.44 +56:11:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:40.98 +56:18:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:41.24 +56:20:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:50.72 +56:19:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:57.20 +56:36:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:58.23 +56:08:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:59.81 +56:13:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:12.73 +56:11:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:16.58 +56:38:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:30.72 +57:30:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:33.01 +56:53:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:37.35 +56:23:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:44.92 +56:56:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:49.77 +56:11:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:51.88 +57:04:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:52.97 +56:54:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:54.10 +56:14:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:58.99 +62:56:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:06.05 +56:37:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:06.61 +56:30:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:09.60 +57:16:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:11.88 +57:09:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:18.98 +55:53:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:18.98 +56:20:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:25.66 +60:43:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:26.05 +56:07:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:26.37 +55:59:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:28.99 +57:11:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:38.17 +56:33:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:38.51 +57:13:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:46.08 +56:26:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:46.25 +55:57:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:51.85 +56:45:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:59.20 +56:42:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:05.15 +56:49:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:05.62 +57:22:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:05.67 +56:39:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:16.04 +56:38:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:17.90 +57:17:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:18.76 +56:21:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:26.23 +56:47:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:40.32 +62:07:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:45.29 +57:08:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:46.69 +56:48:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:55.76 +56:39:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:59.22 +57:28:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:01.83 +57:02:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:03.14 +57:03:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:05.67 +56:13:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:09.48 +57:00:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:13.67 +57:44:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:23.67 +64:25:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:29.99 +57:42:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:31.95 +57:34:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:35.26 +55:54:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:37.63 +57:40:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:40.04 +57:40:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:47.87 +61:42:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:48.99 +57:01:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:49.42 +57:35:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:04.70 +56:30:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:05.16 +56:42:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:06.21 +56:25:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:06.44 +56:37:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:11.11 +55:49:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:24.43 +57:28:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:26.97 +56:29:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:32.44 +64:22:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:35.28 +56:21:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:40.00 +63:00:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:44.75 +56:06:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:04.79 +57:26:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:08.80 +57:36:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:18.58 +57:31:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:20.47 +57:29:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:30.33 +57:03:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:34.11 +57:09:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:38.10 +57:29:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:43.04 +56:44:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:52.05 +57:47:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:07.89 +57:21:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:08.67 +57:39:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:10.97 +60:22:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:19.99 +57:15:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:22.57 +57:40:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:29.15 +57:11:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:33.17 +57:54:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:35.17 +57:36:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:36.23 +57:46:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:56.79 +57:06:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:59.24 +57:56:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:08.74 +57:25:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:31.97 +57:28:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:36.90 +57:51:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:41.05 +57:33:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:50.62 +57:45:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:50.65 +57:54:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:55.13 +57:39:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:18.56 +57:37:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:33.43 +61:54:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:46.94 +57:49:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:39:22.81 +60:42:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:40:00.93 +58:49:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:40:07.39 +58:29:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:41:04.44 +62:17:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:41:50.08 +65:30:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:42:10.42 +61:03:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:43:44.79 +60:40:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:43:55.93 +64:48:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:45:57.12 +62:02:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:48:49.52 +64:11:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:36:55.23 +62:40:46.4 -- not a known variable star
00:41:52.39 +59:10:02.9 -- a known variable star
00:51:08.53 +64:31:35.6 -- not a known variable star
00:51:15.99 +58:39:34.3 -- not a known variable star
00:52:12.67 +64:57:20.9 -- not a known variable star
00:52:30.58 +59:43:27.9 -- not a known variable star
00:57:05.28 +57:30:11.8 -- a known variable star
00:58:01.37 +59:33:23.2 -- a known variable star
01:01:19.84 +58:00:01.2 -- a known variable star
01:01:55.32 +59:00:14.3 -- a known variable star
01:02:09.20 +57:21:42.2 -- a known variable star
01:02:16.17 +57:08:41.8 -- not a known variable star
01:04:09.24 +61:46:55.9 -- not a known variable star
01:04:58.46 +60:30:20.5 -- a known variable star
01:09:38.03 +59:05:13.6 -- a known variable star
01:09:49.42 +65:08:28.8 -- a known variable star
01:10:29.41 +57:08:53.0 -- a known variable star
01:11:51.39 +58:59:24.6 -- a known variable star
01:12:18.51 +60:20:30.2 -- a known variable star
01:13:09.77 +64:46:43.6 -- a known variable star
01:14:57.02 +59:42:13.2 -- a known variable star
01:15:48.97 +62:13:51.2 -- a known variable star
01:16:04.83 +58:33:49.3 -- a known variable star
01:16:12.04 +59:15:22.9 -- a known variable star
01:16:28.97 +60:14:00.5 -- a known variable star
01:17:41.64 +59:18:24.2 -- a known variable star
01:18:52.86 +58:09:31.4 -- a known variable star
01:20:05.35 +59:00:13.2 -- a known variable star
01:20:18.43 +64:28:04.9 -- a known variable star
01:21:36.46 +63:33:51.0 -- a known variable star
01:21:54.86 +61:20:56.1 -- a known variable star
01:22:16.36 +57:23:06.8 -- a known variable star
01:22:23.94 +61:13:51.2 -- a known variable star
01:23:00.77 +64:39:24.1 -- a known variable star
01:23:02.01 +61:59:41.5 -- not a known variable star
01:23:04.06 +57:36:35.9 -- a known variable star
01:23:21.85 +60:18:14.4 -- a known variable star
01:23:28.70 +62:35:10.1 -- a known variable star
01:24:30.64 +59:38:48.6 -- a known variable star
01:25:39.69 +59:16:07.4 -- not a known variable star
01:25:43.43 +60:50:05.7 -- a known variable star
01:25:56.70 +62:14:49.4 -- a known variable star
01:26:01.01 +59:55:35.7 -- a known variable star
01:27:44.43 +62:06:40.7 -- a known variable star
01:28:36.28 +61:12:06.7 -- a known variable star
01:29:35.29 +65:02:04.9 -- a known variable star
01:30:50.42 +60:32:14.2 -- a known variable star
01:31:04.89 +57:13:14.0 -- a known variable star
01:31:28.19 +57:20:36.7 -- a known variable star
01:32:27.26 +60:20:31.1 -- a known variable star
01:32:44.39 +61:45:35.6 -- a known variable star
01:35:09.89 +60:17:10.6 -- a known variable star
01:35:57.20 +59:47:27.0 -- a known variable star
01:36:20.44 +58:31:43.2 -- a known variable star
01:36:21.66 +60:26:52.3 -- a known variable star
01:36:43.18 +61:14:25.3 -- a known variable star
01:36:47.30 +63:02:42.6 -- a known variable star
01:37:01.41 +61:15:57.1 -- a known variable star
01:38:21.64 +57:13:51.3 -- a known variable star
01:39:46.89 +59:42:30.5 -- a known variable star
01:40:46.01 +60:51:39.7 -- a known variable star
01:41:01.13 +61:31:00.7 -- a known variable star
01:41:34.22 +56:56:31.6 -- a known variable star
01:41:46.93 +59:03:48.0 -- a known variable star
01:43:02.78 +61:34:06.4 -- not a known variable star
01:43:36.46 +58:48:08.9 -- a known variable star
01:43:45.28 +58:23:45.8 -- a known variable star
01:43:58.28 +58:41:06.0 -- a known variable star
01:44:48.84 +59:53:34.1 -- a known variable star
01:45:16.05 +57:55:46.8 -- a known variable star
01:46:05.47 +60:59:36.6 -- a known variable star
01:46:35.86 +59:12:14.3 -- not a known variable star
01:47:07.73 +57:00:34.1 -- a known variable star
01:47:21.78 +58:08:40.5 -- a known variable star
01:47:43.89 +62:06:37.4 -- a known variable star
01:49:47.69 +65:03:21.3 -- a known variable star
01:50:36.43 +63:53:30.1 -- a known variable star
01:51:45.69 +65:36:52.8 -- a known variable star
01:52:19.54 +57:19:07.3 -- a known variable star
01:54:09.12 +61:13:07.0 -- a known variable star
01:54:12.35 +65:38:24.8 -- a known variable star
01:54:28.56 +57:17:51.0 -- a known variable star
01:55:07.62 +62:47:31.4 -- a known variable star
01:56:15.73 +60:01:03.3 -- a known variable star
01:56:16.77 +62:11:52.2 -- a known variable star
01:56:38.06 +59:15:34.2 -- a known variable star
01:57:52.45 +64:34:23.0 -- a known variable star
01:57:53.16 +63:48:41.1 -- a known variable star
02:00:13.56 +60:43:20.6 -- not a known variable star
02:00:14.31 +65:03:58.2 -- not a known variable star
02:00:17.58 +57:43:39.7 -- a known variable star
02:00:57.02 +58:36:59.3 -- a known variable star
02:01:05.84 +58:11:26.9 -- a known variable star
02:01:28.10 +58:18:15.0 -- a known variable star
02:02:39.14 +59:22:44.0 -- a known variable star
02:03:00.34 +58:36:13.4 -- a known variable star
02:03:07.41 +57:18:14.7 -- a known variable star
02:03:11.16 +62:07:52.0 -- not a known variable star
02:03:23.58 +57:43:21.9 -- a known variable star
02:03:34.92 +64:11:47.7 -- a known variable star
02:05:05.77 +58:16:24.6 -- a known variable star
02:05:50.44 +62:42:31.3 -- a known variable star
02:07:16.67 +60:08:10.8 -- a known variable star
02:07:21.55 +64:28:11.9 -- a known variable star
02:07:37.49 +62:22:07.0 -- a known variable star
02:07:46.89 +62:11:10.9 -- a known variable star
02:07:48.46 +61:22:16.5 -- a known variable star
02:08:15.60 +59:15:57.1 -- a known variable star
02:08:54.01 +58:42:29.5 -- a known variable star
02:09:24.81 +60:03:15.6 -- a known variable star
02:09:48.70 +59:51:47.0 -- not a known variable star
02:11:32.08 +65:25:28.2 -- a known variable star
02:11:34.44 +59:06:06.6 -- a known variable star
02:12:24.62 +63:16:01.2 -- a known variable star
02:13:08.99 +63:06:22.8 -- a known variable star
02:13:47.58 +63:11:26.0 -- a known variable star
02:14:26.77 +64:29:24.6 -- a known variable star
02:14:27.98 +64:44:14.9 -- a known variable star
02:14:45.13 +57:39:36.6 -- a known variable star
02:14:46.56 +57:37:03.4 -- a known variable star
02:15:20.43 +62:13:50.0 -- a known variable star
02:15:26.81 +62:47:45.7 -- a known variable star
02:15:35.96 +56:21:40.4 -- not a known variable star
02:16:28.46 +58:16:12.0 -- a known variable star
02:18:22.56 +58:47:09.8 -- a known variable star
02:18:24.04 +56:23:24.4 -- not a known variable star
02:18:24.73 +58:37:25.8 -- a known variable star
02:18:53.85 +57:08:41.8 -- a known variable star
02:19:04.00 +62:47:33.4 -- a known variable star
02:19:12.27 +57:48:50.2 -- a known variable star
02:19:16.53 +59:42:22.1 -- a known variable star
02:19:34.19 +58:23:57.9 -- a known variable star
02:19:36.15 +64:09:18.0 -- a known variable star
02:19:36.25 +56:23:22.4 -- a known variable star
02:19:44.52 +56:42:25.7 -- not a known variable star
02:19:45.31 +57:01:15.4 -- not a known variable star
02:19:52.90 +56:15:39.2 -- not a known variable star
02:19:59.14 +59:17:32.1 -- a known variable star
02:20:07.34 +56:27:53.6 -- not a known variable star
02:20:24.36 +56:41:46.0 -- a known variable star
02:20:33.64 +60:06:16.7 -- a known variable star
02:20:54.00 +56:16:37.9 -- a known variable star
02:21:04.81 +56:15:32.5 -- a known variable star
02:21:16.42 +57:08:40.1 -- not a known variable star
02:21:20.02 +61:23:53.5 -- a known variable star
02:21:34.70 +56:26:46.5 -- not a known variable star
02:21:40.62 +60:54:41.8 -- a known variable star
02:21:55.26 +56:25:09.3 -- not a known variable star
02:21:59.04 +56:30:02.2 -- a known variable star
02:22:04.64 +57:10:39.2 -- a known variable star
02:22:10.11 +56:24:22.8 -- not a known variable star
02:22:31.60 +56:14:10.7 -- a known variable star
02:22:32.05 +64:22:11.7 -- a known variable star
02:22:35.24 +56:18:15.4 -- not a known variable star
02:23:18.51 +64:21:47.0 -- a known variable star
02:23:38.25 +61:24:57.1 -- not a known variable star
02:24:05.02 +63:37:15.8 -- a known variable star
02:24:06.55 +56:30:01.1 -- not a known variable star
02:24:09.75 +56:34:02.5 -- not a known variable star
02:24:11.88 +56:35:43.2 -- not a known variable star
02:24:19.53 +64:16:12.9 -- a known variable star
02:24:19.74 +63:24:35.5 -- a known variable star
02:24:29.68 +59:24:31.5 -- a known variable star
02:24:34.96 +61:05:35.0 -- a known variable star
02:24:41.13 +58:22:35.6 -- a known variable star
02:24:41.97 +56:55:48.3 -- not a known variable star
02:24:46.68 +59:43:52.9 -- a known variable star
02:24:52.65 +56:43:13.3 -- not a known variable star
02:25:13.42 +56:30:32.3 -- not a known variable star
02:25:20.49 +56:12:13.5 -- not a known variable star
02:25:27.64 +56:46:55.8 -- not a known variable star
02:25:28.20 +56:11:20.2 -- not a known variable star
02:25:30.00 +56:16:55.3 -- a known variable star
02:25:34.10 +56:34:22.3 -- not a known variable star
02:25:42.03 +56:37:15.5 -- a known variable star
02:26:00.91 +56:46:18.9 -- not a known variable star
02:26:02.45 +56:20:59.5 -- not a known variable star
02:26:07.28 +56:25:11.5 -- not a known variable star
02:26:10.82 +56:48:29.2 -- not a known variable star
02:26:13.37 +56:36:45.1 -- not a known variable star
02:26:43.32 +56:24:14.7 -- not a known variable star
02:26:55.68 +56:30:21.4 -- not a known variable star
02:26:59.10 +56:01:58.1 -- not a known variable star
02:27:07.81 +56:33:54.6 -- not a known variable star
02:27:20.52 +56:01:48.8 -- not a known variable star
02:27:21.83 +62:38:26.5 -- a known variable star
02:27:22.97 +56:19:26.0 -- a known variable star
02:27:23.77 +60:40:47.8 -- a known variable star
02:27:24.36 +56:23:03.5 -- a known variable star
02:27:33.00 +56:13:09.5 -- not a known variable star
02:27:58.38 +56:02:38.8 -- not a known variable star
02:28:09.92 +56:10:50.3 -- not a known variable star
02:28:12.08 +64:31:52.8 -- a known variable star
02:28:12.53 +58:37:11.5 -- a known variable star
02:28:41.20 +56:12:06.5 -- a known variable star
02:28:49.65 +56:07:39.2 -- a known variable star
02:28:50.68 +56:20:50.4 -- not a known variable star
02:29:09.02 +56:37:12.7 -- not a known variable star
02:29:10.08 +56:27:14.1 -- not a known variable star
02:29:12.20 +56:18:00.7 -- not a known variable star
02:29:28.85 +56:33:09.5 -- a known variable star
02:29:33.40 +55:57:20.3 -- not a known variable star
02:29:39.44 +56:11:35.3 -- a known variable star
02:29:40.98 +56:18:42.4 -- not a known variable star
02:29:41.24 +56:20:06.8 -- not a known variable star
02:29:50.72 +56:19:10.9 -- not a known variable star
02:29:57.20 +56:36:49.0 -- not a known variable star
02:29:58.23 +56:08:53.2 -- not a known variable star
02:29:59.81 +56:13:02.8 -- not a known variable star
02:30:12.73 +56:11:27.6 -- a known variable star
02:30:16.58 +56:38:11.3 -- not a known variable star
02:30:30.72 +57:30:28.2 -- not a known variable star
02:30:33.01 +56:53:08.7 -- not a known variable star
02:30:37.35 +56:23:01.5 -- a known variable star
02:30:44.92 +56:56:13.4 -- not a known variable star
02:30:49.77 +56:11:02.6 -- not a known variable star
02:30:51.88 +57:04:10.0 -- not a known variable star
02:30:52.97 +56:54:21.1 -- a known variable star
02:30:54.10 +56:14:28.3 -- not a known variable star
02:30:58.99 +62:56:15.2 -- a known variable star
02:31:06.05 +56:37:19.1 -- not a known variable star
02:31:06.61 +56:30:44.0 -- not a known variable star
02:31:09.60 +57:16:15.9 -- not a known variable star
02:31:11.88 +57:09:48.4 -- not a known variable star
02:31:18.98 +55:53:51.0 -- not a known variable star
02:31:18.98 +56:20:50.6 -- not a known variable star
02:31:25.66 +60:43:53.6 -- a known variable star
02:31:26.05 +56:07:04.8 -- not a known variable star
02:31:26.37 +55:59:07.4 -- a known variable star
02:31:28.99 +57:11:53.7 -- not a known variable star
02:31:38.17 +56:33:35.0 -- a known variable star
02:31:38.51 +57:13:48.2 -- not a known variable star
02:31:46.08 +56:26:43.2 -- not a known variable star
02:31:46.25 +55:57:57.3 -- not a known variable star
02:31:51.85 +56:45:48.0 -- a known variable star
02:31:59.20 +56:42:22.0 -- not a known variable star
02:32:05.15 +56:49:22.4 -- not a known variable star
02:32:05.62 +57:22:03.9 -- not a known variable star
02:32:05.67 +56:39:57.3 -- not a known variable star
02:32:16.04 +56:38:48.1 -- not a known variable star
02:32:17.90 +57:17:10.0 -- a known variable star
02:32:18.76 +56:21:25.6 -- not a known variable star
02:32:26.23 +56:47:10.1 -- not a known variable star
02:32:40.32 +62:07:15.6 -- a known variable star
02:32:45.29 +57:08:07.3 -- not a known variable star
02:32:46.69 +56:48:22.9 -- not a known variable star
02:32:55.76 +56:39:38.1 -- not a known variable star
02:32:59.22 +57:28:35.8 -- not a known variable star
02:33:01.83 +57:02:06.6 -- a known variable star
02:33:03.14 +57:03:26.9 -- not a known variable star
02:33:05.67 +56:13:01.3 -- not a known variable star
02:33:09.48 +57:00:39.2 -- not a known variable star
02:33:13.67 +57:44:32.4 -- not a known variable star
02:33:23.67 +64:25:00.1 -- a known variable star
02:33:29.99 +57:42:17.0 -- a known variable star
02:33:31.95 +57:34:09.2 -- not a known variable star
02:33:35.26 +55:54:24.6 -- not a known variable star
02:33:37.63 +57:40:23.9 -- not a known variable star
02:33:40.04 +57:40:02.5 -- not a known variable star
02:33:47.87 +61:42:03.3 -- a known variable star
02:33:48.99 +57:01:45.0 -- not a known variable star
02:33:49.42 +57:35:11.7 -- a known variable star
02:34:04.70 +56:30:40.2 -- not a known variable star
02:34:05.16 +56:42:26.1 -- a known variable star
02:34:06.21 +56:25:27.6 -- not a known variable star
02:34:06.44 +56:37:23.7 -- not a known variable star
02:34:11.11 +55:49:59.2 -- a known variable star
02:34:24.43 +57:28:27.5 -- not a known variable star
02:34:26.97 +56:29:12.2 -- not a known variable star
02:34:32.44 +64:22:56.6 -- a known variable star
02:34:35.28 +56:21:51.3 -- not a known variable star
02:34:40.00 +63:00:03.4 -- a known variable star
02:34:44.75 +56:06:07.7 -- not a known variable star
02:35:04.79 +57:26:52.8 -- not a known variable star
02:35:08.80 +57:36:14.7 -- not a known variable star
02:35:18.58 +57:31:37.0 -- not a known variable star
02:35:20.47 +57:29:29.4 -- not a known variable star
02:35:30.33 +57:03:27.8 -- not a known variable star
02:35:34.11 +57:09:17.2 -- not a known variable star
02:35:38.10 +57:29:11.6 -- not a known variable star
02:35:43.04 +56:44:19.4 -- a known variable star
02:35:52.05 +57:47:21.5 -- not a known variable star
02:36:07.89 +57:21:40.2 -- not a known variable star
02:36:08.67 +57:39:33.5 -- not a known variable star
02:36:10.97 +60:22:42.0 -- a known variable star
02:36:19.99 +57:15:26.8 -- not a known variable star
02:36:22.57 +57:40:03.4 -- not a known variable star
02:36:29.15 +57:11:43.0 -- not a known variable star
02:36:33.17 +57:54:38.3 -- not a known variable star
02:36:35.17 +57:36:34.3 -- not a known variable star
02:36:36.23 +57:46:58.2 -- not a known variable star
02:36:56.79 +57:06:43.6 -- not a known variable star
02:36:59.24 +57:56:30.4 -- a known variable star
02:37:08.74 +57:25:19.6 -- not a known variable star
02:37:31.97 +57:28:17.7 -- not a known variable star
02:37:36.90 +57:51:16.6 -- not a known variable star
02:37:41.05 +57:33:20.1 -- not a known variable star
02:37:50.62 +57:45:48.2 -- not a known variable star
02:37:50.65 +57:54:15.4 -- not a known variable star
02:37:55.13 +57:39:02.3 -- not a known variable star
02:38:18.56 +57:37:39.8 -- not a known variable star
02:38:33.43 +61:54:31.0 -- a known variable star
02:38:46.94 +57:49:57.0 -- not a known variable star
02:39:22.81 +60:42:41.0 -- a known variable star
02:40:00.93 +58:49:46.1 -- a known variable star
02:40:07.39 +58:29:00.9 -- not a known variable star
02:41:04.44 +62:17:31.5 -- a known variable star
02:41:50.08 +65:30:27.2 -- not a known variable star
02:42:10.42 +61:03:22.2 -- a known variable star
02:43:44.79 +60:40:26.6 -- a known variable star
02:43:55.93 +64:48:54.7 -- a known variable star
02:45:57.12 +62:02:43.5 -- a known variable star
02:48:49.52 +64:11:51.9 -- a known variable star
Found 134 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
313 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 313 (excluding asteroids and hot pixels, 134 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
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461188.86142984 -observatory V36
05:25:37.38 +25:12:24.3 Mercury (-0.9mag)
06:47:17.26 +24:50:53.0 Venus (-3.9mag)
02:18:18.82 +13:07:13.2 Mars (1.3mag)
07:39:40.81 +21:52:32.7 Jupiter (-1.9mag)
00:46:01.94 +02:30:02.9 Saturn (0.9mag)
03:57:35.94 +20:17:52.4 Uranus (5.8mag)
00:15:24.15 +00:12:34.6 Neptune (7.8mag)
20:33:51.64 -23:00:45.5 Pluto (14.5mag)
13:56:23.73 -17:19:55.4 Moon (-11.8mag)
-rw-r--r-- 1 apache apache 363 May 28 03:44 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461188.86142984:
07:39:37.15 +21:52:44.6 Io (6.0mag)
07:39:38.12 +21:52:42.6 Europa (6.1mag)
07:39:59.22 +21:51:42.8 Ganymede (5.5mag)
07:39:11.15 +21:53:54.0 Callisto (6.7mag)
07:40:37.90 +21:28:45.0 Himalia (15.5mag)
07:39:45.24 +21:52:20.2 Thebe (16.5mag)
07:40:53.61 +21:49:03.0 Elara (17.5mag)
07:41:16.13 +22:10:07.4 Pasiphae (17.7mag)
07:46:42.88 +21:53:30.5 Carme (18.8mag)
00:46:12.10 +02:29:47.4 Titan (8.7mag)
00:46:07.50 +02:30:02.0 Rhea (10.0mag)
00:46:28.28 +02:30:33.8 Iapetus (11.4mag)
00:46:11.87 +02:30:22.1 Hyperion (14.7mag)
00:46:57.07 +02:33:31.7 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 28 03:44 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461188.86142984:
17:18:32.87 -33:48:04.8 JWST
10:40:00.47 +45:25:36.3 Chandra
09:13:52.10 -52:38:19.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 28 03:44 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461188.86142984 -observatory V36
13:19:02.40 -26:50:03.3 14.4mag D/1884 O1 (Barnard)
06:41:12.79 +30:36:44.2 15.7mag D/1886 K1 (Brooks)
15:24:17.65 +01:25:49.9 14.6mag D/1895 Q1 (Swift)
05:31:41.19 +24:43:25.2 17.2mag D/1918 W1 (Schorr)
09:46:27.81 +12:32:34.9 17.9mag P/2009 WX51 (Catalina)
18:49:58.23 -31:49:43.9 13.7mag P/2010 H2 (Vales)
05:42:57.53 -68:13:27.0 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:45:07.72 +31:50:01.4 17.5mag C/2017 K2 (PANSTARRS)
17:19:01.40 +14:42:13.8 17.7mag C/2021 G2 (ATLAS)
19:47:50.84 -51:35:53.4 17.9mag P/2021 N1 (ZTF)
23:14:21.33 +31:08:38.4 17.2mag C/2022 E2 (ATLAS)
05:20:42.15 +26:52:59.3 16.4mag C/2022 N2 (PANSTARRS)
09:22:20.77 +31:25:50.5 16.6mag C/2022 QE78 (ATLAS)
08:45:02.85 +03:21:01.4 17.6mag C/2022 R6 (PANSTARRS)
18:35:03.22 +21:17:28.1 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:23:33.10 -11:01:36.1 17.5mag P/2023 B1 (PANSTARRS)
22:16:14.64 +65:48:55.4 17.7mag C/2023 H5 (Lemmon)
18:12:12.46 -05:42:41.0 13.7mag C/2023 R1 (PANSTARRS)
13:33:10.62 +85:21:20.6 17.9mag C/2023 X2 (Lemmon)
06:56:07.67 +63:59:02.7 17.6mag C/2024 A1 (ATLAS)
06:30:23.50 +26:44:08.5 13.2mag C/2024 E1 (Wierzchos)
15:46:04.02 +12:27:12.9 17.3mag C/2024 G6 (ATLAS)
20:18:54.89 +27:50:43.7 14.1mag C/2024 J3 (ATLAS)
04:07:09.84 -16:58:45.3 16.1mag C/2024 T5 (ATLAS)
05:55:43.46 +36:24:59.5 17.9mag C/2025 J1 (Borisov)
11:43:11.75 +53:16:01.0 17.0mag C/2025 L1 (ATLAS)
06:29:02.05 -10:19:47.7 12.9mag C/2025 R3 (PANSTARRS)
12:40:37.03 +04:38:42.3 17.2mag C/2025 Y1 (ATLAS)
01:40:37.73 +42:34:15.6 15.8mag C/2026 B2 (Sun-Gao)
11:10:19.39 -08:00:46.2 16.3mag A/2026 E1
20:03:42.96 -08:08:28.7 9.3mag 10P/Tempel
14:17:51.67 -02:56:55.7 17.8mag 24P/Schaumasse
10:59:59.72 -00:52:16.4 15.9mag 29P/Schwassmann-Wachmann
10:52:47.66 -02:35:11.6 17.8mag 43P/Wolf-Harrington
02:54:52.07 +24:08:54.0 17.6mag 47P/Ashbrook-Jackson
08:36:52.99 +26:46:52.9 16.9mag 63P/Wild
00:17:00.87 -07:08:49.5 15.7mag 65P/Gunn
06:08:34.60 +32:02:11.9 16.6mag 76P/West-Kohoutek-Ikemura
02:43:09.60 +15:43:04.0 13.9mag 78P/Gehrels
00:56:17.64 +02:21:11.8 15.3mag 88P/Howell
04:19:45.79 +29:13:24.9 15.2mag 93P/Lovas
02:13:11.84 +25:45:25.5 17.9mag 114P/Wiseman-Skiff
06:25:02.46 +33:18:03.5 15.7mag 123P/West-Hartley
09:31:37.19 +19:19:03.7 16.4mag 124P/Mrkos
03:41:11.14 +18:27:45.0 16.4mag 128P/Shoemaker-Holt
04:11:56.25 +18:29:25.9 17.7mag 131P/Mueller
05:09:11.34 +19:33:40.7 13.3mag 141P/Machholz
05:11:44.43 +16:41:11.8 13.2mag 141P-A/Machholz
03:58:03.55 +14:13:09.2 10.7mag 141P-D/Machholz
02:49:49.32 -26:18:23.1 17.2mag 161P/Hartley-IRAS
03:06:43.71 +19:12:42.6 14.9mag 162P/SidingSpring
19:35:24.70 -01:11:01.4 17.4mag 169P/NEAT
23:48:52.92 +00:15:10.0 18.0mag 220P/McNaught
17:00:39.69 -09:10:44.7 16.3mag 235P/LINEAR
07:10:01.08 +35:49:32.5 17.4mag 240P/NEAT
00:04:10.38 -06:54:54.3 16.7mag 260P/McNaught
03:35:34.94 +30:22:32.6 17.6mag 295P/LINEAR
22:26:28.88 -24:38:18.1 17.6mag 320P/McNaught
15:20:34.73 +08:20:32.5 17.4mag 391P/Kowalski
07:58:48.98 +20:59:45.0 17.8mag 450P/LONEOS
06:42:18.36 +42:26:32.8 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 3.0K May 28 03:44 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -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
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
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
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
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 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -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
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
-rw-r--r-- 1 apache apache 5.6K May 28 03:44 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
-rw-r--r-- 1 apache apache 188K May 28 03:44 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
12:09:12.149 +41:27:00.14 AT 2026naw 2026-05-11.29 20.6337
06:25:45.633 -48:14:58.83 AT 2026nav 2026-05-04.02 18.255
06:58:22.644 -55:50:37.36 AT 2026nau 2026-05-18.96 18.984
08:46:46.014 +33:52:05.28 AT 2026nat 2026-05-17.28 19.023
10:01:59.220 +03:28:24.29 AT 2026nas 2026-05-16.99 23.35
08:33:18.216 +19:20:44.80 AT 2026nar 2026-05-18.88 19.333
12:51:56.463 +16:16:53.32 SN 2026naq 2026-05-19.19 19.6515
08:02:36.297 +15:58:21.39 AT 2026nap 2026-05-15.16 19.132
12:35:48.509 -01:02:49.40 AT 2026nao 2026-05-16.27 20.0531
11:46:27.658 +23:07:49.57 AT 2026nan 2026-05-08.18 20.1914
11:15:28.304 -01:08:27.49 AT 2026nam 2026-05-16.20 20.4814
02:05:49.697 -30:29:09.67 AT 2026nal 2026-05-18.43 15.4
12:23:18.242 +28:09:07.23 SN 2026nak 2026-05-18.88 19.67
13:47:06.036 +18:15:15.14 AT 2026naj 2026-05-17.91 19.77
15:46:38.025 -55:50:28.50 AT 2026nai 2026-05-17.00 19.04
11:40:58.130 +28:13:30.16 AT 2026nah 2026-05-17.94 19.877
23:21:04.257 +34:14:10.38 SN 2026nag 2026-05-13.19 18.36
14:12:48.859 +54:00:36.42 AT 2026naf 2026-05-18.36 18.96
09:57:42.622 +27:44:09.60 AT 2026nae 2026-05-17.90 20.056
00:31:01.441 -13:38:51.90 SN 2026nad 2026-05-18.40 15.715
-rw-r--r-- 1 apache apache 30K May 28 03:44 tns_transients_list.txt
